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20242026
most citedInvestigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity

10 citations · 16 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.IM2026

A data processing pipeline for the WINTER near-infrared surveyor using the framework

Viraj Karambelkar, Robert Stein, Danielle Frostig +18

We present the data reduction and transient detection pipeline for the Wide-field Infrared Transient Explorer (WINTER) surveyor and report its on-sky performance. The WINTER camera…

astro-ph.HE2026

Multi-Wavelength Identification of a Luminous Mid-Infrared Supernova Powered by Circumstellar Interaction with Binary-Driven Pre-supernova Mass Loss

Kohki Uno, Kishalay De, Geoffrey Mo +6

Terminal mass-loss in massive stars is commonly reconstructed from observations of circumstellar interaction in core-collapse supernovae (CCSNe); however, such signatures can be ea…

astro-ph.SR2026

TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf

Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev +14

Classical novae are transient events powered by thermonuclear burning in a layer of hydrogen-rich material accreted by a white dwarf from its binary companion. Most classical novae…

astro-ph.HE2026

SN~2018erx: A fast-evolving, dust-reddened Type Icn supernova with broad C II emission lines

Kaustav K. Das, Anjasha Gangopadhyay, Mansi M. Kasliwal +17

We present the discovery and characterization of SN~2018erx (ZTF18abkmbpy), a fast-evolving, unusually red, interacting stripped-envelope supernova. Spectroscopically, SN~2018erx s…

astro-ph.HE2026

The rise of the black hole X-ray binary AT2019wey observed with TESS

Alyana Jusino, Kishalay De, Andrea Antoni

Black hole X-ray binaries (BHXRBs) have traditionally been discovered by X-ray surveys with cadences of hours to days. However, large optical time-domain surveys now provide novel…

astro-ph.SR2026

Fading into darkness: A weak mass ejection and low-efficiency fallback accompanying black hole formation in M31-2014-DS1

Kishalay De, Morgan MacLeod, Jacob E. Jencson +10

Stellar-mass black holes (BHs) can form from the near-complete collapse of massive stars, causing them to abruptly disappear. The star M31-2014-DS1 in the Andromeda galaxy was repo…

astro-ph.SR2026

SPHEREx as a frontier for infrared transients: Classification of new Galactic FU Ori outbursts and classical novae

Viraj Karambelkar, Kishalay De, Lynne A. Hillenbrand +3

We demonstrate proof-of-concept of a new strategy for studying infrared (IR) transients enabled by the newly launched SPHEREx space mission, by leveraging its synergy with the NEOW…

astro-ph.SR2026★ 4 cited

Peculiar SN Ic 2022esa: An explosion of a massive Wolf-Rayet star in a binary as a precursor to a BH-BH binary?

Keiichi Maeda, Hanindyo Kuncarayakti, Takashi Nagao +4

A class of supernovae (SNe) termed `SN Ic-CSM' are characterized by late-time emergence of narrow emission lines of elements formed in the oxygen core of a massive star. A popular…

astro-ph.IM2025

Dynamical binary interactions in the 2040s

Nadejda Blagorodnova, Ondřej Pejcha, Tomek Kamiński +15

Dynamical binary interactions such as common envelope (CE) evolution or stellar mergers are a critical phase in the formation of a wide variety of binary phenomena, ranging from bl…

astro-ph.IM2025

The WINTER Observatory: A One-Degree InGaAs Survey Camera to study the Transient Infrared Sky

Danielle Frostig, Nathan Lourie, Viraj Karambelkar +20

The Wide-field Infrared Transient Explorer (WINTER) is a near-infrared time-domain survey instrument operating on a dedicated 1-meter robotic telescope at Palomar Observatory. The…

astro-ph.SR2025

A spectral library and census of near-infrared stellar large-amplitude variables from Palomar Gattini-IR

Nicholas Earley, Viraj Karambelkar, Mansi Kasliwal +9

We present a near-infrared census of stellar large-amplitude variables (LAVs) observed by the Palomar Gattini-IR (PGIR) surveyor from 2019-2021. Over the three-year time period, PG…

astro-ph.HE2025★ 1 cited

Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe

Peter Scherbak, Abigail Polin, Mansi Kasliwal +4

Calcium-rich gap transients are a faint, fast-evolving class of supernovae that show strong nebular Ca emission lines. Their progenitor systems are uncertain, but they are often as…

astro-ph.SR2025

Multi-color characterization of optically invisible FU Orionis-type outbursts: Demonstration and prospects for the WINTER survey

Danielle Frostig, Kishalay De, Lynne A. Hillenbrand +8

Episodic mass accretion is the dominant mechanism for mass assembly in the proto-stellar phase. Although prior optical time-domain searches have allowed detailed studies of individ…

astro-ph.SR2025★ 1 cited

Hot springs and dust reservoirs: JWST reveals the dusty, molecular aftermath of extragalactic stellar mergers

Viraj Karambelkar, Mansi Kasliwal, Ryan M. Lau +7

We present James Webb Space Telescope (JWST) observations of four Luminous Red Novae (LRNe): dusty, extragalactic transients from stellar mergers following common-envelope evolutio…

astro-ph.SR2025

The slow brightening of WNTR23bzdiq / WTP19aalzlk : Possible onset of common-envelope evolution in an asymptotic giant branch star?

Viraj Karambelkar, Mansi Kasliwal, Kishalay De +6

We present WNTR23bzdiq/WTP19aalzlk, a slow eruption of an early-asymptotic giant branch (AGB) star in M31 identified by the Wide-field Infrared Transient Explorer (WINTER) near-inf…

astro-ph.EP2025

A Machine-Learning Compositional Study of Exoplanetary Material Accreted Onto Five Helium-Atmosphere White Dwarfs with

Mariona Badenas-Agusti, Siyi Xu, Andrew Vanderburg +8

We present the first application of the Machine Learning (ML) pipeline to determine the physical parameters and photospheric composition of five metal-polluted H…

astro-ph.SR2024★ 10 cited

Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity

S. de Wit, A. Z. Bonanos, K. Antoniadis +8

Mass loss during the red supergiant (RSG) phase plays a crucial role in the evolution of an intermediate massive star, however, the underlying mechanism remains unknown. We aim to…