activity
20052021
most citedThe Type II-P Supernova 2017eaw: from explosion to the nebular phase

86 citations · 258 across the 8 of their papers we have counts for

collaborators

14 papers

astro-ph.SR20211 cited

A study of the photometric and spectroscopic variations of the prototypical FU Orionis-type star V1057 Cyg

Zs. M. Szabó, Á. Kóspál, P. Ábrahám +19

Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057 Cyg, a classical exa…

astro-ph.SR20218 cited

Dipper-like variability of the Gaia alerted young star V555 Ori

Zsófia Nagy, Elza Szegedi-Elek, Péter Ábrahám +26

V555 Ori is a T Tauri star, whose 1.5 mag brightening was published as a Gaia science alert in 2017. We carried out optical and near-infrared photometric, and optical spectroscopic…

astro-ph.EP2021

101 Trojans: a tale of period bimodality, binaries, and extremely slow rotators from K2 photometry

Csilla E. Kalup, László Molnár, Csaba Kiss +8

Various properties of Jovian trojan asteroids such as composition, rotation periods, and photometric amplitudes, or the rate of binarity in the population can provide information a…

astro-ph.HE202140 cited

The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

Danfeng Xiang, Xiaofeng Wang, Weili Lin +47

We present our photometric and spectroscopic observations on the peculiar transient AT2018cow. The multi-band photometry covers from peak to 70 days and the spectroscopy rang…

astro-ph.HE202070 cited

SN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral Features

Wynn V. Jacobson-Galán, Raffaella Margutti, Charles D. Kilpatrick +64

We present panchromatic observations and modeling of the Calcium-rich supernova 2019ehk in the star-forming galaxy M100 (d16.2 Mpc) starting 10 hours after explosion and c…

astro-ph.HE2019

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…