activity
20192026
most citedASASSN-14ko is a Periodic Nuclear Transient in ESO 253-G003

123 citations · 996 across the 68 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

astro-ph.SR2021

Flares Big and Small: a K2 and TESS View of ASAS-SN Superflares

Jesse Zeldes, Jason T. Hinkle, Benjamin J. Shappee +6

We investigate the flare-frequency distributions of 5 M-dwarfs that experienced superflares with energies in excess of erg detected by ASAS-SN. We use K2 and TESS short-c…

astro-ph.HE2021★ 28 cited

Investigating the Nature of the Luminous Ambiguous Nuclear Transient ASASSN-17jz

Thomas W. -S. Holoien, Jack M. M. Neustadt, Patrick J. Vallely +31

We present observations of the extremely luminous but ambiguous nuclear transient (ANT) ASASSN-17jz, spanning roughly 1200 days of the object's evolution. ASASSN-17jz was discovere…

astro-ph.HE2021★ 71 cited

The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient

Jason T. Hinkle, Thomas W. -S. Holoien, Benjamin. J. Shappee +22

We present observations of ASASSN-20hx, a nearby ambiguous nuclear transient (ANT) discovered in NGC 6297 by the All-Sky Automated Survey for Supernovae (ASAS-SN). We observed ASAS…

astro-ph.HE2021★ 31 cited

Fundamental X-ray Corona Parameters of Swift/BAT AGN

Jason T. Hinkle, Richard Mushotzky

While X-ray emission from active galactic nuclei (AGN) is common, the detailed physics behind this emission is not well understood. This is in part because high quality broadband s…

astro-ph.SR2021★ 24 cited

The Loudest Stellar Heartbeat: Characterizing the most extreme amplitude heartbeat star system

T. Jayasinghe, C. S. Kochanek, J. Strader +16

We characterize the extreme heartbeat star system MACHO 80.7443.1718 in the LMC using TESS photometry and spectroscopic observations from the Magellan Inamori Kyocera Echelle (MIKE…

astro-ph.HE2021★ 35 cited

The Rapid X-ray and UV Evolution of ASASSN-14ko

Anna V. Payne, Benjamin J. Shappee, Jason T. Hinkle +13

ASASSN-14ko is a recently discovered periodically flaring transient at the center of the AGN ESO 253-G003 with a slowly decreasing period. Here we show that the flares originate fr…