---
_id: '1075'
alternative_title:
- American Studies in Austria
author:
- first_name: Bernhard
full_name: Wenzl, Bernhard
id: 479E9046-F248-11E8-B48F-1D18A9856A87
last_name: Wenzl
citation:
ama: 'Wenzl B. An American in Allied-occupied Austria: John Dos Passos Reports on
"The Vienna Frontier" In: Parker J, Poole R, eds. Austria
and America: 20th-Century Cross-Cultural Encounters. Vol 15. LIT Verlag Berlin-Münster-Wien-Zürich-London;
2017:73-80.'
apa: 'Wenzl, B. (2017). An American in Allied-occupied Austria: John Dos Passos
Reports on "The Vienna Frontier" In J. Parker & R. Poole
(Eds.), Austria and America: 20th-Century Cross-Cultural Encounters (Vol.
15, pp. 73–80). LIT Verlag Berlin-Münster-Wien-Zürich-London.'
chicago: 'Wenzl, Bernhard. “An American in Allied-Occupied Austria: John Dos Passos
Reports on "The Vienna Frontier"” In Austria and America:
20th-Century Cross-Cultural Encounters, edited by Joshua Parker and Ralph
Poole, 15:73–80. LIT Verlag Berlin-Münster-Wien-Zürich-London, 2017.'
ieee: 'B. Wenzl, “An American in Allied-occupied Austria: John Dos Passos Reports
on "The Vienna Frontier",” in Austria and America: 20th-Century
Cross-Cultural Encounters, vol. 15, J. Parker and R. Poole, Eds. LIT Verlag
Berlin-Münster-Wien-Zürich-London, 2017, pp. 73–80.'
ista: 'Wenzl B. 2017.An American in Allied-occupied Austria: John Dos Passos Reports
on "The Vienna Frontier" In: Austria and America: 20th-Century
Cross-Cultural Encounters. American Studies in Austria, vol. 15, 73–80.'
mla: 'Wenzl, Bernhard. “An American in Allied-Occupied Austria: John Dos Passos
Reports on "The Vienna Frontier"” Austria and America: 20th-Century
Cross-Cultural Encounters, edited by Joshua Parker and Ralph Poole, vol. 15,
LIT Verlag Berlin-Münster-Wien-Zürich-London, 2017, pp. 73–80.'
short: 'B. Wenzl, in:, J. Parker, R. Poole (Eds.), Austria and America: 20th-Century
Cross-Cultural Encounters, LIT Verlag Berlin-Münster-Wien-Zürich-London, 2017,
pp. 73–80.'
date_created: 2018-12-11T11:50:00Z
date_published: 2017-02-01T00:00:00Z
date_updated: 2021-01-12T06:48:06Z
day: '01'
ddc:
- '001'
editor:
- first_name: Joshua
full_name: Parker, Joshua
last_name: Parker
- first_name: Ralph
full_name: Poole, Ralph
last_name: Poole
extern: '1'
file:
- access_level: open_access
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:08:06Z
date_updated: 2018-12-12T10:08:06Z
file_id: '4666'
file_name: IST-2017-732-v1+1_Austria_and_America_Cross-Cultural_Encounters.pdf
file_size: 380624
relation: main_file
file_date_updated: 2018-12-12T10:08:06Z
has_accepted_license: '1'
intvolume: ' 15'
language:
- iso: eng
month: '02'
oa: 1
oa_version: None
page: 73 - 80
publication: 'Austria and America: 20th-Century Cross-Cultural Encounters'
publication_identifier:
isbn:
- 978-3643908124
publication_status: published
publisher: LIT Verlag Berlin-Münster-Wien-Zürich-London
publist_id: '6306'
status: public
title: 'An American in Allied-occupied Austria: John Dos Passos Reports on "The
Vienna Frontier"'
type: book_chapter
user_id: 2EBD1598-F248-11E8-B48F-1D18A9856A87
volume: 15
year: '2017'
...
---
_id: '11066'
abstract:
- lang: eng
text: Recent studies have shown that a subset of nucleoporins (Nups) can detach
from the nuclear pore complex and move into the nuclear interior to regulate transcription.
One such dynamic Nup, called Nup98, has been implicated in gene activation in
healthy cells and has been shown to drive leukemogenesis when mutated in patients
with acute myeloid leukemia (AML). Here we show that in hematopoietic cells, Nup98
binds predominantly to transcription start sites to recruit the Wdr82–Set1A/COMPASS
(complex of proteins associated with Set1) complex, which is required for deposition
of the histone 3 Lys4 trimethyl (H3K4me3)-activating mark. Depletion of Nup98
or Wdr82 abolishes Set1A recruitment to chromatin and subsequently ablates H3K4me3
at adjacent promoters. Furthermore, expression of a Nup98 fusion protein implicated
in aggressive AML causes mislocalization of H3K4me3 at abnormal regions and up-regulation
of associated genes. Our findings establish a function of Nup98 in hematopoietic
gene activation and provide mechanistic insight into which Nup98 leukemic fusion
proteins promote AML.
article_processing_charge: No
article_type: original
author:
- first_name: Tobias M.
full_name: Franks, Tobias M.
last_name: Franks
- first_name: Asako
full_name: McCloskey, Asako
last_name: McCloskey
- first_name: Maxim Nikolaievich
full_name: Shokhirev, Maxim Nikolaievich
last_name: Shokhirev
- first_name: Chris
full_name: Benner, Chris
last_name: Benner
- first_name: Annie
full_name: Rathore, Annie
last_name: Rathore
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: Franks TM, McCloskey A, Shokhirev MN, Benner C, Rathore A, Hetzer M. Nup98
recruits the Wdr82–Set1A/COMPASS complex to promoters to regulate H3K4 trimethylation
in hematopoietic progenitor cells. Genes & Development. 2017;31(22):2222-2234.
doi:10.1101/gad.306753.117
apa: Franks, T. M., McCloskey, A., Shokhirev, M. N., Benner, C., Rathore, A., &
Hetzer, M. (2017). Nup98 recruits the Wdr82–Set1A/COMPASS complex to promoters
to regulate H3K4 trimethylation in hematopoietic progenitor cells. Genes &
Development. Cold Spring Harbor Laboratory. https://doi.org/10.1101/gad.306753.117
chicago: Franks, Tobias M., Asako McCloskey, Maxim Nikolaievich Shokhirev, Chris
Benner, Annie Rathore, and Martin Hetzer. “Nup98 Recruits the Wdr82–Set1A/COMPASS
Complex to Promoters to Regulate H3K4 Trimethylation in Hematopoietic Progenitor
Cells.” Genes & Development. Cold Spring Harbor Laboratory, 2017. https://doi.org/10.1101/gad.306753.117.
ieee: T. M. Franks, A. McCloskey, M. N. Shokhirev, C. Benner, A. Rathore, and M.
Hetzer, “Nup98 recruits the Wdr82–Set1A/COMPASS complex to promoters to regulate
H3K4 trimethylation in hematopoietic progenitor cells,” Genes & Development,
vol. 31, no. 22. Cold Spring Harbor Laboratory, pp. 2222–2234, 2017.
ista: Franks TM, McCloskey A, Shokhirev MN, Benner C, Rathore A, Hetzer M. 2017.
Nup98 recruits the Wdr82–Set1A/COMPASS complex to promoters to regulate H3K4 trimethylation
in hematopoietic progenitor cells. Genes & Development. 31(22), 2222–2234.
mla: Franks, Tobias M., et al. “Nup98 Recruits the Wdr82–Set1A/COMPASS Complex to
Promoters to Regulate H3K4 Trimethylation in Hematopoietic Progenitor Cells.”
Genes & Development, vol. 31, no. 22, Cold Spring Harbor Laboratory,
2017, pp. 2222–34, doi:10.1101/gad.306753.117.
short: T.M. Franks, A. McCloskey, M.N. Shokhirev, C. Benner, A. Rathore, M. Hetzer,
Genes & Development 31 (2017) 2222–2234.
date_created: 2022-04-07T07:45:59Z
date_published: 2017-12-21T00:00:00Z
date_updated: 2022-07-18T08:33:05Z
day: '21'
doi: 10.1101/gad.306753.117
extern: '1'
external_id:
pmid:
- '29269482'
intvolume: ' 31'
issue: '22'
keyword:
- Developmental Biology
- Genetics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1101/gad.306753.117
month: '12'
oa: 1
oa_version: Published Version
page: 2222-2234
pmid: 1
publication: Genes & Development
publication_identifier:
issn:
- 0890-9369
- 1549-5477
publication_status: published
publisher: Cold Spring Harbor Laboratory
quality_controlled: '1'
scopus_import: '1'
status: public
title: Nup98 recruits the Wdr82–Set1A/COMPASS complex to promoters to regulate H3K4
trimethylation in hematopoietic progenitor cells
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 31
year: '2017'
...
---
_id: '11067'
abstract:
- lang: eng
text: Neural progenitor cells (NeuPCs) possess a unique nuclear architecture that
changes during differentiation. Nucleoporins are linked with cell-type-specific
gene regulation, coupling physical changes in nuclear structure to transcriptional
output; but, whether and how they coordinate with key fate-determining transcription
factors is unclear. Here we show that the nucleoporin Nup153 interacts with Sox2
in adult NeuPCs, where it is indispensable for their maintenance and controls
neuronal differentiation. Genome-wide analyses show that Nup153 and Sox2 bind
and co-regulate hundreds of genes. Binding of Nup153 to gene promoters or transcriptional
end sites correlates with increased or decreased gene expression, respectively,
and inhibiting Nup153 expression alters open chromatin configurations at its target
genes, disrupts genomic localization of Sox2, and promotes differentiation in
vitro and a gliogenic fate switch in vivo. Together, these findings reveal that
nuclear structural proteins may exert bimodal transcriptional effects to control
cell fate.
article_processing_charge: No
article_type: original
author:
- first_name: Tomohisa
full_name: Toda, Tomohisa
last_name: Toda
- first_name: Jonathan Y.
full_name: Hsu, Jonathan Y.
last_name: Hsu
- first_name: Sara B.
full_name: Linker, Sara B.
last_name: Linker
- first_name: Lauren
full_name: Hu, Lauren
last_name: Hu
- first_name: Simon T.
full_name: Schafer, Simon T.
last_name: Schafer
- first_name: Jerome
full_name: Mertens, Jerome
last_name: Mertens
- first_name: Filipe V.
full_name: Jacinto, Filipe V.
last_name: Jacinto
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
- first_name: Fred H.
full_name: Gage, Fred H.
last_name: Gage
citation:
ama: Toda T, Hsu JY, Linker SB, et al. Nup153 interacts with Sox2 to enable bimodal
gene regulation and maintenance of neural progenitor cells. Cell Stem Cell.
2017;21(5):618-634.e7. doi:10.1016/j.stem.2017.08.012
apa: Toda, T., Hsu, J. Y., Linker, S. B., Hu, L., Schafer, S. T., Mertens, J., …
Gage, F. H. (2017). Nup153 interacts with Sox2 to enable bimodal gene regulation
and maintenance of neural progenitor cells. Cell Stem Cell. Elsevier. https://doi.org/10.1016/j.stem.2017.08.012
chicago: Toda, Tomohisa, Jonathan Y. Hsu, Sara B. Linker, Lauren Hu, Simon T. Schafer,
Jerome Mertens, Filipe V. Jacinto, Martin Hetzer, and Fred H. Gage. “Nup153 Interacts
with Sox2 to Enable Bimodal Gene Regulation and Maintenance of Neural Progenitor
Cells.” Cell Stem Cell. Elsevier, 2017. https://doi.org/10.1016/j.stem.2017.08.012.
ieee: T. Toda et al., “Nup153 interacts with Sox2 to enable bimodal gene
regulation and maintenance of neural progenitor cells,” Cell Stem Cell,
vol. 21, no. 5. Elsevier, p. 618–634.e7, 2017.
ista: Toda T, Hsu JY, Linker SB, Hu L, Schafer ST, Mertens J, Jacinto FV, Hetzer
M, Gage FH. 2017. Nup153 interacts with Sox2 to enable bimodal gene regulation
and maintenance of neural progenitor cells. Cell Stem Cell. 21(5), 618–634.e7.
mla: Toda, Tomohisa, et al. “Nup153 Interacts with Sox2 to Enable Bimodal Gene Regulation
and Maintenance of Neural Progenitor Cells.” Cell Stem Cell, vol. 21, no.
