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20242026
most citedJWST Spectroscopy of SN Ia 2022aaiq and 2024gy: Evidence for Enhanced Central Stable Ni Abundance and a Deflagration-to-Detonation Transition

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astro-ph.HE2024

Spectral dataset of young type Ib supernovae and their time evolution

N. Yesmin, C. Pellegrino, M. Modjaz +11

Due to high-cadence automated surveys, we can now detect and classify supernovae (SNe) within a few days after explosion, if not earlier. Early-time spectra of young SNe directly p…

astro-ph.HE2024

Detection of an Orphan X-ray Flare from a Blazar Candidate EP240709a with Einstein Probe

Mingjun Liu, Yijia Zhang, Yun Wang +49

Blazars are often observed to flare across multiple wavelengths. Orphan flares from blazars have been only detected a few times, providing an opportunity to understand the structur…

astro-ph.HE2024

Probing the Circumstellar Environment of highly luminous type IIn SN ASASSN-14il

Naveen Dukiya, Anjasha Gangopadhyay, Kuntal Misra +8

We present long-term photometric and spectroscopic studies of Circumstellar Material (CSM)-Ejecta interacting supernova (SN) ASASSN-14il in the galaxy PGC 3093694. The SN reaches a…

astro-ph.HE2024

Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor

Aravind P. Ravi, Stefano Valenti, Yize Dong +34

We present supernova (SN) 2023ufx, a unique Type IIP SN with the shortest known plateau duration ( 47 days), a luminous V-band peak ( = 18.42 0…

astro-ph.HE2024

Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties

Yize Dong, Stefano Valenti, Chris Ashall +52

We present optical and near-infrared observations of SN~2022crv, a stripped envelope supernova in NGC~3054, discovered within 12 hrs of explosion by the Distance Less Than 40 Mpc S…

astro-ph.IM2024

SAGUARO: Time-domain Infrastructure for the Fourth Gravitational-wave Observing Run and Beyond

Griffin Hosseinzadeh, Kerry Paterson, Jillian C. Rastinejad +14

We present upgraded infrastructure for Searches after Gravitational Waves Using ARizona Observatories (SAGUARO) during LIGO, Virgo, and KAGRA's fourth gravitational-wave (GW) obser…