---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19964'
abstract:
- lang: eng
text: It has been suggested that giant planet occurrence peaks for stars with M*
≈ 3 M⊙ at a value a factor of 4 higher than observed for solar-mass stars. This
population of giant planets predicted to frequently orbit main-sequence B stars
at a ≈ 10 au is difficult to characterize during the few hundred million years
while fusion persists in their host stars. By the time those stars become massive,
young white dwarfs, any giant planets present would still be luminous as a consequence
of their recent formation. From an initial sample of 2195 Gaia-identified massive,
young white dwarfs, we use homogeneous Spitzer Infrared Array Camera (IRAC) photometry
to search for evidence of unresolved giant planets. For 30 systems, these IRAC
data provide sensitivity to objects with M ≲ 10 MJup, and we identify one candidate
with M ≈ 4 MJup orbiting the white dwarf GALEX J071816.4+373139. Correcting for
the possibility that some of the white dwarfs in our sample result from mergers,
we find a giant planet occurrence n GP = 0.11+0.13-0.07 for stars with initial
masses M* ≳ 3 M⊙. Our occurrence inference is consistent with both the Doppler-inferred
occurrence of giant planets orbiting M* ≈ 2 M⊙ giant stars and the theoretically
predicted factor of 4 enhancement in the occurrence of giant planets orbiting
M* ≈ 3 M⊙ stars relative to solar-mass stars. Future James Webb Space Telescope
NIRCam observations of our sample would provide sensitivity to Saturn-mass planets
and thereby a definitive estimate of the occurrence of giant planets orbiting
stars with M* ≳ 3 M⊙.
acknowledgement: "We thank Jay Farihi, Guangwei Fu, J. J. Hermes, Mary Anne Limbach,
and Daniel Thorngren for useful discussions. S.C. thanks Siyu Yao for her constant
inspiration and encouragement. S.C. acknowledges the support of the Martin A. and
Helen Chooljian Member Fund, funding from the Zurich Insurance Company, and the
Fund for Natural Sciences at the Institute for Advanced Study. This work has made
use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia),
processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium).
Funding for the DPAC has been provided by national institutions, in particular the
institutions participating in the Gaia Multilateral Agreement. This work is based
in part on observations made with the Spitzer Space Telescope, which is operated
by the Jet Propulsion Laboratory, California Institute of Technology under a contract
with NASA. This publication makes use of data products from the Wide-field Infrared
Survey Explorer, which is a joint project of the University of California, Los Angeles,
and the Jet Propulsion Laboratory/California Institute of Technology, funded by
the National Aeronautics and Space Administration. 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. This research has made use of NASA’s Astrophysics
Data System.\r\nFacilities: ADS - , ESO:VISTA - European Southern Observatory's
4.1 meter Visible and Infrared Survey Telescope for Astronomy, Exoplanet Archive
- , Gaia - , IRSA - , NEOWISE - , Spitzer - Spitzer Space Telescope satellite, UKIRT
- United Kingdom Infrared Telescope, WISE - Wide-field Infrared Survey Explorer.\r\nSoftware:
astropy (Astropy Collaboration et al. 2013, 2018, 2022), numpy (C. R. Harris et
al. 2020), matplotlib (J. D. Hunter 2007), R (R Core Team 2024), SciPy (P. Virtanen
et al. 2020)."
article_number: '47'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Sihao
full_name: Cheng, Sihao
last_name: Cheng
- first_name: Kevin C.
full_name: Schlaufman, Kevin C.
last_name: Schlaufman
- first_name: Ilaria
full_name: Caiazzo, Ilaria
id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
last_name: Caiazzo
orcid: 0000-0002-4770-5388
citation:
ama: Cheng S, Schlaufman KC, Caiazzo I. A candidate giant planet companion to the
massive, young White Dwarf GALEX J071816.4+373139 informs the occurrence of giant
planets orbiting B stars. The Astronomical Journal. 2025;170(1). doi:10.3847/1538-3881/addd21
apa: Cheng, S., Schlaufman, K. C., & Caiazzo, I. (2025). A candidate giant planet
companion to the massive, young White Dwarf GALEX J071816.4+373139 informs the
occurrence of giant planets orbiting B stars. The Astronomical Journal.
IOP Publishing. https://doi.org/10.3847/1538-3881/addd21
chicago: Cheng, Sihao, Kevin C. Schlaufman, and Ilaria Caiazzo. “A Candidate Giant
Planet Companion to the Massive, Young White Dwarf GALEX J071816.4+373139 Informs
the Occurrence of Giant Planets Orbiting B Stars.” The Astronomical Journal.
