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20162026
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 9.7k across the 90 of their papers we have counts for

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28 papers · 1 filter

astro-ph.SR2023

OGLE-BLAP-009 -- A Case Study for the Properties and Evolution of Blue Large-Amplitude Pulsators

Corey W. Bradshaw, Matti Dorsch, Thomas Kupfer +5

Blue large-amplitude pulsators (BLAPs) make up a rare class of hot pulsating stars with effective temperatures of 30,000 K and surface gravities of 4.0 - 5.0 dex (cgs). Th…

astro-ph.SR2023

Electromagnetic characterization of the LISA verification binary ZTF J05265934

Alekzander Kosakowski, Thomas Kupfer, P. Bergeron +1

We present an analysis of new and archival data to the 20.506-minute LISA verification binary J052610.42593445.32 (J05265934). Our joint spectroscopic and photometric analysi…

astro-ph.SR2023★ 15 cited

LISA Galactic binaries with astrometry from Gaia DR3

Thomas Kupfer, Valeriya Korol, Tyson B. Littenberg +11

Galactic compact binaries with orbital periods shorter than a few hours emit detectable gravitational waves at low frequencies. Their gravitational wave signals can be detected wit…

astro-ph.SR2021★ 23 cited

New Variable Hot Subdwarf Stars Identified from Anomalous Gaia Flux Errors, Observed by TESS, and Classified via Fourier Diagnostics

Brad N. Barlow, Kyle A. Corcoran, Isabelle M. Parker +7

Hot subdwarf stars are mostly stripped red giants that can exhibit photometric variations due to stellar pulsations, eclipses, the reflection effect, ellipsoidal modulation, and Do…

astro-ph.SR2021★ 38 cited

Discovery of a double detonation thermonuclear supernova progenitor

Thomas Kupfer, Evan B. Bauer, Jan van Roestel +12

We present the discovery of a new double detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with an P=76.34179(2) min orbital per…

astro-ph.SR2021★ 66 cited

A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor

Ingrid Pelisoli, P. Neunteufel, S. Geier +8

Supernova Ia are bright explosive events that can be used to estimate cosmological distances, allowing us to study the expansion of the Universe. They are understood to result from…

astro-ph.SR2021★ 36 cited

Phases of Mass Transfer from Hot Subdwarfs to White Dwarf Companions and Their Photometric Properties

Evan B. Bauer, Thomas Kupfer

Binary systems of a hot subdwarf B (sdB) star + a white dwarf (WD) with orbital periods less than 2-3 hours can come into contact due to gravitational waves and transfer mass from…

astro-ph.SR2021★ 4 cited

ZTFJ0038+2030: a long period eclipsing white dwarf and a substellar companion

Jan van Roestel, Thomas Kupfer, Keaton J. Bell +11

In a search for eclipsing white dwarfs using the Zwicky Transient Facility lightcurves, we identified a deep eclipsing white dwarf with a dark, substellar companion. The lack of an…

astro-ph.SR2021★ 28 cited

A systematic search for outbursting AM CVn systems with the Zwicky Transient Facility

Jan van Roestel, Leah Creter, Thomas Kupfer +15

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 f…

astro-ph.SR2021★ 48 cited

Year 1 of the ZTF high-cadence Galactic Plane Survey: Strategy, goals, and early results on new single-mode hot subdwarf B-star pulsators

Thomas Kupfer, Thomas A. Prince, Jan van Roestel +18

We present the goals, strategy and first results of the high-cadence Galactic plane survey using the Zwicky Transient Facility (ZTF). The goal of the survey is to unveil the Galact…

astro-ph.SR2021★ 7 cited

HO Puppis: Not a Be Star but a Newly Confirmed IW And-Type Star

Chien-De Lee, Jia-Yu Ou, Po-Chieh Yu +19

HO Puppis (HO Pup) was considered as a Be-star candidate based on its gamma-Cassiopeiae-type light curve, but lacked spectroscopic confirmation. Using distance measured from Gaia D…

astro-ph.SR2021★ 5 cited

The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor

Nadejda Blagorodnova, Jakub Klencki, Ondrej Pejcha +12

Luminous Red Novae (LRNe) are astrophysical transients associated with the partial ejection of a binary system's common envelope (CE) shortly before its merger. Here we present the…

