---
_id: '11615'
abstract:
- lang: eng
text: The recently published Kepler mission Data Release 25 (DR25) reported on ∼197 000
targets observed during the mission. Despite this, no wide search for red giants
showing solar-like oscillations have been made across all stars observed in Kepler’s
long-cadence mode. In this work, we perform this task using custom apertures on
the Kepler pixel files and detect oscillations in 21 914 stars, representing the
largest sample of solar-like oscillating stars to date. We measure their frequency
at maximum power, νmax, down to νmax≃4μHz and obtain log (g) estimates with a
typical uncertainty below 0.05 dex, which is superior to typical measurements
from spectroscopy. Additionally, the νmax distribution of our detections show
good agreement with results from a simulated model of the Milky Way, with a ratio
of observed to predicted stars of 0.992 for stars with 10<νmax<270μHz. Among our
red giant detections, we find 909 to be dwarf/subgiant stars whose flux signal
is polluted by a neighbouring giant as a result of using larger photometric apertures
than those used by the NASA Kepler science processing pipeline. We further find
that only 293 of the polluting giants are known Kepler targets. The remainder
comprises over 600 newly identified oscillating red giants, with many expected
to belong to the Galactic halo, serendipitously falling within the Kepler pixel
files of targeted stars.
acknowledgement: Funding for this Discovery mission is provided by NASA’s Science
mission Directorate. We thank the entire Kepler team without whom this investigation
would not be possible. DS is the recipient of an Australian Research Council Future
Fellowship (project number FT1400147). RAG acknowledges the support from CNES. SM
acknowledges support from NASA grant NNX15AF13G, NSF grant AST-1411685, and the
Ramon y Cajal fellowship number RYC-2015-17697. ILC acknowledges scholarship support
from the University of Sydney. We would like to thank Nicholas Barbara and Timothy
Bedding for providing us with a list of variable stars that helped to validate a
number of detections in this study. We also thank the group at the University of
Sydney for fruitful discussions. Finally, we gratefully acknowledge the support
of NVIDIA Corporation with the donation of the Titan Xp GPU used for this research.
article_processing_charge: No
article_type: original
author:
- first_name: Marc
full_name: Hon, Marc
last_name: Hon
- first_name: Dennis
full_name: Stello, Dennis
last_name: Stello
- first_name: Rafael A
full_name: García, Rafael A
last_name: García
- first_name: Savita
full_name: Mathur, Savita
last_name: Mathur
- first_name: Sanjib
full_name: Sharma, Sanjib
last_name: Sharma
- first_name: Isabel L
full_name: Colman, Isabel L
last_name: Colman
- first_name: Lisa Annabelle
full_name: Bugnet, Lisa Annabelle
id: d9edb345-f866-11ec-9b37-d119b5234501
last_name: Bugnet
orcid: 0000-0003-0142-4000
citation:
ama: Hon M, Stello D, García RA, et al. A search for red giant solar-like oscillations
in all Kepler data. Monthly Notices of the Royal Astronomical Society.
2019;485(4):5616-5630. doi:10.1093/mnras/stz622
apa: Hon, M., Stello, D., García, R. A., Mathur, S., Sharma, S., Colman, I. L.,
& Bugnet, L. A. (2019). A search for red giant solar-like oscillations in
all Kepler data. Monthly Notices of the Royal Astronomical Society. Oxford
University Press. https://doi.org/10.1093/mnras/stz622
chicago: Hon, Marc, Dennis Stello, Rafael A García, Savita Mathur, Sanjib Sharma,
Isabel L Colman, and Lisa Annabelle Bugnet. “A Search for Red Giant Solar-like
Oscillations in All Kepler Data.” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2019. https://doi.org/10.1093/mnras/stz622.
ieee: M. Hon et al., “A search for red giant solar-like oscillations in all
Kepler data,” Monthly Notices of the Royal Astronomical Society, vol. 485,
no. 4. Oxford University Press, pp. 5616–5630, 2019.
ista: Hon M, Stello D, García RA, Mathur S, Sharma S, Colman IL, Bugnet LA. 2019.
A search for red giant solar-like oscillations in all Kepler data. Monthly Notices
of the Royal Astronomical Society. 485(4), 5616–5630.
mla: Hon, Marc, et al. “A Search for Red Giant Solar-like Oscillations in All Kepler
Data.” Monthly Notices of the Royal Astronomical Society, vol. 485, no.
4, Oxford University Press, 2019, pp. 5616–30, doi:10.1093/mnras/stz622.
short: M. Hon, D. Stello, R.A. García, S. Mathur, S. Sharma, I.L. Colman, L.A. Bugnet,
Monthly Notices of the Royal Astronomical Society 485 (2019) 5616–5630.
date_created: 2022-07-18T14:26:03Z
date_published: 2019-06-01T00:00:00Z
date_updated: 2022-08-22T07:35:19Z
day: '01'
doi: 10.1093/mnras/stz622
extern: '1'
external_id:
arxiv:
- '1903.00115'
intvolume: ' 485'
issue: '4'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- asteroseismology
- 'methods: data analysis'
- 'techniques: image processing'
- 'stars: oscillations'
- 'stars: statistics'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1903.00115
month: '06'
oa: 1
oa_version: Preprint
page: 5616-5630
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 search for red giant solar-like oscillations in all Kepler data
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 485
year: '2019'
...