IOP Publishing, 2025. https://doi.org/10.3847/1538-3881/addd21.
ieee: S. Cheng, K. C. Schlaufman, and I. Caiazzo, “A candidate giant planet companion
to the massive, young White Dwarf GALEX J071816.4+373139 informs the occurrence
of giant planets orbiting B stars,” The Astronomical Journal, vol. 170,
no. 1. IOP Publishing, 2025.
ista: Cheng S, Schlaufman KC, Caiazzo I. 2025. A candidate giant planet companion
to the massive, young White Dwarf GALEX J071816.4+373139 informs the occurrence
of giant planets orbiting B stars. The Astronomical Journal. 170(1), 47.
mla: Cheng, Sihao, et al. “A Candidate Giant Planet Companion to the Massive, Young
White Dwarf GALEX J071816.4+373139 Informs the Occurrence of Giant Planets Orbiting
B Stars.” The Astronomical Journal, vol. 170, no. 1, 47, IOP Publishing,
2025, doi:10.3847/1538-3881/addd21.
short: S. Cheng, K.C. Schlaufman, I. Caiazzo, The Astronomical Journal 170 (2025).
date_created: 2025-07-06T22:01:22Z
date_published: 2025-07-01T00:00:00Z
date_updated: 2026-02-19T09:31:41Z
day: '01'
ddc:
- '520'
department:
- _id: IlCa
doi: 10.3847/1538-3881/addd21
external_id:
arxiv:
- '2408.03985'
isi:
- '001514518100001'
file:
- access_level: open_access
checksum: 144b0e46aa3dff0cdf8c6ee7d4fe2fe4
content_type: application/pdf
creator: dernst
date_created: 2025-07-08T06:40:54Z
date_updated: 2025-07-08T06:40:54Z
file_id: '19975'
file_name: 2025_AstronomicalJour_Cheng.pdf
file_size: 931173
relation: main_file
success: 1
file_date_updated: 2025-07-08T06:40:54Z
fulldoi: https://doi.org/10.3847/1538-3881/addd21
has_accepted_license: '1'
intvolume: ' 170'
isi: 1
issue: '1'
language:
- iso: eng
month: '07'
oa: 1
oa_version: Published Version
publication: The Astronomical Journal
publication_identifier:
eissn:
- 1538-3881
issn:
- 0004-6256
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: A candidate giant planet companion to the massive, young White Dwarf GALEX
J071816.4+373139 informs the occurrence of giant planets orbiting B stars
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: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 170
year: '2025'
...
---
_id: '11604'
abstract:
- lang: eng
text: The NASA Transiting Exoplanet Survey Satellite (TESS) is observing tens of
millions of stars with time spans ranging from ∼27 days to about 1 yr of continuous
observations. This vast amount of data contains a wealth of information for variability,
exoplanet, and stellar astrophysics studies but requires a number of processing
steps before it can be fully utilized. In order to efficiently process all the
TESS data and make it available to the wider scientific community, the TESS Data
for Asteroseismology working group, as part of the TESS Asteroseismic Science
Consortium, has created an automated open-source processing pipeline to produce
light curves corrected for systematics from the short- and long-cadence raw photometry
data and to classify these according to stellar variability type. We will process
all stars down to a TESS magnitude of 15. This paper is the next in a series detailing
how the pipeline works. Here, we present our methodology for the automatic variability
classification of TESS photometry using an ensemble of supervised learners that
are combined into a metaclassifier. We successfully validate our method using
a carefully constructed labeled sample of Kepler Q9 light curves with a 27.4 days
time span mimicking single-sector TESS observations, on which we obtain an overall
accuracy of 94.9%. We demonstrate that our methodology can successfully classify
stars outside of our labeled sample by applying it to all ∼167,000 stars observed
in Q9 of the Kepler space mission.
acknowledgement: "The research leading to these results has received funding from
the European Research Council (ERC) under the European Union's Horizon 2020 research
and innovation program (grant agreement No. 670519: MAMSIE), from the KU Leuven
Research Council (grant C16/18/005: PARADISE), from the Research Foundation Flanders
(FWO) under grant agreement G0H5416N (ERC Runner Up Project), as well as from the
BELgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO. D.J.A
acknowledges support from the STFC via an Ernest Rutherford Fellowship (ST/R00384X/1).
Funding for the Stellar Astrophysics Centre is provided by The Danish National Research
Foundation (grant agreement No.: DNRF106). R.H. and M.N.L. acknowledge the ESA PRODEX
program. This research was supported by the National Aeronautics and Space Administration
(80NSSC18K1585 and 80NSSC19K0379) awarded through the TESS Guest Investigator Program.
K.J.B. is supported by the National Science Foundation under Award AST-1903828.
J.S.K and K.J.B. were supported by funding from the European Research Council under
the European Community's Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement
no. 338251 (StellarAges). D.M.B. gratefully acknowledges funding from a senior postdoctoral
fellowship from the Research Foundation Flanders (FWO) with grant agreement No.
