activity
20162026
most citedThe Zwicky Transient Facility: Data Processing, Products, and Archive

1.2k citations · 6.1k across the 94 of their papers we have counts for

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43 papers · 1 filter

astro-ph.SR2026

Discovery of over a thousand variable stars in Terzan 5 and Liller 1 with JWST

Kevin B. Burdge, Ilaria Caiazzo, Malina M. Desai +18

The Bulge Fossil Fragments Terzan 5 and Liller 1 host some of the densest stellar environments in the Galaxy, yet their variable star populations have remained largely unexplored d…

astro-ph.SR2026

A survey of ultra-compact high-state AM CVn binaries with ZTF and Gaia: New discoveries and observational constraints on Galactic space density

Ilkham Galiullin, Antonio C. Rodriguez, Kareem El-Badry +9

Ultra-compact AM CVn binaries in the high-state of stable mass transfer () are expected to be among the loudest persistent sources for upcomin…

astro-ph.SR2026

The Physics of Mass Transfer in Substellar and Low-Mass Binaries

Samuel Whitebook, Jim Fuller, Kevin Burdge +3

Several dozen binary ultracool and brown dwarf systems have been identified to date. These systems represent valuable probes of star and planet formation at the lowest mass scales.…

astro-ph.SR2026

Stars stably accreting from substellar objects

Aaron Householder, Kaitlyn Shin, Kevin B. Burdge +11

Substellar objects such as brown dwarfs and planets are generally expected to remain detached from their main-sequence host stars unless orbital decay or stellar expansion brings t…

astro-ph.SR2026★ 1 cited

A Mass Transferring Brown Dwarf Binary on a 57 Minute Orbit

Samuel Whitebook, Antonio C. Rodriguez, Kevin Burdge +9

Mass transfer in stellar binaries has been well studied in most stellar mass ranges, with the notable exception of ultracool stars and substellar brown dwarfs. We report the discov…

astro-ph.SR2026

JWST observations of three long-period AM CVn binaries: detection of the donors and hints of magnetically truncated disks

Kareem El-Badry, Antonio C. Rodriguez, Matthew J. Green +1

We present JWST/NIRSpec high-cadence infrared spectroscopy of three long-period, eclipsing AM CVn binaries, Gaia14aae, SRGeJ0453, and ZTFJ1637. These systems have orbital periods o…

astro-ph.SR2026

An eclipsing 8.56 minute orbital period mass-transferring binary

Emma T. Chickles, Joheen Chakraborty, Kevin B. Burdge +34

We report the discovery of ATLAS J101342.5-451656.8 (hereafter ATLAS J1013-4516), an 8.56 minute orbital period mass transferring AM Canum Venaticorum binary with mean Gaia magnitu…

astro-ph.SR2025

Circumstellar interaction in the extreme white dwarf merger remnant ZTF\,J1901+1458: A new class of white dwarf merger remnants with X-ray emission

Aayush Desai, Ilaria Caiazzo, Stephane Vennes +31

Double degenerate white dwarf (WD) mergers can exhibit extreme magnetic fields exceeding G and rapid rotation, but their spectral-energy distributions and high-energy emis…

astro-ph.SR2025★ 4 cited

A half-ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant

Andrei A. Cristea, Ilaria Caiazzo, Tim Cunningham +31

Many white dwarfs are observed in compact double white dwarf binaries and, through the emission of gravitational waves, a large fraction are destined to merge. The merger remnants…

astro-ph.SR2025

Eclipsing white dwarf from the Zwicky Transient Facility: II. Seven eclipsing double white dwarfs

J. van Roestel, K. Burdge, I. Caiazzo +15

In a systematic search for eclipsing white dwarfs using Zwicky transient facility (ZTF) data, we found seven eclipsing double white dwarfs with orbital periods ranging from 45 minu…

astro-ph.SR2025★ 1 cited

21 years of Astronomy at Warwick: celebrating the legacy of Prof. Tom Marsh

Ingrid Pelisoli, Boris Gänsicke, Keith Horne +7

Between the 4th and 6th of September 2024, the Astronomy & Astrophysics group at the University of Warwick held a meeting to celebrate 21 years of astronomy at Warwick and the scie…

astro-ph.SR2025

Double White Dwarf Tides with Multi-messenger Measurements

Nathaniel Leslie, Liang Dai, Kevin Burdge

Short-period Galactic double white dwarf (DWD) systems will be observable both in visible light through photometric monitoring and in mHz-range gravitational waves (GWs) with forth…

astro-ph.SR2025

A Link Between White Dwarf Pulsars and Polars: Multiwavelength Observations of the 9.36-Minute Period Variable Gaia22ayj