---
_id: '11614'
abstract:
- lang: eng
text: The NASA Transiting Exoplanet Survey Satellite (TESS) is about to provide
full-frame images of almost the entire sky. The amount of stellar data to be analysed
represents hundreds of millions stars, which is several orders of magnitude more
than the number of stars observed by the Convection, Rotation and planetary Transits
satellite (CoRoT), and NASA Kepler and K2 missions. We aim at automatically classifying
the newly observed stars with near real-time algorithms to better guide the subsequent
detailed studies. In this paper, we present a classification algorithm built to
recognise solar-like pulsators among classical pulsators. This algorithm relies
on the global amount of power contained in the power spectral density (PSD), also
known as the flicker in spectral power density (FliPer). Because each type of
pulsating star has a characteristic background or pulsation pattern, the shape
of the PSD at different frequencies can be used to characterise the type of pulsating
star. The FliPer classifier (FliPerClass) uses different FliPer parameters along
with the effective temperature as input parameters to feed a ML algorithm in order
to automatically classify the pulsating stars observed by TESS. Using noisy TESS-simulated
data from the TESS Asteroseismic Science Consortium (TASC), we classify pulsators
with a 98% accuracy. Among them, solar-like pulsating stars are recognised with
a 99% accuracy, which is of great interest for a further seismic analysis of these
stars, which are like our Sun. Similar results are obtained when we trained our
classifier and applied it to 27-day subsets of real Kepler data. FliPerClass is
part of the large TASC classification pipeline developed by the TESS Data for
Asteroseismology (T’DA) classification working group.
acknowledgement: We thank the enitre T’DA team for useful comments and discussions,
in particular Andrew Tkachenko. We also acknowledge Marc Hon, Keaton Bell, and James
Kuszlewicz for useful comments on the manuscript. L.B. and R.A.G. acknowledge the
support from PLATO and GOLF CNES grants. S.M. acknowledges support by the Ramon
y Cajal fellowship number RYC-2015-17697. O.J.H. and B.M.R. acknowledge the support
of the UK Science and Technology Facilities Council (STFC). M.N.L. acknowledges
the support of the ESA PRODEX programme (PEA 4000119301). Funding for the Stellar
Astrophysics Centre is provided by the Danish National Research Foundation (Grant
DNRF106).
article_number: A79
article_processing_charge: No
article_type: original
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: García, R. A.
last_name: García
- first_name: S.
full_name: Mathur, S.
last_name: Mathur
- first_name: G. R.
full_name: Davies, G. R.
last_name: Davies
- first_name: O. J.
full_name: Hall, O. J.
last_name: Hall
- first_name: M. N.
full_name: Lund, M. N.
last_name: Lund
- first_name: B. M.
full_name: Rendle, B. M.
last_name: Rendle
citation:
ama: 'Bugnet LA, García RA, Mathur S, et al. FliPerClass: In search of solar-like
pulsators among TESS targets. Astronomy & Astrophysics. 2019;624. doi:10.1051/0004-6361/201834780'
apa: 'Bugnet, L. A., García, R. A., Mathur, S., Davies, G. R., Hall, O. J., Lund,
M. N., & Rendle, B. M. (2019). FliPerClass: In search of solar-like pulsators
among TESS targets. Astronomy & Astrophysics. EDP Science. https://doi.org/10.1051/0004-6361/201834780'
chicago: 'Bugnet, Lisa Annabelle, R. A. García, S. Mathur, G. R. Davies, O. J. Hall,
M. N. Lund, and B. M. Rendle. “FliPerClass: In Search of Solar-like Pulsators
among TESS Targets.” Astronomy & Astrophysics. EDP Science, 2019. https://doi.org/10.1051/0004-6361/201834780.'
ieee: 'L. A. Bugnet et al., “FliPerClass: In search of solar-like pulsators
among TESS targets,” Astronomy & Astrophysics, vol. 624. EDP Science,
2019.'
ista: 'Bugnet LA, García RA, Mathur S, Davies GR, Hall OJ, Lund MN, Rendle BM. 2019.
FliPerClass: In search of solar-like pulsators among TESS targets. Astronomy &
Astrophysics. 624, A79.'
mla: 'Bugnet, Lisa Annabelle, et al. “FliPerClass: In Search of Solar-like Pulsators
among TESS Targets.” Astronomy & Astrophysics, vol. 624, A79, EDP Science,
2019, doi:10.1051/0004-6361/201834780.'
short: L.A. Bugnet, R.A. García, S. Mathur, G.R. Davies, O.J. Hall, M.N. Lund, B.M.
Rendle, Astronomy & Astrophysics 624 (2019).
date_created: 2022-07-18T14:13:34Z
date_published: 2019-04-19T00:00:00Z
date_updated: 2022-08-22T07:32:51Z
day: '19'
doi: 10.1051/0004-6361/201834780
extern: '1'
external_id:
arxiv:
- '1902.09854'
intvolume: ' 624'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1902.09854
month: '04'
oa: 1
oa_version: Preprint
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Science
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'FliPerClass: In search of solar-like pulsators among TESS targets'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 624
year: '2019'
...
---
_id: '11623'
abstract:
- lang: eng
text: Brightness variations due to dark spots on the stellar surface encode information
about stellar surface rotation and magnetic activity. In this work, we analyze
the Kepler long-cadence data of 26,521 main-sequence stars of spectral types M
and K in order to measure their surface rotation and photometric activity level.
Rotation-period estimates are obtained by the combination of a wavelet analysis
and autocorrelation function of the light curves. Reliable rotation estimates
are determined by comparing the results from the different rotation diagnostics
and four data sets. We also measure the photometric activity proxy Sph using the
amplitude of the flux variations on an appropriate timescale. We report rotation
periods and photometric activity proxies for about 60% of the sample, including
4431 targets for which McQuillan et al. did not report a rotation period. For
the common targets with rotation estimates in this study and in McQuillan et al.,
our rotation periods agree within 99%. In this work, we also identify potential
polluters, such as misclassified red giants and classical pulsator candidates.
Within the parameter range we study, there is a mild tendency for hotter stars
to have shorter rotation periods. The photometric activity proxy spans a wider
range of values with increasing effective temperature. The rotation period and
photometric activity proxy are also related, with Sph being larger for fast rotators.
