collaborators

6 papers

astro-ph.SR2025

A New FU Orionis Accretion Outburst in the W5 HII Region

Lynne A. Hillenbrand, Matthew J. Graham, Mansi M. Kasliwal +9

We announce a recently detected outburst that is currently only a few months old, and probably of FU Orionis type. The progenitor to the outburst was an emission-line, flat-spectru…

astro-ph.SR2025

Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. II. Long-Timescale Variables including Wide Binary and Late Thermal Pulse Candidates

Soumyadeep Bhattacharjee, Nicole Reindl, Howard E. Bond +14

In this second paper on our variability survey of central stars of planetary nebulae (CSPNe) using ZTF, we report 11 long-timescale variables with variability timescales ranging fr…

astro-ph.SR2025

A ZTF Search for Circumstellar Debris Transits in White Dwarfs: Six New Candidates, one with Gas Disk Emission, identified in a Novel Metric Space

Soumyadeep Bhattacharjee, Zachary P. Vanderbosch, Mark A. Hollands +13

White dwarfs (WDs) showing transits from orbiting planetary debris provide significant insights into the structure and dynamics of debris disks. This is a rare class of objects wit…

astro-ph.GA2025

A Massive Black Hole 0.8 kpc from the Host Nucleus Revealed by the Offset Tidal Disruption Event AT2024tvd

Yuhan Yao, Ryan Chornock, Charlotte Ward +31

Tidal disruption events (TDEs) that are spatially offset from the nuclei of their host galaxies offer a new probe of massive black hole (MBH) wanderers, binaries, triples, and reco…

astro-ph.IM2025

Cryoscope: A Cryogenic Infrared Survey Telescope in Antarctica

Mansi M. Kasliwal, Nicholas Earley, Roger Smith +58

We present Cryoscope--a new 50 deg field-of-view, 1.2 m aperture, survey telescope to be located at Dome C, Antarctica. Cryoscope has an innovative optical-thermal d…

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…