5, Elsevier, 2017, p. 618–634.e7, doi:10.1016/j.stem.2017.08.012.
short: T. Toda, J.Y. Hsu, S.B. Linker, L. Hu, S.T. Schafer, J. Mertens, F.V. Jacinto,
M. Hetzer, F.H. Gage, Cell Stem Cell 21 (2017) 618–634.e7.
date_created: 2022-04-07T07:46:12Z
date_published: 2017-11-02T00:00:00Z
date_updated: 2022-07-18T08:33:07Z
day: '02'
doi: 10.1016/j.stem.2017.08.012
extern: '1'
external_id:
pmid:
- '28919367'
intvolume: ' 21'
issue: '5'
keyword:
- Cell Biology
- Genetics
- Molecular Medicine
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1016/j.stem.2017.08.012
month: '11'
oa: 1
oa_version: Published Version
page: 618-634.e7
pmid: 1
publication: Cell Stem Cell
publication_identifier:
issn:
- 1934-5909
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Nup153 interacts with Sox2 to enable bimodal gene regulation and maintenance
of neural progenitor cells
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 21
year: '2017'
...
---
_id: '11065'
abstract:
- lang: eng
text: Premature aging disorders provide an opportunity to study the mechanisms that
drive aging. In Hutchinson-Gilford progeria syndrome (HGPS), a mutant form of
the nuclear scaffold protein lamin A distorts nuclei and sequesters nuclear proteins.
We sought to investigate protein homeostasis in this disease. Here, we report
a widespread increase in protein turnover in HGPS-derived cells compared to normal
cells. We determine that global protein synthesis is elevated as a consequence
of activated nucleoli and enhanced ribosome biogenesis in HGPS-derived fibroblasts.
Depleting normal lamin A or inducing mutant lamin A expression are each sufficient
to drive nucleolar expansion. We further show that nucleolar size correlates with
donor age in primary fibroblasts derived from healthy individuals and that ribosomal
RNA production increases with age, indicating that nucleolar size and activity
can serve as aging biomarkers. While limiting ribosome biogenesis extends lifespan
in several systems, we show that increased ribosome biogenesis and activity are
a hallmark of premature aging.
article_number: '328'
article_processing_charge: No
article_type: original
author:
- first_name: Abigail
full_name: Buchwalter, Abigail
last_name: Buchwalter
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: Buchwalter A, Hetzer M. Nucleolar expansion and elevated protein translation
in premature aging. Nature Communications. 2017;8. doi:10.1038/s41467-017-00322-z
apa: Buchwalter, A., & Hetzer, M. (2017). Nucleolar expansion and elevated protein
translation in premature aging. Nature Communications. Springer Nature.
https://doi.org/10.1038/s41467-017-00322-z
chicago: Buchwalter, Abigail, and Martin Hetzer. “Nucleolar Expansion and Elevated
Protein Translation in Premature Aging.” Nature Communications. Springer
Nature, 2017. https://doi.org/10.1038/s41467-017-00322-z.
ieee: A. Buchwalter and M. Hetzer, “Nucleolar expansion and elevated protein translation
in premature aging,” Nature Communications, vol. 8. Springer Nature, 2017.
ista: Buchwalter A, Hetzer M. 2017. Nucleolar expansion and elevated protein translation
in premature aging. Nature Communications. 8, 328.
mla: Buchwalter, Abigail, and Martin Hetzer. “Nucleolar Expansion and Elevated Protein
Translation in Premature Aging.” Nature Communications, vol. 8, 328, Springer
Nature, 2017, doi:10.1038/s41467-017-00322-z.
short: A. Buchwalter, M. Hetzer, Nature Communications 8 (2017).
date_created: 2022-04-07T07:45:50Z
date_published: 2017-08-30T00:00:00Z
date_updated: 2022-07-18T08:33:03Z
day: '30'
doi: 10.1038/s41467-017-00322-z
extern: '1'
external_id:
pmid:
- '28855503'
intvolume: ' 8'
keyword:
- General Physics and Astronomy
- General Biochemistry
- Genetics and Molecular Biology
- General Chemistry
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1038/s41467-017-00322-z
month: '08'
oa: 1
oa_version: Published Version
pmid: 1
publication: Nature Communications
publication_identifier:
issn:
- 2041-1723
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Nucleolar expansion and elevated protein translation in premature aging
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 8
year: '2017'
...
---
_id: '11518'
abstract:
- lang: eng
text: "We present spectroscopic follow-up observations of CR7 with ALMA, targeted
at constraining the infrared (IR) continuum and [C II]158 mm line-emission at
high spatial resolution matched to the HST/WFC3 imaging. CR7 is a luminous Lyα
emitting galaxy at z = 6.6 that consists of three separated UV-continuum components.
Our observations reveal several well-separated components of [C II] emission.
The two most luminous components in [C II] coincide with the brightest UV components
(A and B), blueshifted by »150 km s−1 with respect to the\r\npeak of Lyα emission.
Other [C II] components are observed close to UV clumps B and C and are blueshifted
by »300 and ≈80 km s−1 with respect to the systemic redshift. We do not detect
FIR continuum emission due to dust with a 3σ limiting luminosity LIR T L d 35
K 3.1 10 = <´ 10 ( ) . This allows us to mitigate uncertainties in the dust-corrected
SFR and derive SFRs for the three UV clumps A, B, and C of 28, 5, and 7 M yr−1.
All clumps have [C II] luminosities consistent within the scatter observed in
the local relation between SFR and L[ ] C II , implying that strong Lyα emission
does not necessarily anti-correlate with [C II] luminosity. Combining\r\nour measurements
with the literature, we show that galaxies with blue UV slopes have weaker [C
II] emission at fixed SFR, potentially due to their lower metallicities and/or
higher photoionization. Comparison with hydrodynamical simulations suggests that
CR7ʼs clumps have metallicities of 0.1 Z Z 0.2 < < . The observed ISM structure
of CR7 indicates that we are likely witnessing the build up of a central galaxy
in the early universe through complex accretion of satellites."
acknowledgement: 'We thank the referee for their constructive comments, which have
helped improve the quality and clarity of this work. We thank Raffaella Schneider
for comments on an earlier version of this paper. We thank Leindert Boogaard, Steven
Bos, Rychard Bouwens, and Renske Smit for discussions. J.M. acknowledges the support
of a Huygens PhD fellowship from Leiden University. D.S. acknowledges financial
support from the Netherlands Organisation for Scientific research (NWO) through
a Veni fellowship and from Lancaster University through an Early Career Internal
Grant A100679. A.F. acknowledges support from the ERC Advanced Grant INTERSTELLAR
H2020/740120. B.D. acknowledges financial support from NASA through the Astrophysics
Data Analysis Program (ADAP), grant number NNX12AE20G. Based on observations made
with ESO Telescopes at the La Silla Paranal Observatory under programme ID 294.A-5018.
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.00122.S. ALMA
is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan),
together with NRC (Canada) and NSC and ASIAA (Taiwan), and KASI (Republic of Korea),
in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated
by ESO, AUI/NRAO, and NAOJ.'
article_number: '145'
article_processing_charge: No
article_type: original
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: D.
full_name: Sobral, D.
last_name: Sobral
- first_name: F.
full_name: Boone, F.
last_name: Boone
- first_name: H.
full_name: Röttgering, H.
last_name: Röttgering
- first_name: D.
full_name: Schaerer, D.
last_name: Schaerer
- first_name: M.
full_name: Girard, M.
last_name: Girard
- first_name: A.
full_name: Pallottini, A.
last_name: Pallottini
- first_name: L.
full_name: Vallini, L.
last_name: Vallini
- first_name: A.
full_name: Ferrara, A.
last_name: Ferrara
- first_name: B.
full_name: Darvish, B.
last_name: Darvish
- first_name: B.
full_name: Mobasher, B.
last_name: Mobasher
citation:
ama: Matthee JJ, Sobral D, Boone F, et al. ALMA reveals metals yet no dust within
multiple components in CR7. The Astrophysical Journal. 2017;851(2). doi:10.3847/1538-4357/aa9931
apa: Matthee, J. J., Sobral, D., Boone, F., Röttgering, H., Schaerer, D., Girard,
M., … Mobasher, B. (2017). ALMA reveals metals yet no dust within multiple components
in CR7. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/aa9931
chicago: Matthee, Jorryt J, D. Sobral, F. Boone, H. Röttgering, D. Schaerer, M.
Girard, A. Pallottini, et al. “ALMA Reveals Metals yet No Dust within Multiple
Components in CR7.” The Astrophysical Journal. IOP Publishing, 2017. https://doi.org/10.3847/1538-4357/aa9931.
ieee: J. J. Matthee et al., “ALMA reveals metals yet no dust within multiple
components in CR7,” The Astrophysical Journal, vol. 851, no. 2. IOP Publishing,
2017.
ista: Matthee JJ, Sobral D, Boone F, Röttgering H, Schaerer D, Girard M, Pallottini
A, Vallini L, Ferrara A, Darvish B, Mobasher B. 2017. ALMA reveals metals yet
no dust within multiple components in CR7. The Astrophysical Journal. 851(2),
145.
mla: Matthee, Jorryt J., et al. “ALMA Reveals Metals yet No Dust within Multiple
Components in CR7.” The Astrophysical Journal, vol. 851, no. 2, 145, IOP
Publishing, 2017, doi:10.3847/1538-4357/aa9931.
short: J.J. Matthee, D. Sobral, F. Boone, H. Röttgering, D. Schaerer, M. Girard,
A. Pallottini, L. Vallini, A. Ferrara, B. Darvish, B. Mobasher, The Astrophysical
Journal 851 (2017).
date_created: 2022-07-07T08:48:04Z
date_published: 2017-12-21T00:00:00Z
date_updated: 2022-08-18T10:23:35Z
day: '21'
doi: 10.3847/1538-4357/aa9931
extern: '1'
external_id:
arxiv:
- '1709.06569'
intvolume: ' 851'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- dark ages
- reionization
- 'first stars – galaxies: formation – galaxies: high-redshift – galaxies: ISM – galaxies:
kinematics and dynamics'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1709.06569
month: '12'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: ALMA reveals metals yet no dust within multiple components in CR7
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 851
year: '2017'
...
---
_id: '11562'
abstract:
- lang: eng
text: We present the CAlibrating LYMan-α with Hα (CALYMHA) pilot survey and new
results on Lyman α (Lyα) selected galaxies at z ∼ 2. We use a custom-built Lyα
narrow-band filter at the Isaac Newton Telescope, designed to provide a matched
volume coverage to the z = 2.23 Hα HiZELS survey. Here, we present the first results
for the COSMOS and UDS fields. Our survey currently reaches a 3σ line flux limit
of ∼4 × 10−17 erg s−1 cm−2, and a Lyα luminosity limit of ∼1042.3 erg s−1. We
find 188 Lyα emitters over 7.3 × 105 Mpc3, but also find significant numbers of
other line-emitting sources corresponding to He II, C III] and C IV emission lines.
These sources are important contaminants, and we carefully remove them, unlike
most previous studies. We find that the Lyα luminosity function at z = 2.23 is
very well described by a Schechter function up to LLy α ≈ 1043 erg s−1 with L∗=1042.59+0.16−0.08
erg s−1, ϕ∗=10−3.09+0.14−0.34 Mpc−3 and α = −1.75 ± 0.25. Above LLy α ≈ 1043 erg
s−1, the Lyα luminosity function becomes power-law like, driven by X-ray AGN.
We find that Lyα-selected emitters have a high escape fraction of 37 ± 7 per cent,
anticorrelated with Lyα luminosity and correlated with Lyα equivalent width. Lyα
emitters have ubiquitous large (≈40 kpc) Lyα haloes, ∼2 times larger than their
Hα extents. By directly comparing our Lyα and Hα luminosity functions, we find
that the global/overall escape fraction of Lyα photons (within a 13 kpc radius)
from the full population of star-forming galaxies is 5.1 ± 0.2 per cent at the
peak of the star formation history. An extra 3.3 ± 0.3 per cent of Lyα photons
likely still escape, but at larger radii.
acknowledgement: 'We thank the reviewer for his/her helpful comments and suggestions
that have greatly improved this work. DS and JM acknowledge financial support from
the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship.