Similar to McQuillan et al., we find a bimodal distribution of rotation periods.
acknowledgement: "The authors thank Róbert Szabó Paul G. Beck, Katrien Kolenberg,
and Isabel L. Colman for helping on the classification of stars. This paper includes
data collected by the Kepler mission and obtained from the MAST data archive at
the Space Telescope Science Institute (STScI). Funding for the Kepler mission is
provided by the National Aeronautics and Space Administration (NASA) Science Mission
Directorate. STScI is operated by the Association of Universities for Research in
Astronomy, Inc., under NASA contract NAS 5–26555. A.R.G.S. acknowledges the support
from NASA under grant NNX17AF27G. R.A.G. and L.B. acknowledge the support from PLATO
and GOLF CNES grants. S.M. acknowledges the support from the Ramon y Cajal fellowship
number RYC-2015-17697. T.S.M. acknowledges support from a Visiting Fellowship at
the Max Planck Institute for Solar System Research. This research has made use of
the NASA Exoplanet Archive, which is operated by the California Institute of Technology,
under contract with the National Aeronautics and Space Administration under the
Exoplanet Exploration Program.\r\n\r\nSoftware: KADACS (García et al. 2011), NumPy
(van der Walt et al. 2011), SciPy (Jones et al. 2001), Matplotlib (Hunter 2007).\r\n\r\nFacilities:
MAST - , Kepler Eclipsing Binary Catalog - , Exoplanet Archive. -"
article_number: '21'
article_processing_charge: No
article_type: original
author:
- first_name: A. R. G.
full_name: Santos, A. R. G.
last_name: Santos
- first_name: R. A.
full_name: García, R. A.
last_name: García
- first_name: S.
full_name: Mathur, S.
last_name: Mathur
- 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: J. L.
full_name: van Saders, J. L.
last_name: van Saders
- first_name: T. S.
full_name: Metcalfe, T. S.
last_name: Metcalfe
- first_name: G. V. A.
full_name: Simonian, G. V. A.
last_name: Simonian
- first_name: M. H.
full_name: Pinsonneault, M. H.
last_name: Pinsonneault
citation:
ama: Santos ARG, García RA, Mathur S, et al. Surface rotation and photometric activity
for Kepler targets. I. M and K main-sequence stars. The Astrophysical Journal
Supplement Series. 2019;244(1). doi:10.3847/1538-4365/ab3b56
apa: Santos, A. R. G., García, R. A., Mathur, S., Bugnet, L. A., van Saders, J.
L., Metcalfe, T. S., … Pinsonneault, M. H. (2019). Surface rotation and photometric
activity for Kepler targets. I. M and K main-sequence stars. The Astrophysical
Journal Supplement Series. IOP Publishing. https://doi.org/10.3847/1538-4365/ab3b56
chicago: Santos, A. R. G., R. A. García, S. Mathur, Lisa Annabelle Bugnet, J. L.
van Saders, T. S. Metcalfe, G. V. A. Simonian, and M. H. Pinsonneault. “Surface
Rotation and Photometric Activity for Kepler Targets. I. M and K Main-Sequence
Stars.” The Astrophysical Journal Supplement Series. IOP Publishing, 2019.
https://doi.org/10.3847/1538-4365/ab3b56.
ieee: A. R. G. Santos et al., “Surface rotation and photometric activity
for Kepler targets. I. M and K main-sequence stars,” The Astrophysical Journal
Supplement Series, vol. 244, no. 1. IOP Publishing, 2019.
ista: Santos ARG, García RA, Mathur S, Bugnet LA, van Saders JL, Metcalfe TS, Simonian
GVA, Pinsonneault MH. 2019. Surface rotation and photometric activity for Kepler
targets. I. M and K main-sequence stars. The Astrophysical Journal Supplement
Series. 244(1), 21.
mla: Santos, A. R. G., et al. “Surface Rotation and Photometric Activity for Kepler
Targets. I. M and K Main-Sequence Stars.” The Astrophysical Journal Supplement
Series, vol. 244, no. 1, 21, IOP Publishing, 2019, doi:10.3847/1538-4365/ab3b56.
short: A.R.G. Santos, R.A. García, S. Mathur, L.A. Bugnet, J.L. van Saders, T.S.
Metcalfe, G.V.A. Simonian, M.H. Pinsonneault, The Astrophysical Journal Supplement
Series 244 (2019).
date_created: 2022-07-19T09:21:58Z
date_published: 2019-09-19T00:00:00Z
date_updated: 2022-08-22T08:10:38Z
day: '19'
doi: 10.3847/1538-4365/ab3b56
extern: '1'
external_id:
arxiv:
- '1908.05222'
intvolume: ' 244'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'methods: data analysis'
- 'stars: activity'
- 'stars: low-mass'
- 'stars: rotation'
- starspots
- 'techniques: photometric'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1908.05222
month: '09'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal Supplement Series
publication_identifier:
issn:
- 0067-0049
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Surface rotation and photometric activity for Kepler targets. I. M and K main-sequence
stars
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 244
year: '2019'
...
---
_id: '11627'
abstract:
- lang: eng
text: 'For a solar-like star, the surface rotation evolves with time, allowing in
principle to estimate the age of a star from its surface rotation period. Here
we are interested in measuring surface rotation periods of solar-like stars observed
by the NASA mission Kepler. Different methods have been developed to track rotation
signals in Kepler photometric light curves: time-frequency analysis based on wavelet
techniques, autocorrelation and composite spectrum. We use the learning abilities
of random forest classifiers to take decisions during two crucial steps of the
analysis. First, given some input parameters, we discriminate the considered Kepler
targets between rotating MS stars, non-rotating MS stars, red giants, binaries
and pulsators. We then use a second classifier only on the MS rotating targets
to decide the best data analysis treatment.'
article_number: '1906.09609'
article_processing_charge: No
author:
- first_name: S. N.
full_name: Breton, S. N.
last_name: Breton
- 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: A. R. G.
full_name: Santos, A. R. G.
last_name: Santos
- first_name: A. Le
full_name: Saux, A. Le
last_name: Saux
- first_name: S.
full_name: Mathur, S.
last_name: Mathur
- first_name: P. L.
full_name: Palle, P. L.
last_name: Palle
- first_name: R. A.
full_name: Garcia, R. A.
last_name: Garcia
citation:
ama: Breton SN, Bugnet LA, Santos ARG, et al. Determining surface rotation periods
of solar-like stars observed by the Kepler mission using machine learning techniques.
arXiv. doi:10.48550/arXiv.1906.09609
apa: Breton, S. N., Bugnet, L. A., Santos, A. R. G., Saux, A. L., Mathur, S., Palle,
P. L., & Garcia, R. A. (n.d.). Determining surface rotation periods of solar-like
stars observed by the Kepler mission using machine learning techniques. arXiv.
https://doi.org/10.48550/arXiv.1906.09609
chicago: Breton, S. N., Lisa Annabelle Bugnet, A. R. G. Santos, A. Le Saux, S. Mathur,
P. L. Palle, and R. A. Garcia. “Determining Surface Rotation Periods of Solar-like
Stars Observed by the Kepler Mission Using Machine Learning Techniques.” ArXiv,
n.d. https://doi.org/10.48550/arXiv.1906.09609.
ieee: S. N. Breton et al., “Determining surface rotation periods of solar-like
stars observed by the Kepler mission using machine learning techniques,” arXiv.
