SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy

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Auteurs principaux: Hinkle, Jason T., Tucker, Michael A., Shappee, Benjamin. J., Holoien, Thomas W. -S., Vallely, Patrick J., de Jaeger, Thomas, Auchettl, Katie, Aldering, Greg, Ashall, Chris, Desai, Dhvanil D., Do, Aaron, Payne, Anna V., Tonry, John L.
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Publié: 2022
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author Hinkle, Jason T.
Tucker, Michael A.
Shappee, Benjamin. J.
Holoien, Thomas W. -S.
Vallely, Patrick J.
de Jaeger, Thomas
Auchettl, Katie
Aldering, Greg
Ashall, Chris
Desai, Dhvanil D.
Do, Aaron
Payne, Anna V.
Tonry, John L.
author_facet Hinkle, Jason T.
Tucker, Michael A.
Shappee, Benjamin. J.
Holoien, Thomas W. -S.
Vallely, Patrick J.
de Jaeger, Thomas
Auchettl, Katie
Aldering, Greg
Ashall, Chris
Desai, Dhvanil D.
Do, Aaron
Payne, Anna V.
Tonry, John L.
contents We present the discovery that ATLAS18mlw was a tidal disruption event (TDE) in the galaxy WISEA J073544.83+663717.3, at a luminosity distance of 334 Mpc. Initially discovered by the Asteroid Terrestrial Impact Last Alert System (ATLAS) on 2018 March 17.3, the TDE nature of the transient was uncovered only recently with the re-reduction of a SuperNova Integral Field Spectrograph (SNIFS) spectrum. This spectrum, taken by the Spectral Classification of Astronomical Transients (SCAT) survey, shows a strong blue continuum and a broad H$α$ emission line. Here we present roughly six years of optical survey photometry beginning before the TDE to constrain AGN activity, optical spectroscopy of the transient, and a detailed study of the host galaxy properties through analysis of archival photometry and a host spectrum. ATLAS18mlw was detected in ground-based light curves for roughly two months. From a blackbody fit to the transient spectrum and bolometric correction of the optical light curve, we conclude that ATLAS18mlw is best explained by a low-luminosity TDE with a peak luminosity of log(L [erg s$^{-1}$]) = $43.5 \pm 0.2$. The TDE classification is further supported by the quiescent Balmer strong nature of the host galaxy. We also calculated the TDE decline rate from the bolometric light curve and find $ΔL_{40} = -0.7 \pm 0.2$ dex, making ATLAS18mlw a member of the growing class of ``faint and fast'' TDEs with low peak luminosities and fast decline rates.
format Preprint
id arxiv_https___arxiv_org_abs_2202_05281
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy
Hinkle, Jason T.
Tucker, Michael A.
Shappee, Benjamin. J.
Holoien, Thomas W. -S.
Vallely, Patrick J.
de Jaeger, Thomas
Auchettl, Katie
Aldering, Greg
Ashall, Chris
Desai, Dhvanil D.
Do, Aaron
Payne, Anna V.
Tonry, John L.
High Energy Astrophysical Phenomena
We present the discovery that ATLAS18mlw was a tidal disruption event (TDE) in the galaxy WISEA J073544.83+663717.3, at a luminosity distance of 334 Mpc. Initially discovered by the Asteroid Terrestrial Impact Last Alert System (ATLAS) on 2018 March 17.3, the TDE nature of the transient was uncovered only recently with the re-reduction of a SuperNova Integral Field Spectrograph (SNIFS) spectrum. This spectrum, taken by the Spectral Classification of Astronomical Transients (SCAT) survey, shows a strong blue continuum and a broad H$α$ emission line. Here we present roughly six years of optical survey photometry beginning before the TDE to constrain AGN activity, optical spectroscopy of the transient, and a detailed study of the host galaxy properties through analysis of archival photometry and a host spectrum. ATLAS18mlw was detected in ground-based light curves for roughly two months. From a blackbody fit to the transient spectrum and bolometric correction of the optical light curve, we conclude that ATLAS18mlw is best explained by a low-luminosity TDE with a peak luminosity of log(L [erg s$^{-1}$]) = $43.5 \pm 0.2$. The TDE classification is further supported by the quiescent Balmer strong nature of the host galaxy. We also calculated the TDE decline rate from the bolometric light curve and find $ΔL_{40} = -0.7 \pm 0.2$ dex, making ATLAS18mlw a member of the growing class of ``faint and fast'' TDEs with low peak luminosities and fast decline rates.
title SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2202.05281