activity
20062024
most citedA change in the optical polarization associated with a gamma-ray flare in the blazar 3C 279

334 citations · 2.5k across the 72 of their papers we have counts for

collaborators

70 papers

astro-ph.HE2024

SN 2021foa: the bridge between SN IIn and Ibn

Anjasha Gangopadhyay, Naveen Dukiya, Takashi J Moriya +26

We present the long-term photometric and spectroscopic analysis of a transitioning SN~IIn/Ibn from 10.8 d to 150.7 d post -band maximum. SN~2021foa shows prominent He {\sc i}…

astro-ph.SR2024

MASTER OT J030227.28+191754.5: an unprecedentedly energetic dwarf nova outburst

Yusuke Tampo, Taichi Kato, Keisuke Isogai +60

We present a detailed study of the MASTER OT J030227.28+191754.5 outburst in 2021-2022, reaching an amplitude of 10.2 mag and a duration of 60 d. The detections of (1) the double-p…

astro-ph.HE2024

Intermediate-luminosity Type IIP SN 2021gmj: a low-energy explosion with signatures of circumstellar material

Yuta Murai, Masaomi Tanaka, Miho Kawabata +28

We present photometric, spectroscopic and polarimetric observations of the intermediate-luminosity Type IIP supernova (SN) 2021gmj from 1 to 386 days after the explosion. The peak…

astro-ph.SR2023

Spectra of V1405 Cas at the very beginning indicate a low-mass ONeMg white dwarf progenitor

Kenta Taguchi, Keiichi Maeda, Hiroyuki Maehara +9

The lowest possible mass of ONeMg white dwarfs (WDs) has not been clarified despite its importance in the formation and evolution of WDs. We tackle this issue by studying the prope…

astro-ph.HE2023★ 18 cited

Gamma rays from a reverse shock with turbulent magnetic fields in GRB 180720B

Makoto Arimoto, Katsuaki Asano, Koji S. Kawabata +14

Gamma-ray bursts (GRBs) are the most electromagnetically luminous cosmic explosions. They are powered by collimated streams of plasma (jets) ejected by a newborn stellar-mass black…

astro-ph.HE2023

Bridging between type IIb and Ib supernovae: SN IIb 2022crv with a very thin Hydrogen envelope

Anjasha Gangopadhyay, Keiichi Maeda, Avinash Singh +26

We present optical, near-infrared, and radio observations of supernova (SN) SN~IIb 2022crv. We show that it retained a very thin H envelope and transitioned from a SN~IIb to a SN~I…