.
ista: Breton SN, Bugnet LA, Santos ARG, Saux AL, Mathur S, Palle PL, Garcia RA.
Determining surface rotation periods of solar-like stars observed by the Kepler
mission using machine learning techniques. arXiv, 1906.09609.
mla: Breton, S. N., et al. “Determining Surface Rotation Periods of Solar-like Stars
Observed by the Kepler Mission Using Machine Learning Techniques.” ArXiv,
1906.09609, doi:10.48550/arXiv.1906.09609.
short: S.N. Breton, L.A. Bugnet, A.R.G. Santos, A.L. Saux, S. Mathur, P.L. Palle,
R.A. Garcia, ArXiv (n.d.).
date_created: 2022-07-20T11:18:53Z
date_published: 2019-06-23T00:00:00Z
date_updated: 2022-08-22T08:16:53Z
day: '23'
doi: 10.48550/arXiv.1906.09609
extern: '1'
external_id:
arxiv:
- '1906.09609'
keyword:
- asteroseismology
- rotation
- solar-like stars
- kepler
- machine learning
- random forest
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1906.09609
month: '06'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: Determining surface rotation periods of solar-like stars observed by the Kepler
mission using machine learning techniques
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...
---
_id: '11630'
abstract:
- lang: eng
text: 'The second mission of NASA’s Kepler satellite, K2, has collected hundreds
of thousands of lightcurves for stars close to the ecliptic plane. This new sample
could increase the number of known pulsating stars and then improve our understanding
of those stars. For the moment only a few stars have been properly classified
and published. In this work, we present a method to automaticly classify K2 pulsating
stars using a Machine Learning technique called Random Forest. The objective is
to sort out the stars in four classes: red giant (RG), main-sequence Solar-like
stars (SL), classical pulsators (PULS) and Other. To do this we use the effective
temperatures and the luminosities of the stars as well as the FliPer features,
that measures the amount of power contained in the power spectral density. The
classifier now retrieves the right classification for more than 80% of the stars.'
article_number: '1906.09611'
article_processing_charge: No
author:
- first_name: A. Le
full_name: Saux, A. Le
last_name: Saux
- 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: S.
full_name: Mathur, S.
last_name: Mathur
- first_name: S. N.
full_name: Breton, S. N.
last_name: Breton
- first_name: R. A.
full_name: Garcia, R. A.
last_name: Garcia
citation:
ama: Saux AL, Bugnet LA, Mathur S, Breton SN, Garcia RA. Automatic classification
of K2 pulsating stars using machine learning techniques. arXiv. doi:10.48550/arXiv.1906.09611
apa: Saux, A. L., Bugnet, L. A., Mathur, S., Breton, S. N., & Garcia, R. A.
(n.d.). Automatic classification of K2 pulsating stars using machine learning
techniques. arXiv. https://doi.org/10.48550/arXiv.1906.09611
chicago: Saux, A. Le, Lisa Annabelle Bugnet, S. Mathur, S. N. Breton, and R. A.
Garcia. “Automatic Classification of K2 Pulsating Stars Using Machine Learning
Techniques.” ArXiv, n.d. https://doi.org/10.48550/arXiv.1906.09611.
ieee: A. L. Saux, L. A. Bugnet, S. Mathur, S. N. Breton, and R. A. Garcia, “Automatic
classification of K2 pulsating stars using machine learning techniques,” arXiv.
.
ista: Saux AL, Bugnet LA, Mathur S, Breton SN, Garcia RA. Automatic classification
of K2 pulsating stars using machine learning techniques. arXiv, 1906.09611.
mla: Saux, A. Le, et al. “Automatic Classification of K2 Pulsating Stars Using Machine
Learning Techniques.” ArXiv, 1906.09611, doi:10.48550/arXiv.1906.09611.
short: A.L. Saux, L.A. Bugnet, S. Mathur, S.N. Breton, R.A. Garcia, ArXiv (n.d.).
date_created: 2022-07-21T06:57:10Z
date_published: 2019-06-23T00:00:00Z
date_updated: 2022-08-22T08:20:29Z
day: '23'
doi: 10.48550/arXiv.1906.09611
extern: '1'
external_id:
arxiv:
- '1906.09611'
keyword:
- asteroseismology - methods
- data analysis - thecniques
- machine learning - stars
- oscillations
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.1906.09611
month: '06'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: Automatic classification of K2 pulsating stars using machine learning techniques
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...
---
_id: '11826'
abstract:
- lang: eng
text: "The diameter, radius and eccentricities are natural graph parameters. While
these problems have been studied extensively, there are no known dynamic algorithms
for them beyond the ones that follow from trivial recomputation after each update
or from solving dynamic All-Pairs Shortest Paths (APSP), which is very computationally
intensive. This is the situation for dynamic approximation algorithms as well,
and even if only edge insertions or edge deletions need to be supported.\r\nThis
paper provides a comprehensive study of the dynamic approximation of Diameter,
Radius and Eccentricities, providing both conditional lower bounds, and new algorithms
whose bounds are optimal under popular hypotheses in fine-grained complexity.
Some of the highlights include:\r\n- Under popular hardness hypotheses, there
can be no significantly better fully dynamic approximation algorithms than recomputing
the answer after each update, or maintaining full APSP.\r\n- Nearly optimal partially
dynamic (incremental/decremental) algorithms can be achieved via efficient reductions
to (incremental/decremental) maintenance of Single-Source Shortest Paths. For
instance, a nearly (3/2+epsilon)-approximation to Diameter in directed or undirected
n-vertex, m-edge graphs can be maintained decrementally in total time m^{1+o(1)}sqrt{n}/epsilon^2.