DS also acknowledges funding from FCT through an FCT Investigator Starting Grant
and Start-up Grant (IF/01154/2012/CP0189/CT0010). PNB is grateful for support from
the UK STFC via grant ST/M001229/1. IRS acknowledges support from STFC (ST/L00075X/1),
the ERC Advanced Investigator programme DUSTYGAL 321334 and a Royal Society/Wolfson
merit award. We thank Matthew Hayes, Ryan Trainor, Kimihiko Nakajima and Anne Verhamme
for many helpful discussions and Ana Sobral, Carolina Duarte and Miguel Domingos
for taking part in observations with the NB392 filter. We also thank Sergio Santos
for helpful comments. This research is based on observations obtained on the Isaac
Newton Telescope (INT), programs: I13AN002, I14AN002, 088-INT7/14A, I14BN006, 118-INT13/14B
& I15AN008. The authors acknowledge the award of time from programmes: I13AN002,
I14AN002, 088-INT7/14A, I14BN006, 118-INT13/14B, I15AN008 on the INT. INT is operated
on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio
del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Based on
observations made with ESO Telescopes at the La Silla Paranal Observatory under
programme ID 098.A 0819. We have benefited greatly from the publicly available programming
language PYTHON, including the NUMPY, MATPLOTLIB, PYFITS, SCIPY and ASTROPY packages,
the astronomical imaging tools SEXTRACTOR, SWARP (Bertin & Arnouts 1996; Bertin
2010), SCAMP (Bertin 2006) and TOPCAT (Taylor 2005). Dedicated to the memory of
M. L. Nicolau and M. C. Serrano.'
article_processing_charge: No
article_type: original
author:
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Philip
full_name: Best, Philip
last_name: Best
- first_name: Andra
full_name: Stroe, Andra
last_name: Stroe
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
- first_name: Iván
full_name: Oteo, Iván
last_name: Oteo
- first_name: Ian
full_name: Smail, Ian
last_name: Smail
- first_name: Leah
full_name: Morabito, Leah
last_name: Morabito
- first_name: Ana
full_name: Paulino-Afonso, Ana
last_name: Paulino-Afonso
citation:
ama: 'Sobral D, Matthee JJ, Best P, et al. The CALYMHA survey: Lyα luminosity function
and global escape fraction of Lyα photons at z = 2.23. Monthly Notices of the
Royal Astronomical Society. 2017;466(1):1242-1258. doi:10.1093/mnras/stw3090'
apa: 'Sobral, D., Matthee, J. J., Best, P., Stroe, A., Röttgering, H., Oteo, I.,
… Paulino-Afonso, A. (2017). The CALYMHA survey: Lyα luminosity function and global
escape fraction of Lyα photons at z = 2.23. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stw3090'
chicago: 'Sobral, David, Jorryt J Matthee, Philip Best, Andra Stroe, Huub Röttgering,
Iván Oteo, Ian Smail, Leah Morabito, and Ana Paulino-Afonso. “The CALYMHA Survey:
Lyα Luminosity Function and Global Escape Fraction of Lyα Photons at z = 2.23.”
Monthly Notices of the Royal Astronomical Society. Oxford University Press,
2017. https://doi.org/10.1093/mnras/stw3090.'
ieee: 'D. Sobral et al., “The CALYMHA survey: Lyα luminosity function and
global escape fraction of Lyα photons at z = 2.23,” Monthly Notices of the
Royal Astronomical Society, vol. 466, no. 1. Oxford University Press, pp.
1242–1258, 2017.'
ista: 'Sobral D, Matthee JJ, Best P, Stroe A, Röttgering H, Oteo I, Smail I, Morabito
L, Paulino-Afonso A. 2017. The CALYMHA survey: Lyα luminosity function and global
escape fraction of Lyα photons at z = 2.23. Monthly Notices of the Royal Astronomical
Society. 466(1), 1242–1258.'
mla: 'Sobral, David, et al. “The CALYMHA Survey: Lyα Luminosity Function and Global
Escape Fraction of Lyα Photons at z = 2.23.” Monthly Notices of the Royal Astronomical
Society, vol. 466, no. 1, Oxford University Press, 2017, pp. 1242–58, doi:10.1093/mnras/stw3090.'
short: D. Sobral, J.J. Matthee, P. Best, A. Stroe, H. Röttgering, I. Oteo, I. Smail,
L. Morabito, A. Paulino-Afonso, Monthly Notices of the Royal Astronomical Society
466 (2017) 1242–1258.
date_created: 2022-07-12T12:04:16Z
date_published: 2017-04-01T00:00:00Z
date_updated: 2022-08-19T07:18:20Z
day: '01'
doi: 10.1093/mnras/stw3090
extern: '1'
external_id:
arxiv:
- '1609.05897'
intvolume: ' 466'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: haloes'
- 'galaxies: high-redshift'
- 'galaxies: luminosity function'
- mass function
- 'galaxies: statistics'
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1609.05897
month: '04'
oa: 1
oa_version: Preprint
page: 1242-1258
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The CALYMHA survey: Lyα luminosity function and global escape fraction of
Lyα photons at z = 2.23'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 466
year: '2017'
...
---
_id: '11566'
abstract:
- lang: eng
text: While traditionally associated with active galactic nuclei (AGN), the properties
of the C II] (λ = 2326 Å), C III] (λ, λ = 1907, 1909 Å) and C IV (λ, λ = 1549,
1551 Å) emission lines are still uncertain as large, unbiased samples of sources
are scarce. We present the first blind, statistical study of C II], C III] and
C IV emitters at z ∼ 0.68, 1.05, 1.53, respectively, uniformly selected down to
a flux limit of ∼4 × 10−17 erg s−1 cm−1 through a narrow-band survey covering
an area of ∼1.4 deg2 over COSMOS and UDS. We detect 16 C II], 35 C III] and 17
C IV emitters, whose nature we investigate using optical colours as well as Hubble
Space Telescope (HST), X-ray, radio and far-infrared data. We find that z ∼ 0.7
C II] emitters are consistent with a mixture of blue (UV slope β = −2.0 ± 0.4)
star-forming (SF) galaxies with discy HST structure and AGN with Seyfert-like
morphologies. Bright C II] emitters have individual X-ray detections as well as
high average black hole accretion rates (BHARs) of ∼0.1 M⊙ yr−1. C III] emitters
at z ∼ 1.05 trace a general population of SF galaxies, with β = −0.8 ± 1.1, a
variety of optical morphologies, including isolated and interacting galaxies and
low BHAR (<0.02 M⊙ yr−1). Our C IV emitters at z ∼ 1.5 are consistent with young,
blue quasars (β ∼ −1.9) with point-like optical morphologies, bright X-ray counterparts
and large BHAR (0.8 M⊙ yr−1). We also find some surprising C II], C III] and
C IV emitters with rest-frame equivalent widths (EWs) that could be as large as
50–100 Å. AGN or spatial offsets between the UV continuum stellar disc and the
line-emitting regions may explain the large EW. These bright C II], C III] and
C IV emitters are ideal candidates for spectroscopic follow-up to fully unveil
their nature.
acknowledgement: 'We would like to thank the anonymous referee for her/his valuable
input that helped improve the clarity and interpretation of our results. DS acknowledges
financial support from the Netherlands Organisation for Scientific research (NWO),
through a Veni fellowship. IO acknowledges support from the European Research Council
in the form of the Advanced Investigator Programme, 321302, COSMICISM. CALYMHA data
are based on observations made with the Isaac Newton Telescope (proposals 13AN002,
I14AN002, 088-INT7/14A, I14BN006, 118-INT13/14B, I15AN008) operated on the island
of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los
Muchachos of the Instituto de Astrofísica de Canarias. Also based on data products
from observations made with ESO Telescopes at the La Silla Paranal Observatory under
ESO programme IDs 098.A-0819 and 179.A-2005. We are grateful to E. L. Wright and
J. Schombert for their cosmology calculator. We would like to thank the authors
of NUMPY (van der Walt et al. 2011), SCIPY (Jones et al. 2001), MATPLOTLIB (Hunter
2007) and ASTROPY (Astropy Collaboration et al. 2013) for making these packages
publicly available. This research has made use of the NASA/IPAC Extragalactic Database
(NED), which is '
article_processing_charge: No
article_type: original
author:
- first_name: Andra
full_name: Stroe, Andra
last_name: Stroe
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: João
full_name: Calhau, João
last_name: Calhau
- first_name: Ivan
full_name: Oteo, Ivan
last_name: Oteo
citation:
ama: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. A 1.4 deg2 blind survey for
C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and equivalent
widths . Monthly Notices of the Royal Astronomical Society. 2017;471(3):2558-2574.
doi:10.1093/mnras/stx1712
apa: Stroe, A., Sobral, D., Matthee, J. J., Calhau, J., & Oteo, I. (2017). A
1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies
and equivalent widths . Monthly Notices of the Royal Astronomical Society.
Oxford University Press. https://doi.org/10.1093/mnras/stx1712
chicago: Stroe, Andra, David Sobral, Jorryt J Matthee, João Calhau, and Ivan Oteo.
“A 1.4 Deg2 Blind Survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature,
Morphologies and Equivalent Widths .” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1712.
ieee: A. Stroe, D. Sobral, J. J. Matthee, J. Calhau, and I. Oteo, “A 1.4 deg2 blind
survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and
equivalent widths ,” Monthly Notices of the Royal Astronomical Society,
vol. 471, no. 3. Oxford University Press, pp. 2558–2574, 2017.
ista: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. 2017. A 1.4 deg2 blind survey
for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and equivalent
widths . Monthly Notices of the Royal Astronomical Society. 471(3), 2558–2574.
mla: Stroe, Andra, et al. “A 1.4 Deg2 Blind Survey for C II], C III] and C IV at
z ∼ 0.7–1.5 – I. Nature, Morphologies and Equivalent Widths .” Monthly Notices
of the Royal Astronomical Society, vol. 471, no. 3, Oxford University Press,
2017, pp. 2558–74, doi:10.1093/mnras/stx1712.
short: A. Stroe, D. Sobral, J.J. Matthee, J. Calhau, I. Oteo, Monthly Notices of
the Royal Astronomical Society 471 (2017) 2558–2574.
date_created: 2022-07-12T12:33:16Z
date_published: 2017-11-01T00:00:00Z
date_updated: 2022-08-19T07:59:57Z
day: '01'
doi: 10.1093/mnras/stx1712
extern: '1'
external_id:
arxiv:
- '1703.10169'
intvolume: ' 471'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: active'
- 'galaxies: high-redshift'
- 'quasars: emission lines'
- 'galaxies: star formation'
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1703.10169
month: '11'
oa: 1
oa_version: Preprint
page: 2558-2574
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'A 1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature,
morphologies and equivalent widths '
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '11564'
abstract:
- lang: eng
text: We study the production rate of ionizing photons of a sample of 588 Hα emitters
(HAEs) and 160 Lyman-α emitters (LAEs) at z = 2.2 in the COSMOS field in order
to assess the implied emissivity from galaxies, based on their ultraviolet (UV)
luminosity. By exploring the rest-frame Lyman Continuum (LyC) with GALEX/NUV data,
we find fesc < 2.8 (6.4) per cent through median (mean) stacking. By combining
the Hα luminosity density with intergalactic medium emissivity measurements from
absorption studies, we find a globally averaged 〈fesc〉 of 5.9+14.5−4.2 per cent
at z = 2.2 if we assume HAEs are the only source of ionizing photons. We find
similarly low values of the global 〈fesc〉 at z ≈ 3–5, also ruling out a high 〈fesc〉
at z < 5. These low escape fractions allow us to measure ξion, the number of produced
ionizing photons per unit UV luminosity, and investigate how this depends on galaxy
properties. We find a typical ξion ≈ 1024.77 ± 0.04 Hz erg−1 for HAEs and ξion
≈ 1025.14 ± 0.09 Hz erg−1 for LAEs. LAEs and low-mass HAEs at z = 2.2 show similar
values of ξion as typically assumed in the reionization era, while the typical
HAE is three times less ionizing. Due to an increasing ξion with increasing EW(Hα),
ξion likely increases with redshift. This evolution alone is fully in line with
the observed evolution of ξion between z ≈ 2 and 5, indicating a typical value
of ξion ≈ 1025.4 Hz erg−1 in the reionization era.
acknowledgement: "We thank the referee for the many helpful and constructive comments
which have significantly improved this paper. JM acknowledges the support of a Huygens
PhD fellowship from Leiden University. DS acknowledges financial support from the
Netherlands Organization for Scientific research (NWO) through a Veni fellowship
and from FCT through an FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010).
