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20112026
most citedSN 2017gmr: An energetic Type II-P supernova with asymmetries

53 citations · 394 across the 42 of their papers we have counts for

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astro-ph.HE2019★ 35 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.HE2019★ 9 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.HE2019★ 28 cited

Multi-band optical variability of 3C 279 on diverse timescales

Aditi Agarwal, Sergio A. Cellone, Ileana Andruchow +8

We have monitored the flat spectrum radio quasar, 3C 279, in the optical , , and passbands from 2018 February to 2018 July for 24 nights, with a total of 716 frames,…

astro-ph.HE2019★ 53 cited

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…

astro-ph.GA2019★ 26 cited

A low-frequency study of recently identified double-double radio galaxies

S. Nandi, D. J. Saikia, R. Roy +6

In order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasars, which are still unclear, we have identified such sources with a large range…

astro-ph.HE2019★ 7 cited

SN 2016B a.k.a ASASSN-16ab: a transitional type II supernova

Raya Dastidar, Kuntal Misra, Mridweeka Singh +12

We present photometry, polarimetry and spectroscopy of the Type II supernova ASASSN-16ab/SN 2016B in PGC 037392. The photometric and spectroscopic follow-up commenced about two wee…