This nearly matches the static 3/2-approximation algorithm for the problem that
is known to be conditionally optimal."
alternative_title:
- LIPIcs
article_number: '13'
article_processing_charge: No
author:
- first_name: Bertie
full_name: Ancona, Bertie
last_name: Ancona
- 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: Liam
full_name: Roditty, Liam
last_name: Roditty
- first_name: Virginia Vassilevska
full_name: Williams, Virginia Vassilevska
last_name: Williams
- first_name: Nicole
full_name: Wein, Nicole
last_name: Wein
citation:
ama: 'Ancona B, Henzinger MH, Roditty L, Williams VV, Wein N. Algorithms and hardness
for diameter in dynamic graphs. In: 46th International Colloquium on Automata,
Languages, and Programming. Vol 132. Schloss Dagstuhl - Leibniz-Zentrum für
Informatik; 2019. doi:10.4230/LIPICS.ICALP.2019.13'
apa: 'Ancona, B., Henzinger, M. H., Roditty, L., Williams, V. V., & Wein, N.
(2019). Algorithms and hardness for diameter in dynamic graphs. In 46th International
Colloquium on Automata, Languages, and Programming (Vol. 132). Patras, Greece:
Schloss Dagstuhl - Leibniz-Zentrum für Informatik. https://doi.org/10.4230/LIPICS.ICALP.2019.13'
chicago: Ancona, Bertie, Monika H Henzinger, Liam Roditty, Virginia Vassilevska
Williams, and Nicole Wein. “Algorithms and Hardness for Diameter in Dynamic Graphs.”
In 46th International Colloquium on Automata, Languages, and Programming,
Vol. 132. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2019. https://doi.org/10.4230/LIPICS.ICALP.2019.13.
ieee: B. Ancona, M. H. Henzinger, L. Roditty, V. V. Williams, and N. Wein, “Algorithms
and hardness for diameter in dynamic graphs,” in 46th International Colloquium
on Automata, Languages, and Programming, Patras, Greece, 2019, vol. 132.
ista: 'Ancona B, Henzinger MH, Roditty L, Williams VV, Wein N. 2019. Algorithms
and hardness for diameter in dynamic graphs. 46th International Colloquium on
Automata, Languages, and Programming. ICALP: International Colloquium on Automata,
Languages, and Programming, LIPIcs, vol. 132, 13.'
mla: Ancona, Bertie, et al. “Algorithms and Hardness for Diameter in Dynamic Graphs.”
46th International Colloquium on Automata, Languages, and Programming,
vol. 132, 13, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2019, doi:10.4230/LIPICS.ICALP.2019.13.
short: B. Ancona, M.H. Henzinger, L. Roditty, V.V. Williams, N. Wein, in:, 46th
International Colloquium on Automata, Languages, and Programming, Schloss Dagstuhl
- Leibniz-Zentrum für Informatik, 2019.
conference:
end_date: 2019-07-12
location: Patras, Greece
name: 'ICALP: International Colloquium on Automata, Languages, and Programming'
start_date: 2019-07-09
date_created: 2022-08-12T08:14:51Z
date_published: 2019-07-04T00:00:00Z
date_updated: 2023-02-16T10:48:24Z
day: '04'
doi: 10.4230/LIPICS.ICALP.2019.13
extern: '1'
external_id:
arxiv:
- '811.12527'
intvolume: ' 132'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.4230/LIPIcs.ICALP.2019.13
month: '07'
oa: 1
oa_version: Published Version
publication: 46th International Colloquium on Automata, Languages, and Programming
publication_identifier:
isbn:
- 978-3-95977-109-2
issn:
- 1868-8969
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
scopus_import: '1'
status: public
title: Algorithms and hardness for diameter in dynamic graphs
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 132
year: '2019'
...
---
_id: '11850'
abstract:
- lang: eng
text: 'Modern networked systems are increasingly reconfigurable, enabling demand-aware
infrastructures whose resources can be adjusted according to the workload they
currently serve. Such dynamic adjustments can be exploited to improve network
utilization and hence performance, by moving frequently interacting communication
partners closer, e.g., collocating them in the same server or datacenter. However,
dynamically changing the embedding of workloads is algorithmically challenging:
communication patterns are often not known ahead of time, but must be learned.
During the learning process, overheads related to unnecessary moves (i.e., re-embeddings)
should be minimized. This paper studies a fundamental model which captures the
tradeoff between the benefits and costs of dynamically collocating communication
partners on l servers, in an online manner. Our main contribution is a distributed
online algorithm which is asymptotically almost optimal, i.e., almost matches
the lower bound (also derived in this paper) on the competitive ratio of any (distributed
or centralized) online algorithm.'
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: Stefan
full_name: Neumann, Stefan
last_name: Neumann
- first_name: Stefan
full_name: Schmid, Stefan
last_name: Schmid
citation:
ama: 'Henzinger MH, Neumann S, Schmid S. Efficient distributed workload (re-)embedding.
In: SIGMETRICS’19: International Conference on Measurement and Modeling of
Computer Systems. Association for Computing Machinery; 2019:43–44. doi:10.1145/3309697.3331503'
apa: 'Henzinger, M. H., Neumann, S., & Schmid, S. (2019). Efficient distributed
workload (re-)embedding. In SIGMETRICS’19: International Conference on Measurement
and Modeling of Computer Systems (pp. 43–44). Phoenix, AZ, United States:
Association for Computing Machinery. https://doi.org/10.1145/3309697.3331503'
chicago: 'Henzinger, Monika H, Stefan Neumann, and Stefan Schmid. “Efficient Distributed
Workload (Re-)Embedding.” In SIGMETRICS’19: International Conference on Measurement
and Modeling of Computer Systems, 43–44. Association for Computing Machinery,
2019. https://doi.org/10.1145/3309697.3331503.'
ieee: 'M. H. Henzinger, S. Neumann, and S. Schmid, “Efficient distributed workload
(re-)embedding,” in SIGMETRICS’19: International Conference on Measurement
and Modeling of Computer Systems, Phoenix, AZ, United States, 2019, pp. 43–44.'
ista: 'Henzinger MH, Neumann S, Schmid S. 2019. Efficient distributed workload (re-)embedding.
