collaborators

14 papers

astro-ph.HE2026

Heavy element dust explains the late-time spectra of kilonovae

Nanae Domoto, Kenta Hotokezaka, Daniel Kasen

Neutron star mergers are a leading site of -process, producing radioactively powered optical and infrared transients known as kilonovae. Observations of the kilonovae AT2017gfo,…

astro-ph.HE2026

Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy

Ido Keinan, Iair Arcavi, D. Andrew Howell +34

We present a summary of gravitational-wave (GW) follow-up using the Las Cumbres Observatory global network of telescopes during the third (O3) and fourth (O4) observing runs of the…

astro-ph.HE2026

The Light Curve of Wind-Reprocessed Tidal Disruption Events

Brenna Mockler, David Khatami, Daniel Kasen +2

The source of the optical/UV emission in tidal disruption events (TDEs) remains an enduring question in the field. Connecting the observed emission to the source is critical for bo…

astro-ph.GA2026

A Unified Ionization Framework for the Spectroscopic Diversity of Tidal Disruption Events

Lars L. Thomsen, Lixin Dai, Daniel Kasen +4

Optical tidal disruption events (TDEs) exhibit extremely broad emission lines (-) and are observationally classified into four spectroscopic typ…

astro-ph.HE2026

Collapse of Magnetized White Dwarfs as site of Heavy Element Formation and Kilonova Signal

Tetyana Pitik, David Radice, Daniel Kasen +3

We present the first end-to-end calculation connecting the accretion-induced collapse (AIC) of a magnetized, rapidly rotating white dwarf to observable kilonova signatures, combini…

astro-ph.HE2026

Gamma-ray Signatures of r-Process Radioactivity from the Collapse of Magnetized White Dwarfs

Tetyana Pitik, Yong-Zhong Qian, David Radice +1

We predict the gamma-ray line emission from -process nuclei synthesized in the ejecta of the accretion-induced collapse (AIC) of a magnetized, rapidly rotating white dwarf. Usin…