activity
20202026
most citedTESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26

205 citations · 438 across the 19 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2026

Quasi-periodic eruption spectral-timing: EMRIs crossing warped accretion disks

Joheen Chakraborty, Andrew Mummery, Eliot Quataert +3

Quasi-periodic eruptions (QPEs) are repeating X-ray transients from galactic nuclei potentially caused by a stellar-mass orbiter repeatedly colliding with the accretion disk of a s…

astro-ph.HE2026

Relativistic outflows power a quasi-periodic eruption: constraints on energetics, mass loss, and emission mechanisms

Joheen Chakraborty, Erin Kara, Wenbin Lu +17

Quasi-periodic eruptions (QPEs) are recurring bursts of X-ray radiation originating from supermassive black holes (SMBHs). They are an unprecedented type of structured, high-amplit…

astro-ph.HE2026

Observations of X-ray quasi-periodic eruptions

Thomas Wevers, Joheen Chakraborty, Erwan Quintin +2

Quasi-periodic eruptions (QPEs) are a novel class of repeating nuclear transients, discovered exclusively in the X-ray band to date. Since their initial discovery in 2019, the QPE…

astro-ph.HE2026

Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5704014

Rahul Sharma, Chandreyee Maitra, Frank Haberl +9

We present timing and spectral analysis of the recently identified ultracompact double-degenerate (DD) white dwarf binary eRASSU J060839.5704014 using observations from NICER an…

astro-ph.SR2026

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories

James Munday, Antonio C. Rodriguez, Nicole Reindl +23

The AM CVn class includes mass transferring, ultra-compact double white dwarf binaries with orbital periods on the timescale of minutes. A long-standing puzzle is that none of the…

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.HE2026

A positive period derivative in the quasi-periodic eruptions of ZTF19acnskyy

Joheen Chakraborty, Saul A. Rappaport, Riccardo Arcodia +9

We report the first direct measurement of the period derivative in a quasi-periodic eruption (QPE), finding a smoothly increasing period with $\dot{P}\approx (1.7\pm 0.02)\times10^…

astro-ph.HE2026

X-ray Spectral-Timing Properties of Tidal Disruption Events

Joheen Chakraborty, Megan Masterson, Andrew Mummery +4

We perform the first systematic study of the minute-to-hours-timescale stochastic variability observed in the X-ray luminosity of tidal disruption events (TDEs) using XMM-Newton da…

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.HE2026★ 1 cited

Disk-to-Corona State Transition and Extreme X-ray Variability in the Tidal Disruption Event AT2019teq

Vera Berger, Erin Kara, Joheen Chakraborty +2

We present a five-year X-ray spectral and timing analysis of the optically selected Tidal Disruption Event (TDE) AT2019teq, which displays extreme variability, including order-of-m…

astro-ph.HE2026★ 2 cited

XRISM finds the Changing-Look AGN NGC 1365 in an extended low state: A dense, highly ionized outflow obscures the central source

Fatima Zaidouni, Erin Kara, Peter Kosec +21

We present the first XRISM/Resolve observations of the active galactic nucleus, NGC 1365, obtained in 2024 February and July. NGC 1365 is known for rapid transitions between Compto…

astro-ph.HE2025★ 3 cited

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.HE2025

Prospects for EMRI/MBH parameter estimation using Quasi-Periodic Eruption timings: short-timescale analysis

Joheen Chakraborty, Lisa V. Drummond, Matteo Bonetti +11

Quasi-Periodic Eruptions (QPEs) are luminous, recurring X-ray outbursts from galactic nuclei, with timescales of hours to days. While their origin remains uncertain, leading models…

astro-ph.HE2025

Millihertz Oscillations Near the Innermost Orbit of a Supermassive Black Hole

Megan Masterson, Erin Kara, Christos Panagiotou +22

Recent discoveries from time-domain surveys are defying our expectations for how matter accretes onto supermassive black holes (SMBHs). The increased rate of short-timescale, repet…

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.HE2024★ 18 cited

Eppur si muove: Evidence of disc precession or a sub-milliparsec SMBH binary in the QPE-emitting galaxy GSN 069

Giovanni Miniutti, Alessia Franchini, Matteo Bonetti +8

X-ray quasi-periodic eruptions (QPEs) are intense soft X-ray bursts from the nuclei of nearby low-mass galaxies typically lasting about one hour and repeating every few. Their phys…

astro-ph.HE2024

Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks

Joheen Chakraborty, Kevin B. Burdge, Saul A. Rappaport +35

We report the discovery of three ultracompact binary white dwarf systems hosting accretion disks, with orbital periods of 7.95, 8.68, and 13.15 minutes. This significantly augments…

astro-ph.HE2023★ 62 cited

Alive and kicking: A new QPE phase in GSN 069 revealing a quiescent luminosity threshold for QPEs

G. Miniutti, M. Giustini, R. Arcodia +4

X-ray quasi-periodic eruptions (QPEs) are intense repeating soft X-ray bursts from the nuclei of nearby galaxies. Their physical origin is still largely unconstrained, and several…

astro-ph.EP2022★ 3 cited

Transit Duration and Timing Variations from Binary Planets

Joheen Chakraborty, David Kipping

Systems of two gravitationally bound exoplanets orbiting a common barycenter outside their physical radii ("binary planets") may result from tidal capture during planet-planet scat…

astro-ph.SR2021★ 205 cited

TESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26

Andrej Prsa, Angela Kochoska, Kyle E. Conroy +44

In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binar…

astro-ph.HE2021★ 137 cited

Possible X-ray Quasi-Periodic Eruptions in a Tidal Disruption Event Candidate

Joheen Chakraborty, Erin Kara, Megan Masterson +3

X-ray Quasi-Periodic Eruptions (QPEs) are a recently discovered phenomenon associated with supermassive black holes at the centers of galaxies. They are high amplitude soft X-ray f…

astro-ph.EP2020★ 7 cited

Hundreds of new periodic signals detected in the first year of with the

Joheen Chakraborty, Adam Wheeler, David Kipping

We apply the , a nonparametric signal detection algorithm based on phase dispersion minimization, in a search for low duty-cycle periodic signals in the Transi…