activity
20172026
most citedSN 2017gmr: An energetic Type II-P supernova with asymmetries

53 citations · 516 across the 50 of their papers we have counts for

collaborators

50 papers

astro-ph.HE2026

Tomography analysis of the intermediate-luminosity Type Iax SN 2024pxl

Barnabás Barna, Mridweeka Singh, Lindsey A. Kwok +90

We present an abundance tomography analysis of SN 2024pxl, an intermediate luminosity Type Iax supernova ( mag), with the most-detailed follow-up in the Type…

astro-ph.HE2026

Wild behaviour near the finish line: the Type Ibn SN 2020able and its stratified environment

L. Tartaglia, E. Cappellaro, G. Valerin +29

We present spectrophotometric observations of the Type Ibn supernova SN~2020able, along with a comprehensive analysis and modelling of its evolution. The transient occurred in SDSS…

astro-ph.HE2026

SN 2022xus: bridging the gap between Type IIP and IIL supernovae

Monalisa Dubey, Kuntal Misra, Naveen Dukiya +16

We present optical photometric and spectroscopic observations of the Type~II supernova SN~2022xus. The SN reached its peak {\em V} band magnitude of mag within 7 day…

astro-ph.HE2026

Early Near-Infrared Excess and Rapid Disk-Corona Evolution in the Tidal Disruption Event 2024aepd

Yongxin Wu, Yanan Wang, Thomas M. Reynolds +38

We present multi-wavelength observations of the tidal disruption event (TDE) 2024aepd, spanning primarily the first 300 days after discovery. A prominent near-infrared (NIR)…

astro-ph.HE2026

SN 2023zcu: A Type IIP SN with Early Flash Features

Monalisa Dubey, Kuntal Misra, Géza Csörnyei +51

We present a detailed photometric and spectroscopic analysis of the Type IIP supernova SN~2023zcu, which exploded in the galaxy NGC~2139 (redshift = 0.006). SN~2023zcu exhibits…

astro-ph.HE2026

A Study of Two Type IIb Supernovae: SNe 2008aq and 2019gaf

Mridweeka Singh, Devendra K. Sahu, Raya Dastidar +12

We present photometric and spectroscopic studies of two core-collapse supernovae (SNe) 2008aq and 2019gaf in the optical wavelengths. Light curve and spectral sequence of both the…

astro-ph.HE2026

SN 2024abfl: A Flat-Plateau, Low-Luminosity Type IIP Supernova with Early CSM Interaction

Madison Gerard, Jennifer E. Andrews, Geoffrey C. Clayton +29

We present photometric and spectroscopic observations of SN 2024abfl, a low-luminosity Type IIP supernova (LLSN) discovered shortly after explosion. The transient reached a peak ab…

astro-ph.HE2025

SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host

R. Dastidar, G. Pignata, N. Dukiya +14

We present the analysis of the luminous Type II Supernova (SN) 2021tsz, which exploded in a low-luminosity galaxy. It reached a peak magnitude of -18.88 0.13 mag in the b…

astro-ph.HE2025

Progenitor Insights of Type IIP SN 2018pq: A Comprehensive Photometric and Spectroscopic Study

Monalisa Dubey, Kuntal Misra, Raya Dastidar +10

We present high-cadence photometric and low-resolution (R 400--700) optical spectroscopic observations of Type IIP supernova, SN~2018pq, which exploded on the outskirts of t…

astro-ph.HE2025★ 1 cited

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 rem…

astro-ph.HE2025★ 13 cited

JWST and Ground-based Observations of the Type Iax Supernovae SN 2024pxl and SN 2024vjm: Evidence for Weak Deflagration Explosions

Lindsey A. Kwok, Mridweeka Singh, Saurabh W. Jha +89

We present panchromatic optical near-infrared (NIR) mid-infrared (MIR) observations of the intermediate-luminosity Type Iax supernova (SN Iax) 2024pxl and the extremely low…

astro-ph.HE2025

Photometry and Spectroscopy of SN 2024pxl: A Luminosity Link Among Type Iax Supernovae

