activity
20172020
most citedThe Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days

152 citations · 483 across the 8 of their papers we have counts for

collaborators

12 papers

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.HE202022 cited

The low-luminosity type II SN\,2016aqf: A well-monitored spectral evolution of the Ni/Fe abundance ratio

Tomás E. Müller-Bravo, Claudia P. Gutiérrez, Mark Sullivan +20

Low-luminosity type II supernovae (LL SNe~II) make up the low explosion energy end of core-collapse SNe, but their study and physical understanding remain limited. We present SN\,2…

astro-ph.HE201935 cited

Flash ionization signatures in the type Ibn supernova SN 2019uo

Anjasha Gangopadhyay, Kuntal Misra, Daichi Hiramatsu +26

We present photometric and spectroscopic observations of the type Ibn supernova (SN) 2019uo, the second ever SN Ibn with flash ionization (He II, C III, N III) features in its earl…

astro-ph.SR2019

SN 2017cfd: A Normal Type Ia Supernova Discovered Very Young

Xuhui Han, WeiKang Zheng, Benjamin E. Stahl +22

The Type~Ia supernova (SN~Ia) 2017cfd in IC~0511 (redshift z = 0.01209+- 0.00016$) was discovered by the Lick Observatory Supernova Search 1.6+-0.7 d after the fitted first-light t…

astro-ph.HE20199 cited

SN 2015an: a normal luminosity type II supernova with low expansion velocity at early phases

Raya Dastidar, Kuntal Misra, Stefano Valenti +10

We present the photometry and spectroscopy of SN 2015an, a Type II Supernova (SN) in IC 2367. The recombination phase of the SN lasts up to 120 d, with a decline rate of 1.24…

astro-ph.SR2019

A luminous stellar outburst during a long-lasting eruptive phase first, and then SN IIn 2018cnf

A. Pastorello, A. Reguitti, A. Morales-Garoffolo +45

We present the results of the monitoring campaign of the Type IIn supernova (SN) 2018cnf (aka ASASSN-18mr). It was discovered about 10 days before the maximum light (on MJD = 58293…