SIGMETRICS’19: International Conference on Measurement and Modeling of Computer
Systems. SIGMETRICS: International Conference on Measurement and Modeling of Computer
Systems, 43–44.'
mla: 'Henzinger, Monika H., et al. “Efficient Distributed Workload (Re-)Embedding.”
SIGMETRICS’19: International Conference on Measurement and Modeling of Computer
Systems, Association for Computing Machinery, 2019, pp. 43–44, doi:10.1145/3309697.3331503.'
short: 'M.H. Henzinger, S. Neumann, S. Schmid, in:, SIGMETRICS’19: International
Conference on Measurement and Modeling of Computer Systems, Association for Computing
Machinery, 2019, pp. 43–44.'
conference:
end_date: 2019-06-28
location: Phoenix, AZ, United States
name: 'SIGMETRICS: International Conference on Measurement and Modeling of Computer
Systems'
start_date: 2019-06-24
date_created: 2022-08-16T07:14:57Z
date_published: 2019-06-20T00:00:00Z
date_updated: 2023-02-17T09:41:45Z
day: '20'
doi: 10.1145/3309697.3331503
extern: '1'
external_id:
arxiv:
- '1904.05474'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1904.05474
month: '06'
oa: 1
oa_version: Preprint
page: 43–44
publication: 'SIGMETRICS''19: International Conference on Measurement and Modeling
of Computer Systems'
publication_identifier:
isbn:
- 978-1-4503-6678-6
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: Efficient distributed workload (re-)embedding
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...
---
_id: '11853'
abstract:
- lang: eng
text: We present a deterministic dynamic algorithm for maintaining a (1+ε)f-approximate
minimum cost set cover with O(f log(Cn)/ε^2) amortized update time, when the input
set system is undergoing element insertions and deletions. Here, n denotes the
number of elements, each element appears in at most f sets, and the cost of each
set lies in the range [1/C, 1]. Our result, together with that of Gupta~et~al.~[STOC'17],
implies that there is a deterministic algorithm for this problem with O(f log(Cn))
amortized update time and O(min(log n, f)) -approximation ratio, which nearly
matches the polynomial-time hardness of approximation for minimum set cover in
the static setting. Our update time is only O(log (Cn)) away from a trivial lower
bound. Prior to our work, the previous best approximation ratio guaranteed by
deterministic algorithms was O(f^2), which was due to Bhattacharya~et~al.~[ICALP`15].
In contrast, the only result that guaranteed O(f) -approximation was obtained
very recently by Abboud~et~al.~[STOC`19], who designed a dynamic algorithm with
(1+ε)f-approximation ratio and O(f^2 log n/ε) amortized update time. Besides the
extra O(f) factor in the update time compared to our and Gupta~et~al.'s results,
the Abboud~et~al.~algorithm is randomized, and works only when the adversary is
oblivious and the sets are unweighted (each set has the same cost). We achieve
our result via the primal-dual approach, by maintaining a fractional packing solution
as a dual certificate. This approach was pursued previously by Bhattacharya~et~al.~and
Gupta~et~al., but not in the recent paper by Abboud~et~al. Unlike previous primal-dual
algorithms that try to satisfy some local constraints for individual sets at all
time, our algorithm basically waits until the dual solution changes significantly
globally, and fixes the solution only where the fix is needed.
article_processing_charge: No
author:
- first_name: Sayan
full_name: Bhattacharya, Sayan
last_name: Bhattacharya
- 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: Danupon
full_name: Nanongkai, Danupon
last_name: Nanongkai
citation:
ama: 'Bhattacharya S, Henzinger MH, Nanongkai D. A new deterministic algorithm for
dynamic set cover. In: 60th Annual Symposium on Foundations of Computer Science.
Institute of Electrical and Electronics Engineers; 2019:406-423. doi:10.1109/focs.2019.00033'
apa: 'Bhattacharya, S., Henzinger, M. H., & Nanongkai, D. (2019). A new deterministic
algorithm for dynamic set cover. In 60th Annual Symposium on Foundations of
Computer Science (pp. 406–423). Baltimore, MD, United States: Institute of
Electrical and Electronics Engineers. https://doi.org/10.1109/focs.2019.00033'
chicago: Bhattacharya, Sayan, Monika H Henzinger, and Danupon Nanongkai. “A New
Deterministic Algorithm for Dynamic Set Cover.” In 60th Annual Symposium on
Foundations of Computer Science, 406–23. Institute of Electrical and Electronics
Engineers, 2019. https://doi.org/10.1109/focs.2019.00033.
ieee: S. Bhattacharya, M. H. Henzinger, and D. Nanongkai, “A new deterministic algorithm
for dynamic set cover,” in 60th Annual Symposium on Foundations of Computer
Science, Baltimore, MD, United States, 2019, pp. 406–423.
ista: 'Bhattacharya S, Henzinger MH, Nanongkai D. 2019. A new deterministic algorithm
for dynamic set cover. 60th Annual Symposium on Foundations of Computer Science.
FOCS: Annual Symposium on Foundations of Computer Science, 406–423.'
mla: Bhattacharya, Sayan, et al. “A New Deterministic Algorithm for Dynamic Set
Cover.” 60th Annual Symposium on Foundations of Computer Science, Institute
of Electrical and Electronics Engineers, 2019, pp. 406–23, doi:10.1109/focs.2019.00033.
short: S. Bhattacharya, M.H. Henzinger, D. Nanongkai, in:, 60th Annual Symposium
on Foundations of Computer Science, Institute of Electrical and Electronics Engineers,
2019, pp. 406–423.
conference:
end_date: 2019-11-12
location: Baltimore, MD, United States
name: 'FOCS: Annual Symposium on Foundations of Computer Science'
start_date: 2019-11-09
date_created: 2022-08-16T08:00:00Z
date_published: 2019-11-01T00:00:00Z
date_updated: 2023-02-17T09:50:37Z
day: '01'
doi: 10.1109/focs.2019.00033
extern: '1'
external_id:
arxiv:
- '1909.11600'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1909.11600
month: '11'
oa: 1
oa_version: Preprint
page: 406-423
publication: 60th Annual Symposium on Foundations of Computer Science
publication_identifier:
eisbn:
- 978-1-7281-4952-3
isbn:
- 978-1-7281-4953-0
issn:
- 2575-8454
publication_status: published
publisher: Institute of Electrical and Electronics Engineers
quality_controlled: '1'
scopus_import: '1'
status: public
title: A new deterministic algorithm for dynamic set cover
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...
