collaborators

6 papers

astro-ph.HE2026

Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse

Rishabh Singh Teja, D. K. Sahu, G. C. Anupama +7

We present extensive, well-sampled multiwavelength photometric and low-resolution optical spectroscopic observations of the low-luminosity Type IIP supernova SN 2024abfl. SN 2024ab…

astro-ph.HE2026

Two years of shock interaction tracing three phases of evolution: the explosion of a Type IIn supernova, SN 2019vxm

Gitika Rameshan, Rishabh Singh Teja, D. K. Sahu +10

We present multi-wavelength photometric and optical spectroscopic observations of the long-lived interacting supernova SN 2019vxm, spanning more than two years after the explosion.…

astro-ph.HE2026

SN 2024dy: Dust formation in a long-lived Type IIn supernova and constraints on the dust mass

Sota Goto, Masayuki Yamanaka, Koji S. Kawabata +10

Type~IIn supernovae (SNe) are a subclass of core-collapse SNe powered by interaction between the ejecta and the dense circumstellar material. Among them, long-lived Type~IIn events…

astro-ph.HE2026

Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST

Shigeo S. Kimura, Masaomi Tanaka, Seiji Toshikage +8

IceCube has been detecting cosmic high-energy neutrinos for more than 10 years, but their major sources are still under debate. To identify them, IceCube is issuing neutrino alerts…

astro-ph.HE2025

SN 2023xgo: Helium-rich Type Icn or Carbon-Flash Type Ibn supernova?

Anjasha Gangopadhyay, Jesper Sollerman, Konstantinos Tsalapatas +35

We present observations of SN~2023xgo, a transitional Type Ibn/Icn supernova, from to ~days relative to the -band peak. Early spectra show C~III emission re…

astro-ph.HE2025

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}…