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20242026
most citedMultiwavelength Modeling of the Luminous Fast Blue Optical Transient AT2024wpp

1 citations · 1 across the 3 of their papers we have counts for

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9 papers

astro-ph.HE2026

A JWST/MIRI Study of Dust in a Sample of Normal Type IIP Core Collapse Supernovae

Bhagya M. Subrayan, David J. Sand, Olivia Culbert +24

Core collapse supernovae (CCSNe) are invoked as major dust producers in the early Universe, yet the amount of dust they form, the timescale over which it grows, and the physical co…

astro-ph.HE2026

First Results from the LSST Shadow Survey: The Restless Luminous Blue Variable AT2017des in the Virgo-Cluster Galaxy, NGC4532

Conor L. Ransome, Bhagya M. Subrayan, David J. Sand +66

The Legacy Survey of Space and Time (LSST) will start in late-summer 2026, revolutionizing transient astronomy. Here, we present the Dark Energy Camera (DECam) Shadow Survey, which…

astro-ph.HE20261 cited

Multiwavelength Modeling of the Luminous Fast Blue Optical Transient AT2024wpp

Conor M. B. Omand, Nikhil Sarin, Gavin P. Lamb +14

Luminous fast blue optical transients (LFBOTs) are a growing class of enigmatic energetic transients. They show fast rises and declines, high temperatures throughout their evolutio…

astro-ph.HE2026

JWST spectroscopy of SN 2010da/NGC 300 ULX-1: a surviving star hidden by dust

Emma R. Beasor, Ryan Lau, Nathan Smith +3

We present new James Webb Space Telescope () NIRSpec and MIRI integral-field spectroscopy of the remarkable system SN~2010da / NGC~300 ULX-1, the only known ultraluminous X-r…

astro-ph.SR2026

The fate of the failed supernova candidate M31-2014-DS1

Emma R. Beasor, Nathan Smith, Jeniveve Pearson +4

The fate of massive stars above 20M remains uncertain. Debate persists about whether they die as supernovae (SNe), or if they collapse directly into black holes (BHs) wit…

astro-ph.SR2025

Quantifying Systematic Age Discrepancies in Very Young Star Clusters

Joseph Guzman, Jeremiah Murphy, Emma Beasor +5

We infer the ages of three young stellar clusters, NGC 2004, NGC 7419, and NGC 2100, using Stellar Ages, a statistical algorithm designed to infer stellar population properties fro…