---
_id: '11865'
abstract:
- lang: eng
text: We present the first sublinear-time algorithm that can compute the edge connectivity
λ of a network exactly on distributed message-passing networks (the CONGEST model),
as long as the network contains no multi-edge. We present the first sublinear-time
algorithm for a distributed message-passing network sto compute its edge connectivity
λ exactly in the CONGEST model, as long as there are no parallel edges. Our algorithm
takes Õ(n1−1/353D1/353+n1−1/706) time to compute λ and a cut of cardinality λ
with high probability, where n and D are the number of nodes and the diameter
of the network, respectively, and Õ hides polylogarithmic factors. This running
time is sublinear in n (i.e. Õ(n1−є)) whenever D is. Previous sublinear-time distributed
algorithms can solve this problem either (i) exactly only when λ=O(n1/8−є) [Thurimella
PODC’95; Pritchard, Thurimella, ACM Trans. Algorithms’11; Nanongkai, Su, DISC’14]
or (ii) approximately [Ghaffari, Kuhn, DISC’13; Nanongkai, Su, DISC’14]. To achieve
this we develop and combine several new techniques. First, we design the first
distributed algorithm that can compute a k-edge connectivity certificate for any
k=O(n1−є) in time Õ(√nk+D). The previous sublinear-time algorithm can do so only
when k=o(√n) [Thurimella PODC’95]. In fact, our algorithm can be turned into the
first parallel algorithm with polylogarithmic depth and near-linear work. Previous
near-linear work algorithms are essentially sequential and previous polylogarithmic-depth
algorithms require Ω(mk) work in the worst case (e.g. [Karger, Motwani, STOC’93]).
Second, we show that by combining the recent distributed expander decomposition
technique of [Chang, Pettie, Zhang, SODA’19] with techniques from the sequential
deterministic edge connectivity algorithm of [Kawarabayashi, Thorup, STOC’15],
we can decompose the network into a sublinear number of clusters with small average
diameter and without any mincut separating a cluster (except the “trivial” ones).
This leads to a simplification of the Kawarabayashi-Thorup framework (except that
we are randomized while they are deterministic). This might make this framework
more useful in other models of computation. Finally, by extending the tree packing
technique from [Karger STOC’96], we can find the minimum cut in time proportional
to the number of components. As a byproduct of this technique, we obtain an Õ(n)-time
algorithm for computing exact minimum cut for weighted graphs.
article_processing_charge: No
author:
- first_name: Mohit
full_name: Daga, Mohit
last_name: Daga
- 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: Danupon
full_name: Nanongkai, Danupon
last_name: Nanongkai
- first_name: Thatchaphol
full_name: Saranurak, Thatchaphol
last_name: Saranurak
citation:
ama: 'Daga M, Henzinger MH, Nanongkai D, Saranurak T. Distributed edge connectivity
in sublinear time. In: Proceedings of the 51st Annual ACM SIGACT Symposium
on Theory of Computing. Association for Computing Machinery; 2019:343–354.
doi:10.1145/3313276.3316346'
apa: 'Daga, M., Henzinger, M. H., Nanongkai, D., & Saranurak, T. (2019). Distributed
edge connectivity in sublinear time. In Proceedings of the 51st Annual ACM
SIGACT Symposium on Theory of Computing (pp. 343–354). Phoenix, AZ, United
States: Association for Computing Machinery. https://doi.org/10.1145/3313276.3316346'
chicago: Daga, Mohit, Monika H Henzinger, Danupon Nanongkai, and Thatchaphol Saranurak.
“Distributed Edge Connectivity in Sublinear Time.” In Proceedings of the 51st
Annual ACM SIGACT Symposium on Theory of Computing, 343–354. Association for
Computing Machinery, 2019. https://doi.org/10.1145/3313276.3316346.
ieee: M. Daga, M. H. Henzinger, D. Nanongkai, and T. Saranurak, “Distributed edge
connectivity in sublinear time,” in Proceedings of the 51st Annual ACM SIGACT
Symposium on Theory of Computing, Phoenix, AZ, United States, 2019, pp. 343–354.
ista: 'Daga M, Henzinger MH, Nanongkai D, Saranurak T. 2019. Distributed edge connectivity
in sublinear time. Proceedings of the 51st Annual ACM SIGACT Symposium on Theory
of Computing. STOC: Symposium on Theory of Computing, 343–354.'
mla: Daga, Mohit, et al. “Distributed Edge Connectivity in Sublinear Time.” Proceedings
of the 51st Annual ACM SIGACT Symposium on Theory of Computing, Association
for Computing Machinery, 2019, pp. 343–354, doi:10.1145/3313276.3316346.
short: M. Daga, M.H. Henzinger, D. Nanongkai, T. Saranurak, in:, Proceedings of
the 51st Annual ACM SIGACT Symposium on Theory of Computing, Association for Computing
Machinery, 2019, pp. 343–354.
conference:
end_date: 2019-06-26
location: Phoenix, AZ, United States
name: 'STOC: Symposium on Theory of Computing'
start_date: 2019-06-23
date_created: 2022-08-16T09:11:17Z
date_published: 2019-06-01T00:00:00Z
date_updated: 2023-02-17T10:26:25Z
day: '01'
doi: 10.1145/3313276.3316346
extern: '1'
external_id:
arxiv:
- '1904.04341'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1904.04341
month: '06'
oa: 1
oa_version: Preprint
page: 343–354
publication: Proceedings of the 51st Annual ACM SIGACT Symposium on Theory of Computing
publication_identifier:
isbn:
- 978-1-4503-6705-9
issn:
- 0737-8017
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: Distributed edge connectivity in sublinear time
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...
