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, Jack M., M. Neustadt, Katie Auchettl, Patrick J. Vallely, Melissa Shahbandeh, Matthias, Kluge, Christopher S. Kochanek, K. Z. Stanek, Mark E. Huber, Richard S. Post,, David Bersier, Christopher Ashall

TL;DR
This paper reports detailed multi-wavelength observations of ASASSN-20hx, a nuclear transient with ambiguous classification, highlighting its slow evolution, luminous UV/X-ray emission, and spectral peculiarities that challenge existing categories.
Contribution
The study provides comprehensive temporal and spectral data on ASASSN-20hx, revealing its unique slow decline and spectral features, and discusses its ambiguous nature between TDEs and AGNs.
Findings
ASASSN-20hx peaked in UV/optical 30 days after discovery.
X-ray luminosity increased significantly before declining.
Spectra lack emission lines, unusual for nuclear transients.
Abstract
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 ASASSN-20hx from 30 to 275 days relative to peak UV/optical emission using high-cadence, multi-wavelength spectroscopy and photometry. From Transiting Exoplanet Survey Satellite (TESS) data, we determine that the ANT began to brighten on 2020 June 22.8 with a linear rise in flux for at least the first week. ASASSN-20hx peaked in the UV/optical 30 days later on 2020 July 22.8 (MJD = 59052.8) at a bolometric luminosity of erg s. The subsequent decline is slower than any TDE observed to date and consistent with many other ANTs. Compared to an archival X-ray detection, the X-ray luminosity of ASASSN-20hx increased by an order of magnitude to $L_{x} \sim 1.5 \times…
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