PNB is grateful for support from the UK STFC via grant ST/M001229/1. IO acknowledges
support from the European Research Council in the form of the Advanced Investigator
Programme, 321302, COSMICISM. The authors thank Andreas Faisst, Michael Rutkowski
and Andreas Sandberg for answering questions related to this work and Daniel Schaerer
and Mark Dijkstra for discussions. We acknowledge the work that has been done by
both the COSMOS team in assembling such large, state-of-the-art multi-wavelength
data set, as this has been crucial for the results presented in this paper. We have
benefited greatly from the public available programming language PYTHON, including
the NUMPY, MATPLOTLIB, PYFITS, SCIPY (Jones et al. 2001; Hunter 2007; Van Der Walt,
Colbert & Varoquaux 2011) and ASTROPY (Astropy Collaboration et al. 2013) packages,
the astronomical imaging tools SEXTRACTOR and SWARP (Bertin & Arnouts 1996;\r\nBertin
2010) and the TOPCAT analysis program (Taylor 2013)."
article_processing_charge: No
article_type: original
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Philip
full_name: Best, Philip
last_name: Best
- first_name: Ali Ahmad
full_name: Khostovan, Ali Ahmad
last_name: Khostovan
- first_name: Iván
full_name: Oteo, Iván
last_name: Oteo
- first_name: Rychard
full_name: Bouwens, Rychard
last_name: Bouwens
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
citation:
ama: Matthee JJ, Sobral D, Best P, et al. The production and escape of Lyman-Continuum
radiation from star-forming galaxies at z ∼ 2 and their redshift evolution. Monthly
Notices of the Royal Astronomical Society. 2017;465(3):3637-3655. doi:10.1093/mnras/stw2973
apa: Matthee, J. J., Sobral, D., Best, P., Khostovan, A. A., Oteo, I., Bouwens,
R., & Röttgering, H. (2017). The production and escape of Lyman-Continuum
radiation from star-forming galaxies at z ∼ 2 and their redshift evolution. Monthly
Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stw2973
chicago: Matthee, Jorryt J, David Sobral, Philip Best, Ali Ahmad Khostovan, Iván
Oteo, Rychard Bouwens, and Huub Röttgering. “The Production and Escape of Lyman-Continuum
Radiation from Star-Forming Galaxies at z ∼ 2 and Their Redshift Evolution.” Monthly
Notices of the Royal Astronomical Society. Oxford University Press, 2017.
https://doi.org/10.1093/mnras/stw2973.
ieee: J. J. Matthee et al., “The production and escape of Lyman-Continuum
radiation from star-forming galaxies at z ∼ 2 and their redshift evolution,” Monthly
Notices of the Royal Astronomical Society, vol. 465, no. 3. Oxford University
Press, pp. 3637–3655, 2017.
ista: Matthee JJ, Sobral D, Best P, Khostovan AA, Oteo I, Bouwens R, Röttgering
H. 2017. The production and escape of Lyman-Continuum radiation from star-forming
galaxies at z ∼ 2 and their redshift evolution. Monthly Notices of the Royal Astronomical
Society. 465(3), 3637–3655.
mla: Matthee, Jorryt J., et al. “The Production and Escape of Lyman-Continuum Radiation
from Star-Forming Galaxies at z ∼ 2 and Their Redshift Evolution.” Monthly
Notices of the Royal Astronomical Society, vol. 465, no. 3, Oxford University
Press, 2017, pp. 3637–55, doi:10.1093/mnras/stw2973.
short: J.J. Matthee, D. Sobral, P. Best, A.A. Khostovan, I. Oteo, R. Bouwens, H.
Röttgering, Monthly Notices of the Royal Astronomical Society 465 (2017) 3637–3655.
date_created: 2022-07-12T12:12:14Z
date_published: 2017-03-01T00:00:00Z
date_updated: 2022-08-19T07:53:04Z
day: '01'
doi: 10.1093/mnras/stw2973
extern: '1'
external_id:
arxiv:
- '1605.08782'
intvolume: ' 465'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: high-redshift'
- 'cosmology: observations'
- dark ages
- reionization
- first stars
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1605.08782
month: '03'
oa: 1
oa_version: Preprint
page: 3637-3655
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: The production and escape of Lyman-Continuum radiation from star-forming galaxies
at z ∼ 2 and their redshift evolution
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 465
year: '2017'
...
---
_id: '11567'
abstract:
- lang: eng
text: Recently, the C III] and C IV emission lines have been observed in galaxies
in the early Universe (z > 5), providing new ways to measure their redshift and
study their stellar populations and active galactic nuclei (AGN). We explore the
first blind C II], C III] and C IV survey (z ∼ 0.68, 1.05, 1.53, respectively)
presented in Stroe et al. (2017). We derive luminosity functions (LF) and study
properties of C II], C III] and C IV line emitters through comparisons to the
LFs of H α and Ly α emitters, UV selected star-forming (SF) galaxies and quasars
at similar redshifts. The C II] LF at z ∼ 0.68 is equally well described by a
Schechter or a power-law LF, characteristic of a mixture of SF and AGN activity.
The C III] LF (z ∼ 1.05) is consistent to a scaled down version of the Schechter
H α and Ly α LF at their redshift, indicating a SF origin. In stark contrast,
the C IV LF at z ∼ 1.53 is well fit by a power-law, quasar-like LF. We find that
the brightest UV sources (MUV < −22) will universally have C III] and C IV emission.
However, on average, C III] and C IV are not as abundant as H α or Ly α emitters
at the same redshift, with cosmic average ratios of ∼0.02–0.06 to H α and ∼0.01–0.1
to intrinsic Ly α. We predict that the C III] and C IV lines can only be truly
competitive in confirming high-redshift candidates when the hosts are intrinsically
bright and the effective Ly α escape fraction is below 1 per cent. While C III]
and C IV were proposed as good tracers of young, relatively low-metallicity galaxies
typical of the early Universe, we find that, at least at z ∼ 1.5, C IV is exclusively
hosted by AGN/quasars, especially at large line equivalent widths.
article_processing_charge: No
article_type: original
author:
- first_name: Andra
full_name: Stroe, Andra
last_name: Stroe
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: João
full_name: Calhau, João
last_name: Calhau
- first_name: Ivan
full_name: Oteo, Ivan
last_name: Oteo
citation:
ama: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. A 1.4 deg2 blind survey for
C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity functions and cosmic average
line ratios. Monthly Notices of the Royal Astronomical Society. 2017;471(3):2575-2586.
doi:10.1093/mnras/stx1713
apa: Stroe, A., Sobral, D., Matthee, J. J., Calhau, J., & Oteo, I. (2017). A
1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity
functions and cosmic average line ratios. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stx1713
chicago: Stroe, Andra, David Sobral, Jorryt J Matthee, João Calhau, and Ivan Oteo.
“A 1.4 Deg2 Blind Survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity
Functions and Cosmic Average Line Ratios.” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1713.
ieee: A. Stroe, D. Sobral, J. J. Matthee, J. Calhau, and I. Oteo, “A 1.4 deg2 blind
survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity functions and
cosmic average line ratios,” Monthly Notices of the Royal Astronomical Society,
vol. 471, no. 3. Oxford University Press, pp. 2575–2586, 2017.
ista: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. 2017. A 1.4 deg2 blind survey
for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity functions and cosmic
average line ratios. Monthly Notices of the Royal Astronomical Society. 471(3),
2575–2586.
mla: Stroe, Andra, et al. “A 1.4 Deg2 Blind Survey for C II], C III] and C IV at
z ∼ 0.7–1.5 – II. Luminosity Functions and Cosmic Average Line Ratios.” Monthly
Notices of the Royal Astronomical Society, vol. 471, no. 3, Oxford University
Press, 2017, pp. 2575–86, doi:10.1093/mnras/stx1713.
short: A. Stroe, D. Sobral, J.J. Matthee, J. Calhau, I. Oteo, Monthly Notices of
the Royal Astronomical Society 471 (2017) 2575–2586.
date_created: 2022-07-12T12:54:57Z
date_published: 2017-11-01T00:00:00Z
date_updated: 2022-08-19T08:02:04Z
day: '01'
doi: 10.1093/mnras/stx1713
extern: '1'
external_id:
arxiv:
- '1703.10169'
intvolume: ' 471'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: active'
- 'galaxies: high redshift'
- 'galaxies: luminosity function'
- mass function
- 'quasars: emission lines'
- star formation
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1703.10169
month: '11'
oa: 1
oa_version: Preprint
page: 2575-2586
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: A 1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity
functions and cosmic average line ratios
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '11565'
abstract:
- lang: eng
text: We use the hydrodynamical EAGLE simulation to study the magnitude and origin
of the scatter in the stellar mass–halo mass relation for central galaxies. We
separate cause and effect by correlating stellar masses in the baryonic simulation
with halo properties in a matched dark matter only (DMO) simulation. The scatter
in stellar mass increases with redshift and decreases with halo mass. At z = 0.1,
it declines from 0.25 dex at M200, DMO ≈ 1011 M⊙ to 0.12 dex at M200, DMO ≈ 1013
M⊙, but the trend is weak above 1012 M⊙. For M200, DMO < 1012.5 M⊙ up to 0.04
dex of the scatter is due to scatter in the halo concentration. At fixed halo
mass, a larger stellar mass corresponds to a more concentrated halo. This is likely
because higher concentrations imply earlier formation times and hence more time
for accretion and star formation, and/or because feedback is less efficient in
haloes with higher binding energies. The maximum circular velocity, Vmax, DMO,
and binding energy are therefore more fundamental properties than halo mass, meaning
that they are more accurate predictors of stellar mass, and we provide fitting
formulae for their relations with stellar mass. However, concentration alone cannot
explain the total scatter in the Mstar−M200,DMO relation, and it does not explain
the scatter in Mstar–Vmax, DMO. Halo spin, sphericity, triaxiality, substructure
and environment are also not responsible for the remaining scatter, which thus
could be due to more complex halo properties or non-linear/stochastic baryonic
effects.
acknowledgement: We thank the anonymous referee for their comments. JM acknowledges
the support of a Huygens PhD fellowship from Leiden University. JM thanks David
Sobral for useful discussions and help with fitting routines and Jonas Chavez Montero
and Ying Zu for providing data. We thank PRACE for the access to the Curie facility
in France. We have used the DiRAC system which is a part of National E-Infrastructure
at Durham University, operated by the Institute for Computational Cosmology on behalf
of the STFC DiRAC HPC Facility (www.dirac.ac.uk); the equipment was funded by BIS
National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1,
STFC DiRAC Operations grant ST/K003267/1 and Durham University. The study was sponsored
by the Dutch National Computing Facilities Foundation (NCF) for the use of supercomputer
facilities, with financial support from the Netherlands Organisation for Scientific
Research (NWO), through VICI grant 639.043.409, and the European Research Council
under the European Union’s Seventh Framework Programme (FP7/2007-2013)/ERC Grant
agreement 278594- GasAroundGalaxies, and from the Belgian Science Policy Office
([AP P7/08 CHARM]). We have benefited greatly from the public available programming
language PYTHON, including the NUMPY, MATPLOTLIB, PYFITS, SCIPY, H5PY and RPY2 packages,
and the TOPCAT analysis program (Taylor 2005).
article_processing_charge: No
article_type: original
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Robert A.
full_name: Crain, Robert A.
last_name: Crain
- first_name: Matthieu
full_name: Schaller, Matthieu
last_name: Schaller
- first_name: Richard
full_name: Bower, Richard
last_name: Bower
- first_name: Tom
full_name: Theuns, Tom
last_name: Theuns
citation:
ama: Matthee JJ, Schaye J, Crain RA, Schaller M, Bower R, Theuns T. The origin of
scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE
simulation. Monthly Notices of the Royal Astronomical Society. 2017;465(2):2381-2396.
doi:10.1093/mnras/stw2884
apa: Matthee, J. J., Schaye, J., Crain, R. A., Schaller, M., Bower, R., & Theuns,
T. (2017). The origin of scatter in the stellar mass–halo mass relation of central
galaxies in the EAGLE simulation. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stw2884
chicago: Matthee, Jorryt J, Joop Schaye, Robert A. Crain, Matthieu Schaller, Richard
Bower, and Tom Theuns. “The Origin of Scatter in the Stellar Mass–Halo Mass Relation
of Central Galaxies in the EAGLE Simulation.” Monthly Notices of the Royal
Astronomical Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stw2884.
ieee: J. J. Matthee, J. Schaye, R. A. Crain, M. Schaller, R. Bower, and T. Theuns,
“The origin of scatter in the stellar mass–halo mass relation of central galaxies
in the EAGLE simulation,” Monthly Notices of the Royal Astronomical Society,
vol. 465, no. 2. Oxford University Press, pp. 2381–2396, 2017.
ista: Matthee JJ, Schaye J, Crain RA, Schaller M, Bower R, Theuns T. 2017. The origin
of scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE
simulation. Monthly Notices of the Royal Astronomical Society. 465(2), 2381–2396.
mla: Matthee, Jorryt J., et al. “The Origin of Scatter in the Stellar Mass–Halo
Mass Relation of Central Galaxies in the EAGLE Simulation.” Monthly Notices
of the Royal Astronomical Society, vol. 465, no. 2, Oxford University Press,
2017, pp. 2381–96, doi:10.1093/mnras/stw2884.
short: J.J. Matthee, J. Schaye, R.A. Crain, M. Schaller, R. Bower, T. Theuns, Monthly
Notices of the Royal Astronomical Society 465 (2017) 2381–2396.
date_created: 2022-07-12T12:25:08Z
date_published: 2017-02-01T00:00:00Z
date_updated: 2022-08-19T07:56:07Z
day: '01'
doi: 10.1093/mnras/stw2884
extern: '1'
external_id:
arxiv:
- '1608.08218'
intvolume: ' 465'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: formation'
- 'galaxies: haloes'
- 'cosmology: theory'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1608.08218
month: '02'
oa: 1
oa_version: Preprint
page: 2381-2396
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: The origin of scatter in the stellar mass–halo mass relation of central galaxies
in the EAGLE simulation
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 465
year: '2017'
...
