activity
20192026
most citedThe Rise and Fall of ASASSN-18pg: Following a TDE from Early To Late Times

64 citations · 181 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2026

The flash-ionised SN Ibn 2025kzr: H-free CSM formed during a precursor outburst 55 days prior to explosion

S. de Wet, G. Leloudas, D. A. H. Buckley +33

Type Ibn supernovae (SNe) are a class of interacting SNe characterised by narrow helium lines in their spectra. We present an extensive observational dataset of the Type Ibn SN 202…

astro-ph.HE2025★ 15 cited

SN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases

R. Dastidar, K. Misra, S. Valenti +31

We present a comprehensive photometric and spectroscopic study of the Type IIP SN 2018is. The -band luminosity and the expansion velocity at 50 days post-explosion are 15.1$\…

astro-ph.SR2024★ 3 cited

Gaia20bdk -- a new FUor in Sh 2-301 Star Forming Region

M. Siwak, Á. Kóspál, P. Ábrahám +28

Context. We analyse multi-colour photometric and spectroscopic observations of a Young Stellar Object Gaia20bdk. Aims. We aim to investigate the exact nature of the eruptive phenom…

astro-ph.HE2023

Transient fading X-ray emission detected during the optical rise of a tidal disruption event

A. Malyali, A. Rau, C. Bonnerot +9

We report on the SRG/eROSITA detection of ultra-soft ( eV) X-ray emission ( erg s) from the tidal disruptio…

astro-ph.HE2023★ 1 cited

Multiwavelength study of extreme variability in LEDA 1154204: A changing-look event in a type 1.9 Seyfert

T. Saha, A. Markowitz, D. Homan +16

Context. Multiwavelength studies of transients in actively accreting supermassive black holes have revealed that large-amplitude variability is frequently linked to significant cha…

astro-ph.HE2020★ 64 cited

The Rise and Fall of ASASSN-18pg: Following a TDE from Early To Late Times

Thomas W. -S. Holoien, Katie Auchettl, Michael A. Tucker +29

We present nearly 500 days of observations of the tidal disruption event ASASSN-18pg, spanning from 54 days before peak light to 441 days after peak light. Our dataset includes X-r…