activity
20132020
most citedDiscovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS

107 citations · 591 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2020★ 52 cited

The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151

Wenlong Yuan, Michael M. Fausnaugh, Samantha L. Hoffmann +15

We derive a distance of Mpc to the archetypical Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid Period-Luminosity relation and new Hubble Space Telescope…

astro-ph.HE2020★ 71 cited

Double-Peaked Balmer Emission Indicating Prompt Accretion Disk Formation in an X-Ray Faint Tidal Disruption Event

Tiara Hung, Ryan J. Foley, Enrico Ramirez-Ruiz +13

We present the multi-wavelength analysis of the tidal disruption event (TDE) AT~2018hyz (ASASSN-18zj). From follow-up optical spectroscopy, we detect the first unambiguous case of…

astro-ph.HE2019★ 107 cited

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

Thomas W. -S. Holoien, Patrick J. Vallely, Katie Auchettl +22

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\…

astro-ph.SR2018★ 55 cited

The largest M dwarfs flares from ASAS-SN

Sarah J. Schmidt, Benjamin J. Shappee, Jennifer L. van Saders +13

The All-Sky Automated Survey for Supernovae (ASAS-SN) is the only project in existence to scan the entire sky in optical light every day, reaching a depth of mag. O…

astro-ph.GA2018★ 76 cited

Continuum Reverberation Mapping of the Accretion Disks in Two Seyfert 1 Galaxies

M. M. Fausnaugh, D. A. Starkey, Keith Horne +69

We present optical continuum lags for two Seyfert 1 galaxies, MCG+08-11-011 and NGC 2617, using monitoring data from a reverberation mapping campaign carried out in 2014. Our light…

astro-ph.SR2016★ 22 cited

The Eruption of the Candidate Young Star ASASSN-15qi

Gregory J. Herczeg, Subo Dong, Benjamin J. Shappee +27

Outbursts on young stars are usually interpreted as accretion bursts caused by instabilities in the disk or the star-disk connection. However, some protostellar outbursts may not f…