---
_id: '11561'
abstract:
- lang: eng
text: We present a sample of ∼1000 emission-line galaxies at z = 0.4–4.7 from the
∼0.7deg2 High-z Emission-Line Survey in the Boötes field identified with a suite
of six narrow-band filters at ≈0.4–2.1 μm. These galaxies have been selected on
their Ly α (73), [O II] (285), H β/[O III] (387) or H α (362) emission line, and
have been classified with optical to near-infrared colours. A subsample of 98
sources have reliable redshifts from multiple narrow-band (e.g. [O II]–H α) detections
and/or spectroscopy. In this survey paper, we present the observations, selection
and catalogues of emitters. We measure number densities of Ly α, [O II], H β/[O III]
and H α and confirm strong luminosity evolution in star-forming galaxies from
z ∼ 0.4 to ∼5, in agreement with previous results. To demonstrate the usefulness
of dual-line emitters, we use the sample of dual [O II]–H α emitters to measure
the observed [O II]/H α ratio at z = 1.47. The observed [O II]/H α ratio increases
significantly from 0.40 ± 0.01 at z = 0.1 to 0.52 ± 0.05 at z = 1.47, which we
attribute to either decreasing dust attenuation with redshift, or due to a bias
in the (typically) fibre measurements in the local Universe that only measure
the central kpc regions. At the bright end, we find that both the H α and Ly α
number densities at z ≈ 2.2 deviate significantly from a Schechter form, following
a power law. We show that this is driven entirely by an increasing X-ray/active
galactic nucleus fraction with line luminosity, which reaches ≈100 per cent at
line luminosities L ≳ 3 × 1044 erg s−1.
article_processing_charge: No
article_type: original
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Philip
full_name: Best, Philip
last_name: Best
- first_name: Ian
full_name: Smail, Ian
last_name: Smail
- first_name: Fuyan
full_name: Bian, Fuyan
last_name: Bian
- first_name: Behnam
full_name: Darvish, Behnam
last_name: Darvish
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
- first_name: Xiaohui
full_name: Fan, Xiaohui
last_name: Fan
citation:
ama: 'Matthee JJ, Sobral D, Best P, et al. Boötes-HiZELS: An optical to near-infrared
survey of emission-line galaxies at z = 0.4–4.7. Monthly Notices of the Royal
Astronomical Society. 2017;471(1):629-649. doi:10.1093/mnras/stx1569'
apa: 'Matthee, J. J., Sobral, D., Best, P., Smail, I., Bian, F., Darvish, B., …
Fan, X. (2017). Boötes-HiZELS: An optical to near-infrared survey of emission-line
galaxies at z = 0.4–4.7. Monthly Notices of the Royal Astronomical Society.
Oxford University Press. https://doi.org/10.1093/mnras/stx1569'
chicago: 'Matthee, Jorryt J, David Sobral, Philip Best, Ian Smail, Fuyan Bian, Behnam
Darvish, Huub Röttgering, and Xiaohui Fan. “Boötes-HiZELS: An Optical to near-Infrared
Survey of Emission-Line Galaxies at z = 0.4–4.7.” Monthly Notices of the Royal
Astronomical Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1569.'
ieee: 'J. J. Matthee et al., “Boötes-HiZELS: An optical to near-infrared
survey of emission-line galaxies at z = 0.4–4.7,” Monthly Notices of the Royal
Astronomical Society, vol. 471, no. 1. Oxford University Press, pp. 629–649,
2017.'
ista: 'Matthee JJ, Sobral D, Best P, Smail I, Bian F, Darvish B, Röttgering H, Fan
X. 2017. Boötes-HiZELS: An optical to near-infrared survey of emission-line galaxies
at z = 0.4–4.7. Monthly Notices of the Royal Astronomical Society. 471(1), 629–649.'
mla: 'Matthee, Jorryt J., et al. “Boötes-HiZELS: An Optical to near-Infrared Survey
of Emission-Line Galaxies at z = 0.4–4.7.” Monthly Notices of the Royal Astronomical
Society, vol. 471, no. 1, Oxford University Press, 2017, pp. 629–49, doi:10.1093/mnras/stx1569.'
short: J.J. Matthee, D. Sobral, P. Best, I. Smail, F. Bian, B. Darvish, H. Röttgering,
X. Fan, Monthly Notices of the Royal Astronomical Society 471 (2017) 629–649.
date_created: 2022-07-12T11:01:35Z
date_published: 2017-10-01T00:00:00Z
date_updated: 2022-08-19T07:15:14Z
day: '01'
doi: 10.1093/mnras/stx1569
extern: '1'
external_id:
arxiv:
- '1702.04721'
intvolume: ' 471'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics galaxies
- active
- galaxies
- evolution
- galaxies
- high-redshift
- galaxies
- luminosity function
- mass function
- 'galaxies: star formation'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1702.04721
month: '10'
oa: 1
oa_version: Preprint
page: 629-649
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Boötes-HiZELS: An optical to near-infrared survey of emission-line galaxies
at z = 0.4–4.7'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '11572'
abstract:
- lang: eng
text: We present spectroscopic follow-up of candidate luminous Ly α emitters (LAEs)
at z = 5.7–6.6 in the SA22 field with VLT/X-SHOOTER. We confirm two new luminous
LAEs at z = 5.676 (SR6) and z = 6.532 (VR7), and also present HST follow-up of
both sources. These sources have luminosities LLy α ≈ 3 × 1043 erg s−1, very high
rest-frame equivalent widths of EW0 ≳ 200 Å and narrow Ly α lines (200–340 km s−1).
VR7 is the most UV-luminous LAE at z > 6.5, with M1500 = −22.5, even brighter
in the UV than CR7. Besides Ly α, we do not detect any other rest-frame UV lines
in the spectra of SR6 and VR7, and argue that rest-frame UV lines are easier to
observe in bright galaxies with low Ly α equivalent widths. We confirm that Ly α
line widths increase with Ly α luminosity at z = 5.7, while there are indications
that Ly α lines of faint LAEs become broader at z = 6.6, potentially due to reionization.
We find a large spread of up to 3 dex in UV luminosity for >L⋆ LAEs, but find
that the Ly α luminosity of the brightest LAEs is strongly related to UV luminosity
at z = 6.6. Under basic assumptions, we find that several LAEs at z ≈ 6–7 have
Ly α escape fractions ≳ 100 per cent, indicating bursty star formation histories,
alternative Ly α production mechanisms, or dust attenuating Ly α emission differently
than UV emission. Finally, we present a method to compute ξion, the production
efficiency of ionizing photons, and find that LAEs at z ≈ 6–7 have high values
of log10(ξion/Hz erg−1) ≈ 25.51 ± 0.09 that may alleviate the need for high Lyman-Continuum
escape fractions required for reionization.
acknowledgement: 'We thank the referee for a constructive report that has improved
the quality and clarity of this work. The authors thank Grecco Oyarzún for discussions.
JM acknowledges the support of a Huygens PhD fellowship from Leiden University.
DS acknowledges financial support from the Netherlands Organisation for Scientific
research (NWO) through a Veni fellowship and from Lancaster University through an
Early Career Internal Grant A100679. BD acknowledges financial support from NASA
through the Astrophysics Data Analysis Program (ADAP), grant number NNX12AE20G.
We thank Kasper Schmidt for providing measurements. Based on observations with the
W.M. Keck Observatory through programme C267D. The W.M. Keck Observatory is operated
as a scientific partnership amongst the California Institute of Technology, the
University of California and the National Aeronautics and Space Administration.
Based on observations made with ESO Telescopes at the La Silla Paranal Observatory
under programme IDs 097.A-0943, 294.A 5018 and 098.A-0819 and on data products produced
by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium.
The authors acknowledge the award of observing time (W16AN004) and of service time
(SW2014b20) on the William Herschel Telescope (WHT). WHT and its service programme
are operated on the island of La Palma by the Isaac Newton Group in the Spanish
Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias.
Based on observations made with the NASA/ESA HST, obtained (from the Data Archive)
at the Space Telescope Science Institute, which is operated by the Association of
Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These
observations are associated with programme #14699. We are grateful for the excellent
data sets from the COSMOS, UltraVISTA, SXDS, UDS and CFHTLS survey teams; without
these legacy surveys, this research would have been impossible. We have benefited
from the public available programming language PYTHON, including the NUMPY, MATPLOTLIB,
PYFITS, SCIPY and ASTROPY packages, the astronomical imaging tools SEXTRACTOR, SWARP
and SCAMP and the TOPCAT analysis tool (Taylor 2013).'
article_processing_charge: No
article_type: original
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Behnam
full_name: Darvish, Behnam
last_name: Darvish
- first_name: Sérgio
full_name: Santos, Sérgio
last_name: Santos
- first_name: Bahram
full_name: Mobasher, Bahram
last_name: Mobasher
- first_name: Ana
full_name: Paulino-Afonso, Ana
last_name: Paulino-Afonso
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
- first_name: Lara
full_name: Alegre, Lara
last_name: Alegre
citation:
ama: Matthee JJ, Sobral D, Darvish B, et al. Spectroscopic properties of luminous
Ly α emitters at z ≈ 6–7 and comparison to the Lyman-break population. Monthly
Notices of the Royal Astronomical Society. 2017;472(1):772-787. doi:10.1093/mnras/stx2061
apa: Matthee, J. J., Sobral, D., Darvish, B., Santos, S., Mobasher, B., Paulino-Afonso,
A., … Alegre, L. (2017). Spectroscopic properties of luminous Ly α emitters at
z ≈ 6–7 and comparison to the Lyman-break population. Monthly Notices of the
Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stx2061
chicago: Matthee, Jorryt J, David Sobral, Behnam Darvish, Sérgio Santos, Bahram
Mobasher, Ana Paulino-Afonso, Huub Röttgering, and Lara Alegre. “Spectroscopic
Properties of Luminous Ly α Emitters at z ≈ 6–7 and Comparison to the Lyman-Break
Population.” Monthly Notices of the Royal Astronomical Society. Oxford
University Press, 2017. https://doi.org/10.1093/mnras/stx2061.
ieee: J. J. Matthee et al., “Spectroscopic properties of luminous Ly α emitters
at z ≈ 6–7 and comparison to the Lyman-break population,” Monthly Notices of
the Royal Astronomical Society, vol. 472, no. 1. Oxford University Press,
pp. 772–787, 2017.
ista: Matthee JJ, Sobral D, Darvish B, Santos S, Mobasher B, Paulino-Afonso A, Röttgering
H, Alegre L. 2017. Spectroscopic properties of luminous Ly α emitters at z ≈ 6–7
and comparison to the Lyman-break population. Monthly Notices of the Royal Astronomical
Society. 472(1), 772–787.
mla: Matthee, Jorryt J., et al. “Spectroscopic Properties of Luminous Ly α Emitters
at z ≈ 6–7 and Comparison to the Lyman-Break Population.” Monthly Notices of
the Royal Astronomical Society, vol. 472, no. 1, Oxford University Press,
2017, pp. 772–87, doi:10.1093/mnras/stx2061.
short: J.J. Matthee, D. Sobral, B. Darvish, S. Santos, B. Mobasher, A. Paulino-Afonso,
H. Röttgering, L. Alegre, Monthly Notices of the Royal Astronomical Society 472
(2017) 772–787.
date_created: 2022-07-13T09:47:39Z
date_published: 2017-11-01T00:00:00Z
date_updated: 2022-08-19T08:05:37Z
day: '01'
doi: 10.1093/mnras/stx2061
extern: '1'
external_id:
arxiv:
- '1706.06591'
intvolume: ' 472'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution – galaxies: high-redshift'
- dark ages
- reionization
- first stars
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1706.06591
month: '11'
oa: 1
oa_version: Preprint
page: 772-787
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Spectroscopic properties of luminous Ly α emitters at z ≈ 6–7 and comparison
to the Lyman-break population
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 472
year: '2017'
...