astro-ph.SR2020

An Outburst by AM CVn binary SDSS J113732.32+405458.3

Tin Long Sunny Wong, Jan van Roestel, Thomas Kupfer +1

We report the discovery of a one magnitude increase in the optical brightness of the 59.63 minute orbital period AM CVn binary SDSS J113732.32+405458.3. Public , , and ba…

astro-ph.SR2020★ 12 cited

EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope

Jeffrey K. Ratzloff, Thomas Kupfer, Brad N. Barlow +10

We present the discovery of EVR-CB-004, a close binary with a remnant stellar core and an unseen white dwarf companion. The analysis in this work reveals the primary is potentially…

astro-ph.SR2020★ 118 cited

A systematic search of Zwicky Transient Facility data for ultracompact binary LISA-detectable gravitational-wave sources

Kevin B. Burdge, Thomas A. Prince, Jim Fuller +31

Using photometry collected with the Zwicky Transient Facility (ZTF), we are conducting an ongoing survey for binary systems with short orbital periods ( with…

astro-ph.SR2020★ 50 cited

A new class of Roche lobe-filling hot subdwarf binaries

Thomas Kupfer, Evan B. Bauer, Kevin B. Burdge +30

We present the discovery of the second binary with a Roche lobe-filling hot subdwarf transferring mass to a white dwarf (WD) companion. This 56 minute binary was discovered using d…

astro-ph.SR2020★ 3 cited

A Search for Extra-Tidal RR Lyrae in the Globular Cluster NGC 5024 and NGC 5053

Chow-Choong Ngeow, Justin Belecki, Rick Burruss +9

Recently, Kundu et al (2019) reported that the globular cluster NGC 5024 (M53) possesses five extra-tidal RR Lyrae. In fact, four of them were instead known members of a nearby glo…

astro-ph.SR2020★ 34 cited

Cataclysmic Variables in the First Year of the Zwicky Transient Facility

Paula Szkody, Brooke Dicenzo, Anna Y. Q. Ho +25

Using selection criteria based on amplitude, time and color, we have identified 329 objects as known or candidate cataclysmic variable (CVs) during the first year of testing and op…

astro-ph.SR2020★ 70 cited

The first ultracompact Roche lobe-filling hot subdwarf binary

Thomas Kupfer, Evan B. Bauer, Thomas R. Marsh +29

We report the discovery of the first short period binary in which a hot subdwarf star (sdOB) fills its Roche lobe and started mass transfer to its companion. The object was discove…

astro-ph.SR2019★ 57 cited

Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen Poor Low Mass White Dwarf

Kevin B Burdge, Jim Fuller, E. Sterl Phinney +14

We report the discovery of a detached double white dwarf binary with an orbital period of , PTF J053332.05+020911.6. The visible object in this binary, PT…

astro-ph.SR2019

EVR-CB-001: An evolving, progenitor, white dwarf compact binary discovered with the Evryscope

Jeffrey K. Ratzloff, Brad N. Barlow, Thomas Kupfer +7

We present EVR-CB-001, the discovery of a compact binary with an extremely low mass () helium core white dwarf progenitor (pre-He WD) and an unseen low mass…

astro-ph.SR2019★ 12 cited

Variability of massive stars in M31 from the Palomar Transient Factory

Monika D. Soraisam, Lars Bildsten, Maria R. Drout +5

Using data from the (intermediate) Palomar Transient Factory (iPTF), we characterize the time variability of ~500 massive stars in M31. Our sample is those stars which are spectral…

astro-ph.SR2019★ 154 cited

General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system

Kevin B. Burdge, Michael W. Coughlin, Jim Fuller +23

General relativity predicts that short orbital period binaries emit significant gravitational radiation, and the upcoming Laser Interferometer Space Antenna (LISA) is expected to d…

astro-ph.SR2018★ 52 cited

Variability of Red Supergiants in M31 from the Palomar Transient Factory

Monika D. Soraisam, Lars Bildsten, Maria R. Drout +9

Most massive stars end their lives as Red Supergiants (RSGs), a short-lived evolution phase when they are known to pulsate with varying amplitudes. The RSG period-luminosity (PL) r…