Antonio C. Rodriguez, Kareem El-Badry, Pasi Hakala +30

White dwarfs (WDs) are the most abundant compact objects, and recent surveys have suggested that over a third of WDs in accreting binaries host a strong (B 1 MG) magnetic…

astro-ph.SR2024

A gravitational wave detectable candidate Type Ia supernova progenitor

Emma T. Chickles, Kevin B. Burdge, Joheen Chakraborty +37

Type Ia supernovae, critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear. Growing evide…

astro-ph.SR2024★ 1 cited

Triple Evolution Pathways to Black Hole Low-Mass X-ray Binaries: Insights from V404 Cygni

Cheyanne Shariat, Smadar Naoz, Kareem El-Badry +5

A recent discovery shows that V404 Cygni, a prototypical black hole low-mass X-ray binary (BH-LMXB) is a hierarchical triple: the BH and donor star are orbited by a M$_{\odot…

astro-ph.SR2023★ 17 cited

A rotating white dwarf shows different compositions on its opposite faces

Ilaria Caiazzo, Kevin B. Burdge, Pier-Emmanuel Tremblay +35

White dwarfs, the extremely dense remnants left behind by most stars after their death, are characterised by a mass comparable to that of the Sun compressed into the size of an Ear…

astro-ph.SR2023★ 29 cited

The fastest stars in the Galaxy

Kareem El-Badry, Ken J. Shen, Vedant Chandra +18

We report a spectroscopic search for hypervelocity white dwarfs (WDs) that are runaways from Type Ia supernovae (SNe Ia) and related thermonuclear explosions. Candidates are select…

astro-ph.SR2023★ 27 cited

A transiting brown dwarf in a 2 hour orbit

Kareem El-Badry, Kevin B. Burdge, Jan van Roestel +1

We report the discovery of ZTF J2020+5033, a high-mass brown dwarf (BD) transiting a low-mass star with an orbital period of 1.90 hours. Phase-resolved spectroscopy, optical and in…

astro-ph.SR2023★ 17 cited

Orbital decay in an accreting and eclipsing 13.7 minute orbital period binary with a luminous donor

Kevin B. Burdge, Kareem El-Badry, Saul Rappaport +24

We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely origi…

astro-ph.SR2023★ 154 cited

A red giant orbiting a black hole

Kareem El-Badry, Hans-Walter Rix, Yvette Cendes +18

We report spectroscopic and photometric follow-up of a dormant black hole (BH) candidate from Gaia DR3. The system, which we call Gaia BH2, contains a red giant a…

astro-ph.SR2022★ 19 cited

A dense star in a 51-minute orbital period eclipsing binary

Kevin B. Burdge, Kareem El-Badry, Thomas R. Marsh +24

In over a thousand known cataclysmic variables (CVs), where a white dwarf is accreting from a hydrogen-rich star, only a dozen have orbital periods below 75 minutes. One way to ach…

astro-ph.SR2022★ 203 cited

A Sun-like star orbiting a black hole

Kareem El-Badry, Hans-Walter Rix, Eliot Quataert +18

We report discovery of a bright, nearby () Sun-like star orbiting a dark object. We identified the system as a black hole candidate via its astrometri…

astro-ph.SR2022★ 51 cited

Magnetic braking saturates: evidence from the orbital period distribution of low-mass detached eclipsing binaries from ZTF

Kareem El-Badry, Charlie Conroy, Jim Fuller +4

We constrain the orbital period () distribution of low-mass detached main-sequence eclipsing binaries (EBs) with light curves from the Zwicky Transient Facility (ZTF),…

astro-ph.SR2022★ 62 cited

Unicorns and Giraffes in the binary zoo: stripped giants with subgiant companions

Kareem El-Badry, Rhys Seeburger, Tharindu Jayasinghe +5

We analyze two binary systems containing giant stars, V723 Mon ("the Unicorn") and 2M04123153+6738486 ("the Giraffe"). Both giants orbit more massive but less luminous companions,…