---
_id: '11573'
abstract:
- lang: eng
text: We present dynamical measurements from the KMOS (K-band multi-object spectrograph)
Deep Survey (KDS), which comprises 77 typical star-forming galaxies at z ≃ 3.5
in the mass range 9.0 < log (M⋆/M⊙) < 10.5. These measurements constrain the internal
dynamics, the intrinsic velocity dispersions (σint) and rotation velocities (VC)
of galaxies in the high-redshift Universe. The mean velocity dispersion of the
galaxies in our sample is σint=70.8+3.3−3.1kms−1, revealing that the increasing
average σint with increasing redshift, reported for z ≲ 2, continues out to z
≃ 3.5. Only 36 ± 8 per cent of our galaxies are rotation-dominated (VC/σint >
1), with the sample average VC/σint value much smaller than at lower redshift.
After carefully selecting comparable star-forming samples at multiple epochs,
we find that the rotation-dominated fraction evolves with redshift with a z−0.2
dependence. The rotation-dominated KDS galaxies show no clear offset from the
local rotation velocity–stellar mass (i.e. VC–M⋆) relation, although a smaller
fraction of the galaxies are on the relation due to the increase in the dispersion-dominated
fraction. These observations are consistent with a simple equilibrium model picture,
in which random motions are boosted in high-redshift galaxies by a combination
of the increasing gas fractions, accretion efficiency, specific star formation
rate and stellar feedback and which may provide significant pressure support against
gravity on the galactic disc scale.
acknowledgement: 'We wish to thank the anonymous referee for their comments, which
have improved the quality and clarity of this work. OJT acknowledges the financial
support of the Science and Technology Facilities Council through a studentship award.
MC and OJT acknowledge the KMOS team and all the personnel of the European Southern
Observatory Very Large Telescope for outstanding support during the KMOS GTO observations.
CMH, AMS and RMS acknowledge the Science and Technology Facilities Council through
grant code ST/L00075X/1. RJM acknowledges the support of the European Research Council
via the award of a Consolidator Grant (PI: McLure). JSD acknowledges the support
of the European Research Council via the award of an Advanced Grant (PI J. Dunlop),
and the contribution of the EC FP7 SPACE project ASTRODEEP (Ref.No: 312725). AMS
acknowledges the Leverhulme Foundation. JM acknowledges the support of a Huygens
PhD fellowship from Leiden University. DS acknowledges financial support from the
Netherlands Organization for Scientific research (NWO) through a Veni fellowship
and from FCT through an FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010).
This work is based on observations taken by the CANDELS Multi-Cycle Treasury Program
with the NASA/ESA HST, which is operated by the Association of Universities for
Research in Astronomy, Inc., under NASA contract NAS5-26555. This work is based
on observations taken by the 3D HST Treasury Program (GO 12177 and 12328) with the
NASA/ESA HST, which is operated by the Association of Universities for Research
in Astronomy, Inc., under NASA contract NAS5-26555. Based on data obtained with
the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large
Program 185.A-0791, and made available by the VUDS team at the CESAM data centre,
Laboratoire d’Astrophysique de Marseille, France. Based on observations obtained
at the Very Large Telescope of the European Southern Observatory. Programme IDs:
092.A 0399(A), 093.A-0122(A,B), 094.A-0214(A,B),095.A0680(A,B),096.A-0315(A,B,C).'
article_processing_charge: No
article_type: original
author:
- first_name: O. J.
full_name: Turner, O. J.
last_name: Turner
- first_name: M.
full_name: Cirasuolo, M.
last_name: Cirasuolo
- first_name: C. M.
full_name: Harrison, C. M.
last_name: Harrison
- first_name: R. J.
full_name: McLure, R. J.
last_name: McLure
- first_name: J. S.
full_name: Dunlop, J. S.
last_name: Dunlop
- first_name: A. M.
full_name: Swinbank, A. M.
last_name: Swinbank
- first_name: H. L.
full_name: Johnson, H. L.
last_name: Johnson
- first_name: D.
full_name: Sobral, D.
last_name: Sobral
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: R. M.
full_name: Sharples, R. M.
last_name: Sharples
citation:
ama: Turner OJ, Cirasuolo M, Harrison CM, et al. The KMOS Deep Survey (KDS) – I.
Dynamical measurements of typical star-forming galaxies at z ≃ 3.5. Monthly
Notices of the Royal Astronomical Society. 2017;471(2):1280-1320. doi:10.1093/mnras/stx1366
apa: Turner, O. J., Cirasuolo, M., Harrison, C. M., McLure, R. J., Dunlop, J. S.,
Swinbank, A. M., … Sharples, R. M. (2017). The KMOS Deep Survey (KDS) – I. Dynamical
measurements of typical star-forming galaxies at z ≃ 3.5. Monthly Notices of
the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stx1366
chicago: Turner, O. J., M. Cirasuolo, C. M. Harrison, R. J. McLure, J. S. Dunlop,
A. M. Swinbank, H. L. Johnson, D. Sobral, Jorryt J Matthee, and R. M. Sharples.
“The KMOS Deep Survey (KDS) – I. Dynamical Measurements of Typical Star-Forming
Galaxies at z ≃ 3.5.” Monthly Notices of the Royal Astronomical Society.
Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1366.
ieee: O. J. Turner et al., “The KMOS Deep Survey (KDS) – I. Dynamical measurements
of typical star-forming galaxies at z ≃ 3.5,” Monthly Notices of the Royal
Astronomical Society, vol. 471, no. 2. Oxford University Press, pp. 1280–1320,
2017.
ista: Turner OJ, Cirasuolo M, Harrison CM, McLure RJ, Dunlop JS, Swinbank AM, Johnson
HL, Sobral D, Matthee JJ, Sharples RM. 2017. The KMOS Deep Survey (KDS) – I. Dynamical
measurements of typical star-forming galaxies at z ≃ 3.5. Monthly Notices of the
Royal Astronomical Society. 471(2), 1280–1320.
mla: Turner, O. J., et al. “The KMOS Deep Survey (KDS) – I. Dynamical Measurements
of Typical Star-Forming Galaxies at z ≃ 3.5.” Monthly Notices of the Royal
Astronomical Society, vol. 471, no. 2, Oxford University Press, 2017, pp.
1280–320, doi:10.1093/mnras/stx1366.
short: O.J. Turner, M. Cirasuolo, C.M. Harrison, R.J. McLure, J.S. Dunlop, A.M.
Swinbank, H.L. Johnson, D. Sobral, J.J. Matthee, R.M. Sharples, Monthly Notices
of the Royal Astronomical Society 471 (2017) 1280–1320.
date_created: 2022-07-13T10:03:01Z
date_published: 2017-10-01T00:00:00Z
date_updated: 2022-08-19T08:07:31Z
day: '01'
doi: 10.1093/mnras/stx1366
extern: '1'
external_id:
arxiv:
- '1704.06263'
intvolume: ' 471'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: high-redshift'
- 'galaxies: kinematics and dynamics'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1704.06263
month: '10'
oa: 1
oa_version: Preprint
page: 1280-1320
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: The KMOS Deep Survey (KDS) – I. Dynamical measurements of typical star-forming
galaxies at z ≃ 3.5
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '11633'
abstract:
- lang: eng
text: Our understanding of stars through asteroseismic data analysis is limited
by our ability to take advantage of the huge amount of observed stars provided
by space missions such as CoRoT, Kepler , K2, and soon TESS and PLATO. Global
seismic pipelines provide global stellar parameters such as mass and radius using
the mean seismic parameters, as well as the effective temperature. These pipelines
are commonly used automatically on thousands of stars observed by K2 for 3 months
(and soon TESS for at least ∼ 1 month). However, pipelines are not immune from
misidentifying noise peaks and stellar oscillations. Therefore, new validation
techniques are required to assess the quality of these results. We present a new
metric called FliPer (Flicker in Power), which takes into account the average
variability at all measured time scales. The proper calibration of FliPer enables
us to obtain good estimations of global stellar parameters such as surface gravity
that are robust against the influence of noise peaks and hence are an excellent
way to find faults in asteroseismic pipelines.
article_number: '1711.02890'
article_processing_charge: No
author:
- first_name: Lisa Annabelle
full_name: Bugnet, Lisa Annabelle
id: d9edb345-f866-11ec-9b37-d119b5234501
last_name: Bugnet
orcid: 0000-0003-0142-4000
- first_name: R. A.
full_name: Garcia, R. A.
last_name: Garcia
- first_name: G. R.
full_name: Davies, G. R.
last_name: Davies
- first_name: S.
full_name: Mathur, S.
last_name: Mathur
- first_name: E.
full_name: Corsaro, E.
last_name: Corsaro
citation:
ama: 'Bugnet LA, Garcia RA, Davies GR, Mathur S, Corsaro E. FliPer: Checking the
reliability of global seismic parameters from automatic pipelines. arXiv.
doi:10.48550/arXiv.1711.02890'
apa: 'Bugnet, L. A., Garcia, R. A., Davies, G. R., Mathur, S., & Corsaro, E.
(n.d.). FliPer: Checking the reliability of global seismic parameters from automatic
pipelines. arXiv. https://doi.org/10.48550/arXiv.1711.02890'
chicago: 'Bugnet, Lisa Annabelle, R. A. Garcia, G. R. Davies, S. Mathur, and E.
Corsaro. “FliPer: Checking the Reliability of Global Seismic Parameters from Automatic
Pipelines.” ArXiv, n.d. https://doi.org/10.48550/arXiv.1711.02890.'
ieee: 'L. A. Bugnet, R. A. Garcia, G. R. Davies, S. Mathur, and E. Corsaro, “FliPer:
Checking the reliability of global seismic parameters from automatic pipelines,”
arXiv. .'
ista: 'Bugnet LA, Garcia RA, Davies GR, Mathur S, Corsaro E. FliPer: Checking the
reliability of global seismic parameters from automatic pipelines. arXiv, 1711.02890.'
mla: 'Bugnet, Lisa Annabelle, et al. “FliPer: Checking the Reliability of Global
Seismic Parameters from Automatic Pipelines.” ArXiv, 1711.02890, doi:10.48550/arXiv.1711.02890.'
short: L.A. Bugnet, R.A. Garcia, G.R. Davies, S. Mathur, E. Corsaro, ArXiv (n.d.).
date_created: 2022-07-21T07:13:13Z
date_published: 2017-11-08T00:00:00Z
date_updated: 2022-08-22T08:45:42Z
day: '08'
doi: 10.48550/arXiv.1711.02890
extern: '1'
external_id:
arxiv:
- '1711.02890'
keyword:
- asteroseismology - methods
- data analysis - stars
- oscillations
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.1711.02890
month: '11'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: 'FliPer: Checking the reliability of global seismic parameters from automatic
pipelines'
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2017'
...
---
_id: '11651'
abstract:
- lang: eng
text: Diffusions and related random walk procedures are of central importance in
many areas of machine learning, data analysis, and applied mathematics. Because
they spread mass agnostically at each step in an iterative manner, they can sometimes
spread mass “too aggressively,” thereby failing to find the “right” clusters.