1286521N. The research leading to these results has received funding from the Research
Foundation Flanders (FWO) under grant agreement G0A2917N (BlackGEM). R.A.G. acknowledges
support from the GOLF and PLATO CNES grants. L.M. was supported by the Premium Postdoctoral
Research Program of the Hungarian Academy of Sciences. The research leading to these
results has been supported by the Hungarian National Research, Development, and
Innovation Office (NKFIH) grant KH_18 130405 and the Lendület LP2014-17 and LP2018-7/2020
grants of the Hungarian Academy of Sciences. D.B. acknowledges support from the
NASA TESS Guest Investigator Program under award 80NSSC19K0385.\r\n\r\nThis paper
includes data collected by the TESS mission, which are publicly available from the
Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission is provided
by NASA's Science Mission directorate. This research has made use of NASA's Astrophysics
Data System as well as the NASA/IPAC Extragalactic Database (NED) which is operated
by the Jet Propulsion Laboratory, California Institute of Technology, under contract
with the National Aeronautics and Space Administration. Funding for the TESS Asteroseismic
Science Operations Centre is provided by the Danish National Research Foundation
(Grant agreement no.: DNRF106), ESA PRODEX (PEA 4000119301), and the Stellar Astrophysics
Centre (SAC) at Aarhus University. We thank the TESS team and staff and TASC/TASOC
for their support of the present work.\r\n\r\nThis paper includes data collected
by the Kepler mission. Funding for the Kepler and K2 mission was provided by NASA's
Science Mission Directorate. The authors acknowledge the efforts of the Kepler Mission
team in obtaining the light-curve data and data validation products used in this
publication. These data were generated by the Kepler Mission science pipeline through
the efforts of the Kepler Science Operations Center and Science Office. The Kepler
light curves are archived at the Mikulski Archive for Space Telescopes.\r\n\r\nThe
numerical results presented in this work were obtained at the Centre for Scientific
Computing, Aarhus. 37 This research made use of Astropy, a community-developed core
Python package for Astronomy (Astropy Collaboration et al. 2013, 2018).\r\n\r\nSoftware:
Scikit-learn (Pedregosa et al. 2011), Numpy (Harris et al. 2020), Astropy (Astropy
Collaboration et al. 2013, 2018), Scipy (Virtanen et al. 2020), Pandas (McKinney
2010; Pandas Development Team 2020), Lightkurve (Lightkurve Collaboration et al.
2018), XGBoost (Chen & Guestrin 2016), Tensorflow (Abadi et al. 2015)."
article_number: '209'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: J.
full_name: Audenaert, J.
last_name: Audenaert
- first_name: J. S.
full_name: Kuszlewicz, J. S.
last_name: Kuszlewicz
- first_name: R.
full_name: Handberg, R.
last_name: Handberg
- first_name: A.
full_name: Tkachenko, A.
last_name: Tkachenko
- first_name: D. J.
full_name: Armstrong, D. J.
last_name: Armstrong
- first_name: M.
full_name: Hon, M.
last_name: Hon
- first_name: R.
full_name: Kgoadi, R.
last_name: Kgoadi
- first_name: M. N.
full_name: Lund, M. N.
last_name: Lund
- first_name: K. J.
full_name: Bell, K. J.
last_name: Bell
- 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: D. M.
full_name: Bowman, D. M.
last_name: Bowman
- first_name: C.
full_name: Johnston, C.
last_name: Johnston
- first_name: R. A.
full_name: García, R. A.
last_name: García
- first_name: D.
full_name: Stello, D.
last_name: Stello
- first_name: L.
full_name: Molnár, L.
last_name: Molnár
- first_name: E.
full_name: Plachy, E.
last_name: Plachy
- first_name: D.
full_name: Buzasi, D.
last_name: Buzasi
- first_name: C.
full_name: Aerts, C.
last_name: Aerts
citation:
ama: 'Audenaert J, Kuszlewicz JS, Handberg R, et al. TESS Data for Asteroseismology
(T’DA) stellar variability classification pipeline: Setup and application to the
Kepler Q9 data. The Astronomical Journal. 2021;162(5). doi:10.3847/1538-3881/ac166a'
apa: 'Audenaert, J., Kuszlewicz, J. S., Handberg, R., Tkachenko, A., Armstrong,
D. J., Hon, M., … Aerts, C. (2021). TESS Data for Asteroseismology (T’DA) stellar
variability classification pipeline: Setup and application to the Kepler Q9 data.
The Astronomical Journal. IOP Publishing. https://doi.org/10.3847/1538-3881/ac166a'
chicago: 'Audenaert, J., J. S. Kuszlewicz, R. Handberg, A. Tkachenko, D. J. Armstrong,
M. Hon, R. Kgoadi, et al. “TESS Data for Asteroseismology (T’DA) Stellar Variability
Classification Pipeline: Setup and Application to the Kepler Q9 Data.” The
Astronomical Journal. IOP Publishing, 2021. https://doi.org/10.3847/1538-3881/ac166a.'
ieee: 'J. Audenaert et al., “TESS Data for Asteroseismology (T’DA) stellar
variability classification pipeline: Setup and application to the Kepler Q9 data,”
The Astronomical Journal, vol. 162, no. 5. IOP Publishing, 2021.'
ista: 'Audenaert J, Kuszlewicz JS, Handberg R, Tkachenko A, Armstrong DJ, Hon M,
Kgoadi R, Lund MN, Bell KJ, Bugnet LA, Bowman DM, Johnston C, García RA, Stello
D, Molnár L, Plachy E, Buzasi D, Aerts C. 2021. TESS Data for Asteroseismology
(T’DA) stellar variability classification pipeline: Setup and application to the
Kepler Q9 data. The Astronomical Journal. 162(5), 209.'
mla: 'Audenaert, J., et al. “TESS Data for Asteroseismology (T’DA) Stellar Variability
Classification Pipeline: Setup and Application to the Kepler Q9 Data.” The
Astronomical Journal, vol. 162, no. 5, 209, IOP Publishing, 2021, doi:10.3847/1538-3881/ac166a.'
