Types of Transients in the Centers of Post-Starburst and Quiescent Balmer-Strong Galaxies
Iair Arcavi, Irura Nyiha, K. Decker French

TL;DR
This study investigates the types and frequencies of transient events in the centers of post-starburst and quiescent Balmer-strong galaxies, highlighting the dominance of Type Ia supernovae over TDEs and assessing contamination risks in TDE searches.
Contribution
It provides the first detailed comparison of transient types in these specific galaxy classes and quantifies the contamination of TDE searches by Type Ia supernovae.
Findings
TDEs and Type Ia SNe are the main transients in these galaxies.
Type Ia SNe are 8.3 times more common than TDEs in the sample.
Spectroscopically confirmed PS galaxies show TDEs outnumbering SNe 2 to 1.
Abstract
Tidal Disruption Events (TDEs) have been found to show a preference for post-starburst (PS) and quiescent Balmer-strong (QBS) galaxies. This preference can be used to help find TDEs in transient surveys. But what other transients might "contaminate" such a search, and by how much? We examine all reported transients coincident with the centers of galaxies in the French & Zabludoff (2018) catalog of spectroscopically confirmed PS and QBS galaxies and photometrically identified PS and QBS galaxy candidates. We find that TDEs and Type Ia supernovae (SNe) are the only types of transients classified in the centers of these galaxies (aside from one active galactic nucleus flare), with Type Ia SNe being 8.3+-0.2 times more prevalent than TDEs (1-sigma confidence bounds). This factor is ~2.7 times lower than in a control sample of quiescent galaxies. Narrowing the sample to spectroscopically…
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