We introduce a novel Capacity Releasing Diffusion (CRD) Process, which is both
faster and stays more local than the classical spectral diffusion process. As
an application, we use our CRD Process to develop an improved local algorithm
for graph clustering. Our local graph clustering method can find local clusters
in a model of clustering where one begins the CRD Process in a cluster whose vertices
are connected better internally than externally by an O(log2n) factor, where n
is the number of nodes in the cluster. Thus, our CRD Process is the first local
graph clustering algorithm that is not subject to the well-known quadratic Cheeger
barrier. Our result requires a certain smoothness condition, which we expect to
be an artifact of our analysis. Our empirical evaluation demonstrates improved
results, in particular for realistic social graphs where there are moderately
good—but not very good—clusters.
alternative_title:
- PMLR
article_processing_charge: No
author:
- first_name: Di
full_name: Wang, Di
last_name: Wang
- first_name: Kimon
full_name: Fountoulakis, Kimon
last_name: Fountoulakis
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: Michael W.
full_name: Mahoney, Michael W.
last_name: Mahoney
- first_name: ' Satish'
full_name: Rao , Satish
last_name: 'Rao '
citation:
ama: 'Wang D, Fountoulakis K, Henzinger MH, Mahoney MW, Rao Satish. Capacity releasing
diffusion for speed and locality. In: Proceedings of the 34th International
Conference on Machine Learning. Vol 70. ML Research Press; 2017:3598-3607.'
apa: 'Wang, D., Fountoulakis, K., Henzinger, M. H., Mahoney, M. W., & Rao , Satish.
(2017). Capacity releasing diffusion for speed and locality. In Proceedings
of the 34th International Conference on Machine Learning (Vol. 70, pp. 3598–3607).
Sydney, Australia: ML Research Press.'
chicago: Wang, Di, Kimon Fountoulakis, Monika H Henzinger, Michael W. Mahoney, and Satish
Rao . “Capacity Releasing Diffusion for Speed and Locality.” In Proceedings
of the 34th International Conference on Machine Learning, 70:3598–3607. ML
Research Press, 2017.
ieee: D. Wang, K. Fountoulakis, M. H. Henzinger, M. W. Mahoney, and Satish Rao
, “Capacity releasing diffusion for speed and locality,” in Proceedings of
the 34th International Conference on Machine Learning, Sydney, Australia,
2017, vol. 70, pp. 3598–3607.
ista: Wang D, Fountoulakis K, Henzinger MH, Mahoney MW, Rao Satish. 2017. Capacity
releasing diffusion for speed and locality. Proceedings of the 34th International
Conference on Machine Learning. International Conference on Machine Learning,
PMLR, vol. 70, 3598–3607.
mla: Wang, Di, et al. “Capacity Releasing Diffusion for Speed and Locality.” Proceedings
of the 34th International Conference on Machine Learning, vol. 70, ML Research
Press, 2017, pp. 3598–607.
short: D. Wang, K. Fountoulakis, M.H. Henzinger, M.W. Mahoney, Satish Rao , in:,
Proceedings of the 34th International Conference on Machine Learning, ML Research
Press, 2017, pp. 3598–3607.
conference:
end_date: 2017-08-11
location: Sydney, Australia
name: International Conference on Machine Learning
start_date: 2017-08-06
date_created: 2022-07-25T13:59:21Z
date_published: 2017-09-01T00:00:00Z
date_updated: 2023-02-09T09:15:31Z
day: '01'
extern: '1'
external_id:
arxiv:
- '1706.05826'
intvolume: ' 70'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://proceedings.mlr.press/v70/wang17b/wang17b.pdf
month: '09'
oa: 1
oa_version: Published Version
page: 3598-3607
publication: Proceedings of the 34th International Conference on Machine Learning
publication_identifier:
eissn:
- 2640-3498
publication_status: published
publisher: ML Research Press
quality_controlled: '1'
status: public
title: Capacity releasing diffusion for speed and locality
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 70
year: '2017'
...
---
_id: '11665'
abstract:
- lang: eng
text: "We study the problem of maintaining a breadth-first spanning tree (BFS tree)
in partially dynamic distributed networks modeling a sequence of either failures
or additions of communication links (but not both). We present deterministic (1+ϵ)-approximation
algorithms whose amortized time (over some number of link changes) is sublinear
in D, the maximum diameter of the network.\r\n\r\nOur technique also leads to
a deterministic (1+ϵ)-approximate incremental algorithm for single-source shortest
paths in the sequential (usual RAM) model. Prior to our work, the state of the
art was the classic exact algorithm of Even and Shiloach (1981), which is optimal
under some assumptions (Roditty and Zwick 2011; Henzinger et al. 2015). Our result
is the first to show that, in the incremental setting, this bound can be beaten
in certain cases if some approximation is allowed."
acknowledgement: "We thank the reviewers of ICALP 2013 for pointing to related articles
and to an error in an example\r\ngiven in a previous version of this article. We
also thank one of the reviewers of Transactions on\r\nAlgorithms for very detailed
comments."
article_number: '51'
article_processing_charge: No
article_type: original
author:
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: Sebastian
full_name: Krinninger, Sebastian
last_name: Krinninger
- first_name: Danupon
full_name: Nanongkai, Danupon
last_name: Nanongkai
citation:
ama: Henzinger MH, Krinninger S, Nanongkai D. Sublinear-time maintenance of breadth-first
spanning trees in partially dynamic networks. ACM Transactions on Algorithms.
2017;13(4). doi:10.1145/3146550
apa: Henzinger, M. H., Krinninger, S., & Nanongkai, D. (2017). Sublinear-time
maintenance of breadth-first spanning trees in partially dynamic networks. ACM
Transactions on Algorithms. Association for Computing Machinery. https://doi.org/10.1145/3146550
chicago: Henzinger, Monika H, Sebastian Krinninger, and Danupon Nanongkai. “Sublinear-Time
Maintenance of Breadth-First Spanning Trees in Partially Dynamic Networks.” ACM
Transactions on Algorithms. Association for Computing Machinery, 2017. https://doi.org/10.1145/3146550.
ieee: M. H. Henzinger, S. Krinninger, and D. Nanongkai, “Sublinear-time maintenance
of breadth-first spanning trees in partially dynamic networks,” ACM Transactions
on Algorithms, vol. 13, no. 4. Association for Computing Machinery, 2017.
ista: Henzinger MH, Krinninger S, Nanongkai D. 2017. Sublinear-time maintenance
of breadth-first spanning trees in partially dynamic networks. ACM Transactions
on Algorithms. 13(4), 51.
mla: Henzinger, Monika H., et al. “Sublinear-Time Maintenance of Breadth-First Spanning
Trees in Partially Dynamic Networks.” ACM Transactions on Algorithms, vol.
13, no. 4, 51, Association for Computing Machinery, 2017, doi:10.1145/3146550.
short: M.H. Henzinger, S. Krinninger, D. Nanongkai, ACM Transactions on Algorithms
13 (2017).
date_created: 2022-07-27T11:37:23Z
date_published: 2017-10-01T00:00:00Z
date_updated: 2022-09-09T11:57:42Z
day: '01'
doi: 10.1145/3146550
extern: '1'
external_id:
arxiv:
- '1512.08147'
intvolume: ' 13'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1512.08147
month: '10'
oa: 1
oa_version: Preprint
publication: ACM Transactions on Algorithms
publication_identifier:
eissn:
- 1549-6333
issn:
- 1549-6325
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: Sublinear-time maintenance of breadth-first spanning trees in partially dynamic
networks
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 13
year: '2017'
...
---
_id: '11676'
abstract:
- lang: eng
text: We study the problem of maximizing a monotone submodular function with viability
constraints. This problem originates from computational biology, where we are
given a phylogenetic tree over a set of species and a directed graph, the so-called
food web, encoding viability constraints between these species. These food webs
usually have constant depth. The goal is to select a subset of k species that
satisfies the viability constraints and has maximal phylogenetic diversity. As
this problem is known to be NP-hard, we investigate approximation algorithms.
We present the first constant factor approximation algorithm if the depth is constant.
Its approximation ratio is (1−1e√). This algorithm not only applies to phylogenetic
trees with viability constraints but for arbitrary monotone submodular set functions
with viability constraints. Second, we show that there is no (1−1/e+ϵ)-approximation
algorithm for our problem setting (even for additive functions) and that there
is no approximation algorithm for a slight extension of this setting.
acknowledgement: "The research leading to these results has received funding from
the European Research\r\nCouncil under the European Union’s Seventh Framework Programme
(FP/2007-2013)/ERC Grant Agreement No. 340506."
article_processing_charge: No
article_type: original
author:
- first_name: Wolfgang
full_name: Dvořák, Wolfgang
last_name: Dvořák
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: David P.
full_name: Williamson, David P.
last_name: Williamson
citation:
ama: Dvořák W, Henzinger MH, Williamson DP. Maximizing a submodular function with
viability constraints. Algorithmica. 2017;77(1):152-172. doi:10.1007/s00453-015-0066-y
apa: Dvořák, W., Henzinger, M. H., & Williamson, D. P. (2017). Maximizing a
submodular function with viability constraints. Algorithmica. Springer
Nature. https://doi.org/10.1007/s00453-015-0066-y
chicago: Dvořák, Wolfgang, Monika H Henzinger, and David P. Williamson. “Maximizing
a Submodular Function with Viability Constraints.” Algorithmica. Springer
Nature, 2017. https://doi.org/10.1007/s00453-015-0066-y.
ieee: W. Dvořák, M. H. Henzinger, and D. P. Williamson, “Maximizing a submodular
function with viability constraints,” Algorithmica, vol. 77, no. 1. Springer
Nature, pp. 152–172, 2017.
ista: Dvořák W, Henzinger MH, Williamson DP. 2017. Maximizing a submodular function
with viability constraints. Algorithmica. 77(1), 152–172.
mla: Dvořák, Wolfgang, et al. “Maximizing a Submodular Function with Viability Constraints.”
Algorithmica, vol. 77, no. 1, Springer Nature, 2017, pp. 152–72, doi:10.1007/s00453-015-0066-y.
short: W. Dvořák, M.H. Henzinger, D.P. Williamson, Algorithmica 77 (2017) 152–172.
date_created: 2022-07-27T14:37:24Z
date_published: 2017-01-01T00:00:00Z
date_updated: 2022-09-12T08:58:16Z
day: '01'
doi: 10.1007/s00453-015-0066-y
extern: '1'
external_id:
arxiv:
- '1611.05753'
intvolume: ' 77'
issue: '1'
keyword:
- Approximation algorithms
- Submodular functions
- Phylogenetic diversity
- Viability constraints
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1611.05753
month: '01'
oa: 1
oa_version: Preprint
page: 152-172
publication: Algorithmica
publication_identifier:
eissn:
- 1432-0541
issn:
- 0178-4617
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Maximizing a submodular function with viability constraints
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 77
year: '2017'
...
---
_id: '1175'
abstract:
- lang: eng
text: We study space complexity and time-space trade-offs with a focus not on peak
memory usage but on overall memory consumption throughout the computation. Such
a cumulative space measure was introduced for the computational model of parallel
black pebbling by [Alwen and Serbinenko ’15] as a tool for obtaining results in
cryptography. We consider instead the non- deterministic black-white pebble game
and prove optimal cumulative space lower bounds and trade-offs, where in order
to minimize pebbling time the space has to remain large during a significant fraction
of the pebbling. We also initiate the study of cumulative space in proof complexity,
an area where other space complexity measures have been extensively studied during
the last 10–15 years. Using and extending the connection between proof complexity
and pebble games in [Ben-Sasson and Nordström ’08, ’11] we obtain several strong
cumulative space results for (even parallel versions of) the resolution proof
system, and outline some possible future directions of study of this, in our opinion,
natural and interesting space measure.
alternative_title:
- LIPIcs
author:
- first_name: Joel F
full_name: Alwen, Joel F
id: 2A8DFA8C-F248-11E8-B48F-1D18A9856A87
last_name: Alwen
- first_name: Susanna
full_name: De Rezende, Susanna
last_name: De Rezende
- first_name: Jakob
full_name: Nordstrom, Jakob
last_name: Nordstrom
- first_name: Marc
full_name: Vinyals, Marc
last_name: Vinyals
citation:
ama: 'Alwen JF, De Rezende S, Nordstrom J, Vinyals M. Cumulative space in black-white
pebbling and resolution. In: Papadimitriou C, ed. Vol 67. Schloss Dagstuhl - Leibniz-Zentrum
für Informatik; 2017:38:1-38-21. doi:10.4230/LIPIcs.ITCS.2017.38'
apa: 'Alwen, J. F., De Rezende, S., Nordstrom, J., & Vinyals, M. (2017). Cumulative
space in black-white pebbling and resolution. In C. Papadimitriou (Ed.) (Vol.