short: J. Audenaert, J.S. Kuszlewicz, R. Handberg, A. Tkachenko, D.J. Armstrong,
M. Hon, R. Kgoadi, M.N. Lund, K.J. Bell, L.A. Bugnet, D.M. Bowman, C. Johnston,
R.A. García, D. Stello, L. Molnár, E. Plachy, D. Buzasi, C. Aerts, The Astronomical
Journal 162 (2021).
date_created: 2022-07-18T11:54:55Z
date_published: 2021-10-21T00:00:00Z
date_updated: 2022-08-19T10:01:56Z
day: '21'
doi: 10.3847/1538-3881/ac166a
extern: '1'
external_id:
arxiv:
- '2107.06301'
fulldoi: https://doi.org/10.3847/1538-3881/ac166a
intvolume: ' 162'
issue: '5'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2107.06301
month: '10'
oa: 1
oa_version: Preprint
publication: The Astronomical Journal
publication_identifier:
eissn:
- 1538-3881
issn:
- 0004-6256
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'TESS Data for Asteroseismology (T’DA) stellar variability classification pipeline:
Setup and application to the Kepler Q9 data'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 162
year: '2021'
...
---
_id: '13459'
abstract:
- lang: eng
text: The B emission-line stars are rapid rotators that were probably spun up by
mass and angular momentum accretion through mass transfer in an interacting binary.
Mass transfer will strip the donor star of its envelope to create a small and
hot subdwarf remnant. Here we report on Hubble Space Telescope/STIS far-ultraviolet
spectroscopy of a sample of Be stars that reveals the presence of the hot sdO
companion through the calculation of cross-correlation functions of the observed
and model spectra. We clearly detect the spectral signature of the sdO star in
10 of the 13 stars in the sample, and the spectral signals indicate that the sdO
stars are hot, relatively faint, and slowly rotating as predicted by models. A
comparison of their temperatures and radii with evolutionary tracks indicates
that the sdO stars occupy the relatively long-lived, He-core burning stage. Only
1 of the 10 detections was a known binary prior to this investigation, which emphasizes
the difficulty of finding such Be+sdO binaries through optical spectroscopy. However,
these results and others indicate that many Be stars probably host hot subdwarf
companions.
article_number: '248'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Luqian
full_name: Wang, Luqian
last_name: Wang
- first_name: Douglas R.
full_name: Gies, Douglas R.
last_name: Gies
- first_name: Geraldine J.
full_name: Peters, Geraldine J.
last_name: Peters
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
- first_name: S. Drew
full_name: Chojnowski, S. Drew
last_name: Chojnowski
- first_name: Kathryn V.
full_name: Lester, Kathryn V.
last_name: Lester
- first_name: Steve B.
full_name: Howell, Steve B.
last_name: Howell
citation:
ama: Wang L, Gies DR, Peters GJ, et al. The detection and characterization of Be+sdO
binaries from HST/STIS FUV spectroscopy. The Astronomical Journal. 2021;161(5).
doi:10.3847/1538-3881/abf144
apa: Wang, L., Gies, D. R., Peters, G. J., Götberg, Y. L. L., Chojnowski, S. D.,
Lester, K. V., & Howell, S. B. (2021). The detection and characterization
of Be+sdO binaries from HST/STIS FUV spectroscopy. The Astronomical Journal.
American Astronomical Society. https://doi.org/10.3847/1538-3881/abf144
chicago: Wang, Luqian, Douglas R. Gies, Geraldine J. Peters, Ylva Louise Linsdotter
Götberg, S. Drew Chojnowski, Kathryn V. Lester, and Steve B. Howell. “The Detection
and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” The
Astronomical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-3881/abf144.
ieee: L. Wang et al., “The detection and characterization of Be+sdO binaries
from HST/STIS FUV spectroscopy,” The Astronomical Journal, vol. 161, no.
5. American Astronomical Society, 2021.
ista: Wang L, Gies DR, Peters GJ, Götberg YLL, Chojnowski SD, Lester KV, Howell
SB. 2021. The detection and characterization of Be+sdO binaries from HST/STIS
FUV spectroscopy. The Astronomical Journal. 161(5), 248.
mla: Wang, Luqian, et al. “The Detection and Characterization of Be+sdO Binaries
from HST/STIS FUV Spectroscopy.” The Astronomical Journal, vol. 161, no.
5, 248, American Astronomical Society, 2021, doi:10.3847/1538-3881/abf144.
short: L. Wang, D.R. Gies, G.J. Peters, Y.L.L. Götberg, S.D. Chojnowski, K.V. Lester,
S.B. Howell, The Astronomical Journal 161 (2021).
date_created: 2023-08-03T10:11:57Z
date_published: 2021-05-04T00:00:00Z
date_updated: 2023-08-21T11:35:50Z
day: '04'
doi: 10.3847/1538-3881/abf144
extern: '1'
external_id:
arxiv:
- '2103.13642'
fulldoi: https://doi.org/10.3847/1538-3881/abf144
intvolume: ' 161'
issue: '5'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2103.13642
month: '05'
oa: 1
oa_version: Preprint
publication: The Astronomical Journal
publication_identifier:
eissn:
- 1538-3881
issn:
- 0004-6256
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 161
year: '2021'
...
