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Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS

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arxiv 1904.09293 v2 pith:AU375LVJ submitted 2019-04-19 astro-ph.HE

classification astro-ph.HE
keywords daysobservationspeakasassn-19btearlytessbeforedataset
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abstract

We present the discovery and early evolution of ASASSN-19bt, a tidal disruption event (TDE) discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) at a distance of $d\simeq115$ Mpc and the first TDE to be detected by TESS. As the TDE is located in the TESS Continuous Viewing Zone, our dataset includes 30-minute cadence observations starting on 2018 July 25, and we precisely measure that the TDE begins to brighten $\sim8.3$ days before its discovery. Our dataset also includes 18 epochs of Swift UVOT and XRT observations, 2 epochs of XMM-Newton observations, 13 spectroscopic observations, and ground data from the Las Cumbres Observatory telescope network, spanning from 32 days before peak through 37 days after peak. ASASSN-19bt thus has the most detailed pre-peak dataset for any TDE. The TESS light curve indicates that the transient began to brighten on 2019 January 21.6 and that for the first 15 days its rise was consistent with a flux $\propto t^2$ power-law model. The optical/UV emission is well-fit by a blackbody SED, and ASASSN-19bt exhibits an early spike in its luminosity and temperature roughly 32 rest-frame days before peak and spanning up to 14 days that has not been seen in other TDEs, possibly because UV observations were not triggered early enough to detect it. It peaked on 2019 March 04.9 at a luminosity of $L\simeq1.3\times10^{44}$ ergs s$^{-1}$ and radiated $E\simeq3.2\times10^{50}$ ergs during the 41-day rise to peak. X-ray observations after peak indicate a softening of the hard X-ray emission prior to peak, reminiscent of the hard/soft states in X-ray binaries.

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Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Delay Time Distribution of Quasi-Periodic Eruptions

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    QPE host galaxies are more likely to have recently formed a large burst of stars (burst mass fraction above 1%) than TDE host galaxies or mass- and redshift-matched controls.

  2. ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    The tidal disruption event ATLAS22kjn shows a resolved 9-day pre-peak bump, coronal lines that imply a stable ~1e6 K ionising source, and a dust echo whose covering fraction is much higher than typical TDEs.

  3. The Radio Properties of Extreme Coronal Line Emitters: Constraints on the Sub-parsec Environment

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    About half of low-redshift ECLEs are radio-bright like TDEs/AGN; SED modeling of four shows the ECL gas is clumpy (f_V ~ 10^{-5}-10^{-2}) and spatially distinct from the radio-emitting region.

  4. AT2021yky: A Fast-Rising Optical Transient with Evolving Broad Hydrogen Emission Consistent with an Ambiguous Nuclear Transient

    astro-ph.HE 2026-08 accept novelty 5.0 of 10

    AT2021yky is a fast-rising, cool nuclear flare with only broad H-alpha emission, best classified as an ambiguous nuclear transient rather than a typical TDE, AGN flare, supernova, or LFBOT.

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