67, p. 38:1-38-21). Presented at the ITCS: Innovations in Theoretical Computer
Science, Berkeley, CA, United States: Schloss Dagstuhl - Leibniz-Zentrum für Informatik.
https://doi.org/10.4230/LIPIcs.ITCS.2017.38'
chicago: Alwen, Joel F, Susanna De Rezende, Jakob Nordstrom, and Marc Vinyals. “Cumulative
Space in Black-White Pebbling and Resolution.” edited by Christos Papadimitriou,
67:38:1-38-21. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017. https://doi.org/10.4230/LIPIcs.ITCS.2017.38.
ieee: 'J. F. Alwen, S. De Rezende, J. Nordstrom, and M. Vinyals, “Cumulative space
in black-white pebbling and resolution,” presented at the ITCS: Innovations in
Theoretical Computer Science, Berkeley, CA, United States, 2017, vol. 67, p. 38:1-38-21.'
ista: 'Alwen JF, De Rezende S, Nordstrom J, Vinyals M. 2017. Cumulative space in
black-white pebbling and resolution. ITCS: Innovations in Theoretical Computer
Science, LIPIcs, vol. 67, 38:1-38-21.'
mla: Alwen, Joel F., et al. Cumulative Space in Black-White Pebbling and Resolution.
Edited by Christos Papadimitriou, vol. 67, Schloss Dagstuhl - Leibniz-Zentrum
für Informatik, 2017, p. 38:1-38-21, doi:10.4230/LIPIcs.ITCS.2017.38.
short: J.F. Alwen, S. De Rezende, J. Nordstrom, M. Vinyals, in:, C. Papadimitriou
(Ed.), Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017, p. 38:1-38-21.
conference:
end_date: 2017-01-11
location: Berkeley, CA, United States
name: 'ITCS: Innovations in Theoretical Computer Science'
start_date: 2017-01-09
date_created: 2018-12-11T11:50:33Z
date_published: 2017-01-01T00:00:00Z
date_updated: 2021-01-12T06:48:51Z
day: '01'
ddc:
- '005'
- '600'
department:
- _id: KrPi
doi: 10.4230/LIPIcs.ITCS.2017.38
editor:
- first_name: Christos
full_name: Papadimitriou, Christos
last_name: Papadimitriou
file:
- access_level: open_access
checksum: dbc94810be07c2fb1945d5c2a6130e6c
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:17:11Z
date_updated: 2020-07-14T12:44:37Z
file_id: '5263'
file_name: IST-2018-927-v1+1_LIPIcs-ITCS-2017-38.pdf
file_size: 557769
relation: main_file
file_date_updated: 2020-07-14T12:44:37Z
has_accepted_license: '1'
intvolume: ' 67'
language:
- iso: eng
license: https://creativecommons.org/licenses/by/4.0/
month: '01'
oa: 1
oa_version: Published Version
page: 38:1-38-21
publication_identifier:
issn:
- '18688969'
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
publist_id: '6179'
pubrep_id: '927'
quality_controlled: '1'
scopus_import: 1
status: public
title: Cumulative space in black-white pebbling and resolution
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 67
year: '2017'
...
---
_id: '11829'
abstract:
- lang: eng
text: "In recent years it has become popular to study dynamic problems in a sensitivity
setting: Instead of allowing for an arbitrary sequence of updates, the sensitivity
model only allows to apply batch updates of small size to the original input data.
The sensitivity model is particularly appealing since recent strong conditional
lower bounds ruled out fast algorithms for many dynamic problems, such as shortest
paths, reachability, or subgraph connectivity.\r\n\r\nIn this paper we prove conditional
lower bounds for these and additional problems in a sensitivity setting. For example,
we show that under the Boolean Matrix Multiplication (BMM) conjecture combinatorial
algorithms cannot compute the (4/3-\\varepsilon)-approximate diameter of an undirected
unweighted dense graph with truly subcubic preprocessing time and truly subquadratic
update/query time. This result is surprising since in the static setting it is
not clear whether a reduction from BMM to diameter is possible. We further show
under the BMM conjecture that many problems, such as reachability or approximate
shortest paths, cannot be solved faster than by recomputation from scratch even
after only one or two edge insertions. We extend our reduction from BMM to Diameter
to give a reduction from All Pairs Shortest Paths to Diameter under one deletion
in weighted graphs. This is intriguing, as in the static setting it is a big open
problem whether Diameter is as hard as APSP. We further get a nearly tight lower
bound for shortest paths after two edge deletions based on the APSP conjecture.
We give more lower bounds under the Strong Exponential Time Hypothesis. Many of
our lower bounds also hold for static oracle data structures where no sensitivity
is required.\r\n\r\nFinally, we give the first algorithm for the (1+\\varepsilon)-approximate
radius, diameter, and eccentricity problems in directed or undirected unweighted
graphs in case of single edges failures. The algorithm has a truly subcubic running
time for graphs with a truly subquadratic number of edges; it is tight w.r.t.
the conditional lower bounds we obtain."
alternative_title:
- LIPIcs
article_number: '26'
article_processing_charge: No
author:
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: Andrea
full_name: Lincoln, Andrea
last_name: Lincoln
- first_name: Stefan
full_name: Neumann, Stefan
last_name: Neumann
- first_name: Virginia
full_name: Vassilevska Williams, Virginia
last_name: Vassilevska Williams
citation:
ama: 'Henzinger MH, Lincoln A, Neumann S, Vassilevska Williams V. Conditional hardness
for sensitivity problems. In: 8th Innovations in Theoretical Computer Science
Conference. Vol 67. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2017.
doi:10.4230/LIPICS.ITCS.2017.26'
apa: 'Henzinger, M. H., Lincoln, A., Neumann, S., & Vassilevska Williams, V.
(2017). Conditional hardness for sensitivity problems. In 8th Innovations in
Theoretical Computer Science Conference (Vol. 67). Berkley, CA, United States:
Schloss Dagstuhl - Leibniz-Zentrum für Informatik. https://doi.org/10.4230/LIPICS.ITCS.2017.26'
chicago: Henzinger, Monika H, Andrea Lincoln, Stefan Neumann, and Virginia Vassilevska
Williams. “Conditional Hardness for Sensitivity Problems.” In 8th Innovations
in Theoretical Computer Science Conference, Vol. 67. Schloss Dagstuhl - Leibniz-Zentrum
für Informatik, 2017. https://doi.org/10.4230/LIPICS.ITCS.2017.26.
ieee: M. H. Henzinger, A. Lincoln, S. Neumann, and V. Vassilevska Williams, “Conditional
hardness for sensitivity problems,” in 8th Innovations in Theoretical Computer
Science Conference, Berkley, CA, United States, 2017, vol. 67.
ista: 'Henzinger MH, Lincoln A, Neumann S, Vassilevska Williams V. 2017. Conditional
hardness for sensitivity problems. 8th Innovations in Theoretical Computer Science
Conference. ITCS: Innovations in Theoretical Computer Science Conference, LIPIcs,
vol. 67, 26.'
mla: Henzinger, Monika H., et al. “Conditional Hardness for Sensitivity Problems.”
8th Innovations in Theoretical Computer Science Conference, vol. 67, 26,
Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017, doi:10.4230/LIPICS.ITCS.2017.26.
short: M.H. Henzinger, A. Lincoln, S. Neumann, V. Vassilevska Williams, in:, 8th
Innovations in Theoretical Computer Science Conference, Schloss Dagstuhl - Leibniz-Zentrum
für Informatik, 2017.
conference:
end_date: 2017-01-11
location: Berkley, CA, United States
name: 'ITCS: Innovations in Theoretical Computer Science Conference'
start_date: 2017-01-09
date_created: 2022-08-12T08:55:33Z
date_published: 2017-11-28T00:00:00Z
date_updated: 2023-02-16T11:49:15Z
day: '28'
doi: 10.4230/LIPICS.ITCS.2017.26
extern: '1'
external_id:
arxiv:
- '1703.01638'
intvolume: ' 67'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.4230/LIPICS.ITCS.2017.26
month: '11'
oa: 1
oa_version: Published Version
publication: 8th Innovations in Theoretical Computer Science Conference
publication_identifier:
isbn:
- '9783959770293'
issn:
- 1868-8969
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
scopus_import: '1'
status: public
title: Conditional hardness for sensitivity problems
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 67
year: '2017'
...
---
_id: '11833'
abstract:
- lang: eng
text: "We introduce a new algorithmic framework for designing dynamic graph algorithms
in minor-free graphs, by exploiting the structure of such graphs and a tool called
vertex sparsification, which is a way to compress large graphs into small ones
that well preserve relevant properties among a subset of vertices and has previously
mainly been used in the design of approximation algorithms.\r\n\r\nUsing this
framework, we obtain a Monte Carlo randomized fully dynamic algorithm for (1 +
epsilon)-approximating the energy of electrical flows in n-vertex planar graphs
with tilde{O}(r epsilon^{-2}) worst-case update time and tilde{O}((r + n / sqrt{r})
epsilon^{-2}) worst-case query time, for any r larger than some constant. For
r=n^{2/3}, this gives tilde{O}(n^{2/3} epsilon^{-2}) update time and tilde{O}(n^{2/3}
epsilon^{-2}) query time. We also extend this algorithm to work for minor-free
graphs with similar approximation and running time guarantees. Furthermore, we
illustrate our framework on the all-pairs max flow and shortest path problems
by giving corresponding dynamic algorithms in minor-free graphs with both sublinear
update and query times. To the best of our knowledge, our results are the first
to systematically establish such a connection between dynamic graph algorithms
and vertex sparsification.\r\n\r\nWe also present both upper bound and lower bound
for maintaining the energy of electrical flows in the incremental subgraph model,
where updates consist of only vertex activations, which might be of independent
interest."
alternative_title:
- LIPIcs
article_number: '45'
article_processing_charge: No
author:
- first_name: Gramoz
full_name: Goranci, Gramoz
last_name: Goranci
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: Pan
full_name: Peng, Pan
last_name: Peng
citation:
ama: 'Goranci G, Henzinger MH, Peng P. The power of vertex sparsifiers in dynamic
graph algorithms. In: 25th Annual European Symposium on Algorithms. Vol
87. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2017. doi:10.4230/LIPICS.ESA.2017.45'
apa: 'Goranci, G., Henzinger, M. H., & Peng, P. (2017). The power of vertex
sparsifiers in dynamic graph algorithms. In 25th Annual European Symposium
on Algorithms (Vol. 87). Vienna, Austria: Schloss Dagstuhl - Leibniz-Zentrum
für Informatik. https://doi.org/10.4230/LIPICS.ESA.2017.45'
chicago: Goranci, Gramoz, Monika H Henzinger, and Pan Peng. “The Power of Vertex
Sparsifiers in Dynamic Graph Algorithms.” In 25th Annual European Symposium
on Algorithms, Vol. 87. Schloss Dagstuhl - Leibniz-Zentrum für Informatik,
2017. https://doi.org/10.4230/LIPICS.ESA.2017.45.
ieee: G. Goranci, M. H. Henzinger, and P. Peng, “The power of vertex sparsifiers
in dynamic graph algorithms,” in 25th Annual European Symposium on Algorithms,
Vienna, Austria, 2017, vol. 87.
ista: 'Goranci G, Henzinger MH, Peng P. 2017. The power of vertex sparsifiers in
dynamic graph algorithms. 25th Annual European Symposium on Algorithms. ESA: Annual
European Symposium on Algorithms, LIPIcs, vol. 87, 45.'
mla: Goranci, Gramoz, et al. “The Power of Vertex Sparsifiers in Dynamic Graph Algorithms.”
25th Annual European Symposium on Algorithms, vol. 87, 45, Schloss Dagstuhl
- Leibniz-Zentrum für Informatik, 2017, doi:10.4230/LIPICS.ESA.2017.45.
short: G. Goranci, M.H. Henzinger, P. Peng, in:, 25th Annual European Symposium
on Algorithms, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017.
conference:
end_date: 2017-09-06
location: Vienna, Austria
name: 'ESA: Annual European Symposium on Algorithms'
start_date: 2017-09-04
date_created: 2022-08-12T10:46:26Z
date_published: 2017-09-01T00:00:00Z
date_updated: 2023-02-16T11:56:37Z
day: '01'
doi: 10.4230/LIPICS.ESA.2017.45
extern: '1'
external_id:
arxiv:
- '1712.06473'
intvolume: ' 87'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.4230/LIPIcs.ESA.2017.45
month: '09'
oa: 1
oa_version: Published Version
publication: 25th Annual European Symposium on Algorithms
publication_identifier:
isbn:
- 978-3-95977-049-1
issn:
- 1868-8969
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
scopus_import: '1'
status: public
title: The power of vertex sparsifiers in dynamic graph algorithms
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 87
year: '2017'
...