---
_id: '15216'
abstract:
- lang: eng
text: AM CVn systems are a rare type of accreting binary that consists of a white
dwarf and a helium-rich, degenerate donor star. Using the Zwicky Transient Facility
(ZTF), we searched for new AM CVn systems by focusing on blue, outbursting stars.
We first selected outbursting stars using the ZTF alerts. We cross matched the
candidates with Gaia and Pan-STARRS catalogs. The initial selection of candidates
based on the Gaia BP-RP contains 1751 unknown objects. We used the Pan-STARRS
g-r and r-i color in combination with the Gaia color to identify 59 strong AM
CVn candidates. We obtained identification spectra of 35 sources, of which 18
are high-priority candidates, and discovered nine new AM CVn systems and one magnetic
CV that shows only He-ii lines. Using the outburst recurrence time, we estimate
the orbital periods of the nine new AM CVn systems that are in the range of 29–50
minutes. We conclude that targeted follow up of blue, outbursting sources is an
efficient method to find new AM CVn systems and we plan to follow up all candidates
we identified to systematically study the population of outbursting AM CVn systems.
article_number: '113'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jan
full_name: van Roestel, Jan
last_name: van Roestel
- first_name: Leah
full_name: Creter, Leah
last_name: Creter
- first_name: Thomas
full_name: Kupfer, Thomas
last_name: Kupfer
- first_name: Paula
full_name: Szkody, Paula
last_name: Szkody
- first_name: Jim
full_name: Fuller, Jim
last_name: Fuller
- first_name: Matthew J.
full_name: Green, Matthew J.
last_name: Green
- first_name: R. Michael
full_name: Rich, R. Michael
last_name: Rich
- first_name: John
full_name: Sepikas, John
last_name: Sepikas
- first_name: Kevin
full_name: Burdge, Kevin
last_name: Burdge
- first_name: Ilaria
full_name: Caiazzo, Ilaria
id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
last_name: Caiazzo
orcid: 0000-0002-4770-5388
- first_name: Przemek
full_name: Mróz, Przemek
last_name: Mróz
- first_name: Thomas A.
full_name: Prince, Thomas A.
last_name: Prince
- first_name: Dmitry A.
full_name: Duev, Dmitry A.
last_name: Duev
- first_name: Matthew J.
full_name: Graham, Matthew J.
last_name: Graham
- first_name: David L.
full_name: Shupe, David L.
last_name: Shupe
- first_name: Russ R.
full_name: Laher, Russ R.
last_name: Laher
- first_name: Ashish A.
full_name: Mahabal, Ashish A.
last_name: Mahabal
- first_name: Frank J.
full_name: Masci, Frank J.
last_name: Masci
citation:
ama: van Roestel J, Creter L, Kupfer T, et al. A systematic search for outbursting
AM CVn systems with the Zwicky transient facility. The Astronomical Journal.
2021;162(3). doi:10.3847/1538-3881/ac0622
apa: van Roestel, J., Creter, L., Kupfer, T., Szkody, P., Fuller, J., Green, M.
J., … Masci, F. J. (2021). A systematic search for outbursting AM CVn systems
with the Zwicky transient facility. The Astronomical Journal. American
Astronomical Society. https://doi.org/10.3847/1538-3881/ac0622
chicago: Roestel, Jan van, Leah Creter, Thomas Kupfer, Paula Szkody, Jim Fuller,
Matthew J. Green, R. Michael Rich, et al. “A Systematic Search for Outbursting
AM CVn Systems with the Zwicky Transient Facility.” The Astronomical Journal.
American Astronomical Society, 2021. https://doi.org/10.3847/1538-3881/ac0622.
ieee: J. van Roestel et al., “A systematic search for outbursting AM CVn
systems with the Zwicky transient facility,” The Astronomical Journal,
vol. 162, no. 3. American Astronomical Society, 2021.
ista: van Roestel J, Creter L, Kupfer T, Szkody P, Fuller J, Green MJ, Rich RM,
Sepikas J, Burdge K, Caiazzo I, Mróz P, Prince TA, Duev DA, Graham MJ, Shupe DL,
Laher RR, Mahabal AA, Masci FJ. 2021. A systematic search for outbursting AM CVn
systems with the Zwicky transient facility. The Astronomical Journal. 162(3),
113.
mla: van Roestel, Jan, et al. “A Systematic Search for Outbursting AM CVn Systems
with the Zwicky Transient Facility.” The Astronomical Journal, vol. 162,
no. 3, 113, American Astronomical Society, 2021, doi:10.3847/1538-3881/ac0622.
short: J. van Roestel, L. Creter, T. Kupfer, P. Szkody, J. Fuller, M.J. Green, R.M.
Rich, J. Sepikas, K. Burdge, I. Caiazzo, P. Mróz, T.A. Prince, D.A. Duev, M.J.