---
_id: '11871'
abstract:
- lang: eng
text: "Many dynamic graph algorithms have an amortized update time, rather than
a stronger worst-case guarantee. But amortized data structures are not suitable
for real-time systems, where each individual operation has to be executed quickly.
For this reason, there exist many recent randomized results that aim to provide
a guarantee stronger than amortized expected. The strongest possible guarantee
for a randomized algorithm is that it is always correct (Las Vegas), and has high-probability
worst-case update time, which gives a bound on the time for each individual operation
that holds with high probability.\r\n\r\nIn this paper we present the first polylogarithmic
high-probability worst-case time bounds for the dynamic spanner and the dynamic
maximal matching problem.\r\n\r\n1.\t\r\nFor dynamic spanner, the only known o(n)
worst-case bounds were O(n3/4) high-probability worst-case update time for maintaining
a 3-spanner, and O(n5/9) for maintaining a 5-spanner. We give a O(1)k log3(n)
high-probability worst-case time bound for maintaining a (2k – 1)-spanner, which
yields the first worst-case polylog update time for all constant k. (All the results
above maintain the optimal tradeoff of stretch 2k – 1 and Õ(n1+1/k) edges.)\r\n\r\n2.\t\r\nFor
dynamic maximal matching, or dynamic 2-approximate maximum matching, no algorithm
with o(n) worst-case time bound was known and we present an algorithm with O(log5
(n)) high-probability worst-case time; similar worst-case bounds existed only
for maintaining a matching that was (2 + ∊)-approximate, and hence not maximal.\r\n\r\nOur
results are achieved using a new approach for converting amortized guarantees
to worst-case ones for randomized data structures by going through a third type
of guarantee, which is a middle ground between the two above: an algorithm is
said to have worst-case expected update time α if for every update σ, the expected
time to process σ is at most α. Although stronger than amortized expected, the
worst-case expected guarantee does not resolve the fundamental problem of amortization:
a worst-case expected update time of O(1) still allows for the possibility that
every 1/f(n) updates requires Θ(f(n)) time to process, for arbitrarily high f(n).
In this paper we present a black-box reduction that converts any data structure
with worst-case expected update time into one with a high-probability worst-case
update time: the query time remains the same, while the update time increases
by a factor of O(log2(n)).\r\n\r\nThus we achieve our results in two steps: (1)
First we show how to convert existing dynamic graph algorithms with amortized
expected polylogarithmic running times into algorithms with worst-case expected
polylogarithmic running times. (2) Then we use our black-box reduction to achieve
the polylogarithmic high-probability worst-case time bound. All our algorithms
are Las-Vegas-type algorithms."
article_processing_charge: No
author:
- first_name: Aaron
full_name: Bernstein, Aaron
last_name: Bernstein
- first_name: Sebastian
full_name: Forster, Sebastian
last_name: Forster
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
citation:
ama: 'Bernstein A, Forster S, Henzinger MH. A deamortization approach for dynamic
spanner and dynamic maximal matching. In: 30th Annual ACM-SIAM Symposium on
Discrete Algorithms. Society for Industrial and Applied Mathematics; 2019:1899-1918.
doi:10.1137/1.9781611975482.115'
apa: 'Bernstein, A., Forster, S., & Henzinger, M. H. (2019). A deamortization
approach for dynamic spanner and dynamic maximal matching. In 30th Annual ACM-SIAM
Symposium on Discrete Algorithms (pp. 1899–1918). San Diego, CA, United States:
Society for Industrial and Applied Mathematics. https://doi.org/10.1137/1.9781611975482.115'
chicago: Bernstein, Aaron, Sebastian Forster, and Monika H Henzinger. “A Deamortization
Approach for Dynamic Spanner and Dynamic Maximal Matching.” In 30th Annual
ACM-SIAM Symposium on Discrete Algorithms, 1899–1918. Society for Industrial
and Applied Mathematics, 2019. https://doi.org/10.1137/1.9781611975482.115.
ieee: A. Bernstein, S. Forster, and M. H. Henzinger, “A deamortization approach
for dynamic spanner and dynamic maximal matching,” in 30th Annual ACM-SIAM
Symposium on Discrete Algorithms, San Diego, CA, United States, 2019, pp.
1899–1918.
ista: 'Bernstein A, Forster S, Henzinger MH. 2019. A deamortization approach for
dynamic spanner and dynamic maximal matching. 30th Annual ACM-SIAM Symposium on
Discrete Algorithms. SODA: Symposium on Discrete Algorithms, 1899–1918.'
mla: Bernstein, Aaron, et al. “A Deamortization Approach for Dynamic Spanner and
Dynamic Maximal Matching.” 30th Annual ACM-SIAM Symposium on Discrete Algorithms,
Society for Industrial and Applied Mathematics, 2019, pp. 1899–918, doi:10.1137/1.9781611975482.115.
short: A. Bernstein, S. Forster, M.H. Henzinger, in:, 30th Annual ACM-SIAM Symposium
on Discrete Algorithms, Society for Industrial and Applied Mathematics, 2019,
pp. 1899–1918.
conference:
end_date: 2019-01-09
location: San Diego, CA, United States
name: 'SODA: Symposium on Discrete Algorithms'
start_date: 2019-01-06
date_created: 2022-08-16T09:50:33Z
date_published: 2019-01-01T00:00:00Z
date_updated: 2023-02-21T16:31:21Z
day: '01'
doi: 10.1137/1.9781611975482.115
extern: '1'
external_id:
arxiv:
- '1810.10932'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1810.10932
month: '01'
oa: 1
oa_version: Preprint
page: 1899-1918
publication: 30th Annual ACM-SIAM Symposium on Discrete Algorithms
publication_identifier:
eisbn:
- 978-1-61197-548-2
publication_status: published
publisher: Society for Industrial and Applied Mathematics
quality_controlled: '1'
related_material:
record:
- id: '11871'
relation: earlier_version
status: public
scopus_import: '1'
status: public
title: A deamortization approach for dynamic spanner and dynamic maximal matching
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...