---
_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: '1112'
abstract:
- lang: eng
text: There has been renewed interest in modelling the behaviour of evolutionary
algorithms by more traditional mathematical objects, such as ordinary differential
equations or Markov chains. The advantage is that the analysis becomes greatly
facilitated due to the existence of well established methods. However, this typically
comes at the cost of disregarding information about the process. Here, we introduce
the use of stochastic differential equations (SDEs) for the study of EAs. SDEs
can produce simple analytical results for the dynamics of stochastic processes,
unlike Markov chains which can produce rigorous but unwieldy expressions about
the dynamics. On the other hand, unlike ordinary differential equations (ODEs),
they do not discard information about the stochasticity of the process. We show
that these are especially suitable for the analysis of fixed budget scenarios
and present analogs of the additive and multiplicative drift theorems for SDEs.
We exemplify the use of these methods for two model algorithms ((1+1) EA and RLS)
on two canonical problems(OneMax and LeadingOnes).
author:
- first_name: Tiago
full_name: Paixao, Tiago
id: 2C5658E6-F248-11E8-B48F-1D18A9856A87
last_name: Paixao
orcid: 0000-0003-2361-3953
- first_name: Jorge
full_name: Pérez Heredia, Jorge
last_name: Pérez Heredia
citation:
ama: 'Paixao T, Pérez Heredia J. An application of stochastic differential equations
to evolutionary algorithms. In: Proceedings of the 14th ACM/SIGEVO Conference
on Foundations of Genetic Algorithms. ACM; 2017:3-11. doi:10.1145/3040718.3040729'
apa: 'Paixao, T., & Pérez Heredia, J. (2017). An application of stochastic differential
equations to evolutionary algorithms. In Proceedings of the 14th ACM/SIGEVO
Conference on Foundations of Genetic Algorithms (pp. 3–11). Copenhagen, Denmark:
ACM. https://doi.org/10.1145/3040718.3040729'
chicago: Paixao, Tiago, and Jorge Pérez Heredia. “An Application of Stochastic Differential
Equations to Evolutionary Algorithms.” In Proceedings of the 14th ACM/SIGEVO
Conference on Foundations of Genetic Algorithms, 3–11. ACM, 2017. https://doi.org/10.1145/3040718.3040729.
ieee: T. Paixao and J. Pérez Heredia, “An application of stochastic differential
equations to evolutionary algorithms,” in Proceedings of the 14th ACM/SIGEVO
Conference on Foundations of Genetic Algorithms, Copenhagen, Denmark, 2017,
pp. 3–11.
ista: 'Paixao T, Pérez Heredia J. 2017. An application of stochastic differential
equations to evolutionary algorithms. Proceedings of the 14th ACM/SIGEVO Conference
on Foundations of Genetic Algorithms. FOGA: Foundations of Genetic Algorithms,
3–11.'
mla: Paixao, Tiago, and Jorge Pérez Heredia. “An Application of Stochastic Differential
Equations to Evolutionary Algorithms.” Proceedings of the 14th ACM/SIGEVO Conference
on Foundations of Genetic Algorithms, ACM, 2017, pp. 3–11, doi:10.1145/3040718.3040729.
short: T. Paixao, J. Pérez Heredia, in:, Proceedings of the 14th ACM/SIGEVO Conference
on Foundations of Genetic Algorithms, ACM, 2017, pp. 3–11.
conference:
end_date: 2017-01-15
location: Copenhagen, Denmark
name: 'FOGA: Foundations of Genetic Algorithms'
start_date: 2017-01-12
date_created: 2018-12-11T11:50:12Z
date_published: 2017-01-12T00:00:00Z
date_updated: 2021-01-12T06:48:22Z
day: '12'
department:
- _id: NiBa
doi: 10.1145/3040718.3040729
language:
- iso: eng
month: '01'
oa_version: None
page: 3 - 11
publication: Proceedings of the 14th ACM/SIGEVO Conference on Foundations of Genetic
Algorithms
publication_identifier:
isbn:
- 978-145034651-1
publication_status: published
publisher: ACM
publist_id: '6255'
quality_controlled: '1'
scopus_import: 1
status: public
title: An application of stochastic differential equations to evolutionary algorithms
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
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'
...