Graham, D.L. Shupe, R.R. Laher, A.A. Mahabal, F.J. Masci, The Astronomical Journal
162 (2021).
date_created: 2024-03-26T10:32:25Z
date_published: 2021-08-19T00:00:00Z
date_updated: 2024-04-02T07:28:50Z
day: '19'
doi: 10.3847/1538-3881/ac0622
extern: '1'
external_id:
arxiv:
- '2105.02261'
fulldoi: https://doi.org/10.3847/1538-3881/ac0622
intvolume: ' 162'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2105.02261
month: '08'
oa: 1
oa_version: Preprint
publication: The Astronomical Journal
publication_identifier:
eissn:
- 1538-3881
issn:
- 0004-6256
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: A systematic search for outbursting AM CVn systems with the Zwicky transient
facility
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 162
year: '2021'
...
---
OA_type: free access
_id: '17799'
abstract:
- lang: eng
text: The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey
that will eventually cover approximately one-quarter of the celestial sphere and
collect spectra of ≈106 galaxies, 100,000 quasars, 30,000 stars, and 30,000 serendipity
targets. In 2001 June, the SDSS released to the general astronomical community
its early data release, roughly 462 deg2 of imaging data including almost 14 million
detected objects and 54,008 follow-up spectra. The imaging data were collected
in drift-scan mode in five bandpasses (u, g, r, i, and z); our 95% completeness
limits for stars are 22.0, 22.2, 22.2, 21.3, and 20.5, respectively. The photometric
calibration is reproducible to 5%, 3%, 3%, 3%, and 5%, respectively. The spectra
are flux- and wavelength-calibrated, with 4096 pixels from 3800 to 9200 Å at R
≈ 1800. We present the means by which these data are distributed to the astronomical
community, descriptions of the hardware used to obtain the data, the software
used for processing the data, the measured quantities for each observed object,
and an overview of the properties of this data set.
article_processing_charge: No
article_type: original
author:
- first_name: Chris
full_name: Stoughton, Chris
last_name: Stoughton
- first_name: Robert H.
full_name: Lupton, Robert H.
last_name: Lupton
- first_name: Mariangela
full_name: Bernardi, Mariangela
last_name: Bernardi
- first_name: Michael R.
full_name: Blanton, Michael R.
last_name: Blanton
- first_name: Scott
full_name: Burles, Scott
last_name: Burles
- first_name: Francisco J.
full_name: Castander, Francisco J.
last_name: Castander
- first_name: A. J.
full_name: Connolly, A. J.
last_name: Connolly
- first_name: Daniel J.
full_name: Eisenstein, Daniel J.
last_name: Eisenstein
- first_name: Joshua A.
full_name: Frieman, Joshua A.
last_name: Frieman
- first_name: G. S.
full_name: Hennessy, G. S.
last_name: Hennessy
- first_name: Robert B.
full_name: Hindsley, Robert B.
last_name: Hindsley
- first_name: Željko
full_name: Ivezić, Željko
last_name: Ivezić
- first_name: Stephen
full_name: Kent, Stephen
last_name: Kent
- first_name: Peter Z.
full_name: Kunszt, Peter Z.
last_name: Kunszt
- first_name: Brian C.
full_name: Lee, Brian C.
last_name: Lee
- first_name: Avery
full_name: Meiksin, Avery
last_name: Meiksin
- first_name: Jeffrey A.
full_name: Munn, Jeffrey A.
last_name: Munn
- first_name: Heidi Jo
full_name: Newberg, Heidi Jo
last_name: Newberg
- first_name: R. C.
full_name: Nichol, R. C.
last_name: Nichol
- first_name: Tom
full_name: Nicinski, Tom
last_name: Nicinski
- first_name: Jeffrey R.
full_name: Pier, Jeffrey R.
last_name: Pier
- first_name: Gordon T.
full_name: Richards, Gordon T.
last_name: Richards
- first_name: Michael W.
full_name: Richmond, Michael W.
last_name: Richmond
- first_name: David J.
full_name: Schlegel, David J.
last_name: Schlegel
- first_name: J. Allyn
full_name: Smith, J. Allyn
last_name: Smith
- first_name: Michael A.
full_name: Strauss, Michael A.
last_name: Strauss
- first_name: Mark
full_name: SubbaRao, Mark
last_name: SubbaRao
- first_name: Alexander S.
full_name: Szalay, Alexander S.
last_name: Szalay
- first_name: Aniruddha R.
full_name: Thakar, Aniruddha R.
last_name: Thakar
- first_name: Douglas L.
full_name: Tucker, Douglas L.
last_name: Tucker
- first_name: Daniel E.
full_name: Vanden Berk, Daniel E.
last_name: Vanden Berk
- first_name: Brian
full_name: Yanny, Brian
last_name: Yanny
- first_name: Jennifer K.
full_name: Adelman, Jennifer K.
last_name: Adelman
- first_name: John E.
full_name: Anderson, Jr., John E.
last_name: Anderson, Jr.