Mridweeka Singh, Lindsey A. Kwok, Saurabh W. Jha +90

We present extensive ultraviolet to optical photometric and optical to near-infrared (NIR) spectroscopic follow-up observations of the nearby intermediate-luminosity ($M_V = -16.81…

astro-ph.HE2025★ 8 cited

Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems

Bastian Ayala, Joseph P. Anderson, G. Pignata +8

Type IIb supernovae (SNe IIb) often exhibit an early light curve excess (EE) preceding the main peak powered by radioactive nickel decay. The physical origin of this early emission…

astro-ph.HE2025★ 15 cited

SN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases

R. Dastidar, K. Misra, S. Valenti +31

We present a comprehensive photometric and spectroscopic study of the Type IIP SN 2018is. The -band luminosity and the expansion velocity at 50 days post-explosion are 15.1$\…

astro-ph.HE2024

Signatures of the Shock Interaction as an Additional Power Source in the Nebular Spectra of SN 2023ixf

Amit Kumar, Raya Dastidar, Justyn R. Maund +2

Red supergiants may lose significant mass during the final 100-1000 years before core collapse, shaping their circumstellar environment. The supernova (SN) shockwave propagating th…

astro-ph.GA2024★ 1 cited

AT 2021hdr: A candidate tidal disruption of a gas cloud by a binary super massive black hole system

L. Hernández-García, A. M. Muñoz-Arancibia, P. Lira +25

With a growing number of facilities able to monitor the entire sky and produce light curves with a cadence of days, in recent years there has been an increased rate of detection of…

astro-ph.HE2024★ 4 cited

The fast rise of the unusual Type IIL/IIb SN 2018ivc

A. Reguitti, R. Dastidar, G. Pignata +22

We present an analysis of the photometric and spectroscopic dataset of the Type II supernova (SN) 2018ivc in the nearby (10 Mpc) galaxy Messier 77. Thanks to the high cadence of th…

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.HE2024

CSS161010: a luminous, fast blue optical transient with broad blueshifted hydrogen lines

Claudia P. Gutiérrez, Seppo Mattila, Peter Lundqvist +38

We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (…

astro-ph.SR2024★ 8 cited

A study in scarlet -- I. Photometric properties of a sample of Intermediate Luminosity Red Transients

G. Valerin, A. Pastorello, A. Reguitti +57

We investigate the photometric characteristics of a sample of Intermediate Luminosity Red Transients (ILRTs), a class of elusive objects with peak luminosity between that of classi…

astro-ph.SR2024

Unveiling the nature of two dwarf novae: CRTS J080846.2+313106 and V416 Dra

Arti Joshi, Márcio Catelan, Simone Scaringi +8

We present the analysis of optical photometric and spectroscopic observations of two non-magnetic cataclysmic variables, namely CRTS J080846.2+313106 and V416 Dra. CRTS J080846.2+3…

astro-ph.HE2024★ 1 cited

Magnetars as Powering Sources of Gamma-Ray Burst Associated Supernovae, and Unsupervised Clustering of Cosmic Explosions

Amit Kumar, Kaushal Sharma, Jozsef Vinkó +7

We present the semi-analytical light curve modelling of 13 supernovae associated with gamma-ray bursts (GRB-SNe) along with two relativistic broad-lined (Ic-BL) SNe without GRBs as…

astro-ph.HE2024★ 16 cited

Searching for precursor activity of Type IIn Supernovae

A. Reguitti, G. Pignata, A. Pastorello +4

We conducted a search for luminous outbursts prior to the explosion of Type IIn Supernovae (SNe IIn). We built a sample of 27 objects spectroscopically classified as SNe IIn, all l…

astro-ph.HE2024★ 8 cited

SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures

Raya Dastidar, Giuliano Pignata, Naveen Dukiya +9

We present an optical photometric and spectroscopic analysis of the fast-declining hydrogen-rich Type II supernova (SN) 2019nyk. The light curve properties of SN 2019nyk align well…