activity
20182021
most citedIntermediate Luminosity Type Iax SN 2019muj With Narrow Absorption Lines: Long-Lasting Radiation Associated With a Possible Bound Remnant Predicted by the Weak Deflagration Model

19 citations · 44 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.HE202119 cited

Intermediate Luminosity Type Iax SN 2019muj With Narrow Absorption Lines: Long-Lasting Radiation Associated With a Possible Bound Remnant Predicted by the Weak Deflagration Model

Miho Kawabata, Keiichi Maeda, Masayuki Yamanaka +23

We present comprehensive spectroscopic and photometric analyses of the intermediate luminosity Type Iax supernova (SN Iax) 2019muj based on multi-band datasets observed through the…

astro-ph.SR20218 cited

SN 2017hpa: A carbon-rich type Ia supernova

Anirban Dutta, Avinash Singh, G. C. Anupama +2

We present the optical (UBVRI) and ultraviolet (Swift-UVOT) photometry, and optical spectroscopy of Type Ia supernova SN 2017hpa. We study broadband UV+optical light curves and low…

astro-ph.HE202117 cited

SN 2020ank: a bright and fast-evolving H-deficient superluminous supernova

Amit Kumar, Brajesh Kumar, S. B. Pandey +7

We investigate the observational properties of a hydrogen-deficient superluminous supernova (SLSN) SN 2020ank (at z = 0.2485), with the help of early phase observations carried out…

astro-ph.HE2020

Kilonova Luminosity Function Constraints based on Zwicky Transient Facility Searches for 13 Neutron Star Mergers

Mansi M. Kasliwal, Shreya Anand, Tomas Ahumada +100

We present a systematic search for optical counterparts to 13 gravitational wave (GW) triggers involving at least one neutron star during LIGO/Virgo's third observing run. We searc…

astro-ph.HE2019

SN 2018hna: 1987A-like supernova with a signature of shock breakout

Avinash Singh, D. K. Sahu, G. C. Anupama +22

High cadence ultraviolet, optical and near-infrared photometric and low-resolution spectroscopic observations of the peculiar Type II supernova (SN) 2018hna are presented. The earl…

astro-ph.HE2019

GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR

Michael W. Coughlin, Tomás Ahumada, Shreya Anand +76

The third observing run by LVC has brought the discovery of many compact binary coalescences. Following the detection of the first binary neutron star merger in this run (LIGO/Virg…