- first_name: Scott F.
full_name: Anderson, Scott F.
last_name: Anderson
- first_name: James
full_name: Annis, James
last_name: Annis
- first_name: Neta A.
full_name: Bahcall, Neta A.
last_name: Bahcall
- first_name: J. A.
full_name: Bakken, J. A.
last_name: Bakken
- first_name: Matthias
full_name: Bartelmann, Matthias
last_name: Bartelmann
- first_name: Steven
full_name: Bastian, Steven
last_name: Bastian
- first_name: Amanda
full_name: Bauer, Amanda
last_name: Bauer
- first_name: Eileen
full_name: Berman, Eileen
last_name: Berman
- first_name: Hans
full_name: Böhringer, Hans
last_name: Böhringer
- first_name: William N.
full_name: Boroski, William N.
last_name: Boroski
- first_name: Steve
full_name: Bracker, Steve
last_name: Bracker
- first_name: Charlie
full_name: Briegel, Charlie
last_name: Briegel
- first_name: John W.
full_name: Briggs, John W.
last_name: Briggs
- first_name: J.
full_name: Brinkmann, J.
last_name: Brinkmann
- first_name: Robert
full_name: Brunner, Robert
last_name: Brunner
- first_name: Larry
full_name: Carey, Larry
last_name: Carey
- first_name: Michael A.
full_name: Carr, Michael A.
last_name: Carr
- first_name: Bing
full_name: Chen, Bing
last_name: Chen
- first_name: Damian
full_name: Christian, Damian
last_name: Christian
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full_name: Colestock, Patrick L.
last_name: Colestock
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full_name: Crocker, J. H.
last_name: Crocker
- first_name: István
full_name: Csabai, István
last_name: Csabai
- first_name: Paul C.
full_name: Czarapata, Paul C.
last_name: Czarapata
- first_name: Julianne
full_name: Dalcanton, Julianne
last_name: Dalcanton
- first_name: Arthur F.
full_name: Davidsen, Arthur F.
last_name: Davidsen
- first_name: John Eric
full_name: Davis, John Eric
last_name: Davis
- first_name: Walter
full_name: Dehnen, Walter
last_name: Dehnen
- first_name: Scott
full_name: Dodelson, Scott
last_name: Dodelson
- first_name: Mamoru
full_name: Doi, Mamoru
last_name: Doi
- first_name: Tom
full_name: Dombeck, Tom
last_name: Dombeck
- first_name: Megan
full_name: Donahue, Megan
last_name: Donahue
- first_name: Nancy
full_name: Ellman, Nancy
last_name: Ellman
- first_name: Brian R.
full_name: Elms, Brian R.
last_name: Elms
- first_name: Michael L.
full_name: Evans, Michael L.
last_name: Evans
- first_name: Laurent
full_name: Eyer, Laurent
last_name: Eyer
- first_name: Xiaohui
full_name: Fan, Xiaohui
last_name: Fan
- first_name: Glenn R.
full_name: Federwitz, Glenn R.
last_name: Federwitz
- first_name: Scott
full_name: Friedman, Scott
last_name: Friedman
- first_name: Masataka
full_name: Fukugita, Masataka
last_name: Fukugita
- first_name: Roy
full_name: Gal, Roy
last_name: Gal
- first_name: Bruce
full_name: Gillespie, Bruce
last_name: Gillespie
- first_name: Karl
full_name: Glazebrook, Karl
last_name: Glazebrook
- first_name: Jim
full_name: Gray, Jim
last_name: Gray
- first_name: Eva K.
full_name: Grebel, Eva K.
last_name: Grebel
- first_name: Bruce
full_name: Greenawalt, Bruce
last_name: Greenawalt
- first_name: Gretchen
full_name: Greene, Gretchen
last_name: Greene
- first_name: James E.
full_name: Gunn, James E.
last_name: Gunn
- first_name: Ernst
full_name: de Haas, Ernst
last_name: de Haas
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
orcid: 0000-0003-3633-5403
- first_name: Merle
full_name: Haldeman, Merle
last_name: Haldeman
- first_name: Patrick B.
full_name: Hall, Patrick B.
last_name: Hall
- first_name: Masaru
full_name: Hamabe, Masaru
last_name: Hamabe
- first_name: Brad
full_name: Hansen, Brad
last_name: Hansen
- first_name: Frederick H.
full_name: Harris, Frederick H.
last_name: Harris
- first_name: Hugh
full_name: Harris, Hugh
last_name: Harris
- first_name: Michael
full_name: Harvanek, Michael
last_name: Harvanek
- first_name: Suzanne L.
full_name: Hawley, Suzanne L.
last_name: Hawley
- first_name: J. J. E.
full_name: Hayes, J. J. E.
last_name: Hayes
- first_name: Timothy M.
full_name: Heckman, Timothy M.
last_name: Heckman
- first_name: Amina
full_name: Helmi, Amina
last_name: Helmi
- first_name: Arne
full_name: Henden, Arne
last_name: Henden
- first_name: Craig J.
full_name: Hogan, Craig J.
last_name: Hogan
- first_name: David W.
full_name: Hogg, David W.
last_name: Hogg
- first_name: Donald J.
full_name: Holmgren, Donald J.
last_name: Holmgren
- first_name: Jon
full_name: Holtzman, Jon
last_name: Holtzman
- first_name: Chih-Hao
full_name: Huang, Chih-Hao
last_name: Huang
- first_name: Charles
full_name: Hull, Charles
last_name: Hull
- first_name: Shin-Ichi
full_name: Ichikawa, Shin-Ichi
last_name: Ichikawa
- first_name: Takashi
full_name: Ichikawa, Takashi
last_name: Ichikawa
- first_name: David E.
full_name: Johnston, David E.
last_name: Johnston
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full_name: Kauffmann, Guinevere
last_name: Kauffmann
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full_name: Kim, Rita S. J.
last_name: Kim
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full_name: Kimball, Tim
last_name: Kimball
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full_name: Kinney, E.
last_name: Kinney
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full_name: Klaene, Mark
last_name: Klaene
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full_name: Kleinman, S. J.
last_name: Kleinman
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full_name: Klypin, Anatoly
last_name: Klypin
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full_name: Knapp, G. R.
last_name: Knapp
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full_name: Korienek, John
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last_name: Krolik
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full_name: Kron, Richard G.
last_name: Kron
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full_name: Krzesiński, Jurek
last_name: Krzesiński
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full_name: Lamb, D. Q.
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full_name: Leger, R. French
last_name: Leger
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full_name: Lindenmeyer, Carl
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last_name: Neilsen, Jr.
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last_name: Odenkirchen
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citation:
ama: 'Stoughton C, Lupton RH, Bernardi M, et al. Sloan digital sky survey: Early
data release. The Astronomical Journal. 2002;123(1):485-548. doi:10.1086/324741'
apa: 'Stoughton, C., Lupton, R. H., Bernardi, M., Blanton, M. R., Burles, S., Castander,
F. J., … Zheng, W. (2002). Sloan digital sky survey: Early data release. The
Astronomical Journal. American Astronomical Society. https://doi.org/10.1086/324741'
chicago: 'Stoughton, Chris, Robert H. Lupton, Mariangela Bernardi, Michael R. Blanton,
Scott Burles, Francisco J. Castander, A. J. Connolly, et al. “Sloan Digital Sky
Survey: Early Data Release.” The Astronomical Journal. American Astronomical
Society, 2002. https://doi.org/10.1086/324741.'
ieee: 'C. Stoughton et al., “Sloan digital sky survey: Early data release,”
The Astronomical Journal, vol. 123, no. 1. American Astronomical Society,
pp. 485–548, 2002.'
ista: 'Stoughton C et al. 2002. Sloan digital sky survey: Early data release. The
Astronomical Journal. 123(1), 485–548.'
mla: 'Stoughton, Chris, et al. “Sloan Digital Sky Survey: Early Data Release.” The
Astronomical Journal, vol. 123, no. 1, American Astronomical Society, 2002,
pp. 485–548, doi:10.1086/324741.'
short: C. Stoughton, R.H. Lupton, M. Bernardi, M.R. Blanton, S. Burles, F.J. Castander,
A.J. Connolly, D.J. Eisenstein, J.A. Frieman, G.S. Hennessy, R.B. Hindsley, Ž.
Ivezić, S. Kent, P.Z. Kunszt, B.C. Lee, A. Meiksin, J.A. Munn, H.J. Newberg, R.C.
Nichol, T. Nicinski, J.R. Pier, G.T. Richards, M.W. Richmond, D.J. Schlegel, J.A.
Smith, M.A. Strauss, M. SubbaRao, A.S. Szalay, A.R. Thakar, D.L. Tucker, D.E.
Vanden Berk, B. Yanny, J.K. Adelman, J.E. Anderson, Jr., S.F. Anderson, J. Annis,
N.A. Bahcall, J.A. Bakken, M. Bartelmann, S. Bastian, A. Bauer, E. Berman, H.
Böhringer, W.N. Boroski, S. Bracker, C. Briegel, J.W. Briggs, J. Brinkmann, R.
Brunner, L. Carey, M.A. Carr, B. Chen, D. Christian, P.L. Colestock, J.H. Crocker,
I. Csabai, P.C. Czarapata, J. Dalcanton, A.F. Davidsen, J.E. Davis, W. Dehnen,
S. Dodelson, M. Doi, T. Dombeck, M. Donahue, N. Ellman, B.R. Elms, M.L. Evans,
L. Eyer, X. Fan, G.R. Federwitz, S. Friedman, M. Fukugita, R. Gal, B. Gillespie,
K. Glazebrook, J. Gray, E.K. Grebel, B. Greenawalt, G. Greene, J.E. Gunn, E. de
Haas, Z. Haiman, M. Haldeman, P.B. Hall, M. Hamabe, B. Hansen, F.H. Harris, H.
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W. Zheng, The Astronomical Journal 123 (2002) 485–548.
date_created: 2024-09-06T10:32:06Z
date_published: 2002-01-01T00:00:00Z
date_updated: 2024-11-12T09:51:31Z
day: '01'
doi: 10.1086/324741
extern: '1'
fulldoi: https://doi.org/10.1086/324741
intvolume: ' 123'
issue: '1'
language:
- iso: eng
month: '01'
oa_version: None
page: 485-548
publication: The Astronomical Journal
publication_identifier:
eissn:
- 1538-3881
issn:
- 0004-6256
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
related_material:
link:
- relation: erratum
url: https://doi.org/10.1086/340314
scopus_import: '1'
status: public
title: 'Sloan digital sky survey: Early data release'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 123
year: '2002'
...