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Related papers: The Host Galaxies of Rapidly Evolving Transients i…

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We present a comprehensive analysis of the host galaxies of 11 luminous fast blue optical transients (LFBOTs). We model new and archival host photometry and spectroscopy with Prospector. We determine that all LFBOT hosts are actively…

High Energy Astrophysical Phenomena · Physics 2026-03-26 Anya E. Nugent , V. Ashley Villar , Brian D. Metzger , Christopher L. Fryer , Eric Burns , Alexa Gordon , Danielle Frostig

We present the results of a search for rapidly evolving transients in the Dark Energy Survey Supernova Programme. These events are characterized by fast light curve evolution (rise to peak in $\lesssim 10$ d and exponential decline in…

Rapidly evolving transients form a new class of transients which show shorter timescales of the light curves than those of typical core-collapse and thermonuclear supernovae. We performed a systematic search for rapidly evolving transients…

We search the archival Zwicky Transient Facility public survey for rapidly evolving transient (RET) candidates based on well-defined criteria between 2018 May and 2021 December. The search yielded 19 bona-fide RET candidates, corresponding…

High Energy Astrophysical Phenomena · Physics 2023-05-23 Wenxiong Li , Iair Arcavi , Ehud Nakar , Alexei V. Filippenko , Thomas G. Brink , WeiKang Zheng , Marco C. Lam , Ido Keinan , Seán J. Brennan , Noi Shitrit

Fast radio bursts (FRBs) are millisecond-duration extragalactic radio transients of unknown origin, and studying their host galaxies could offer clues to constrain progenitor models. Among host properties, gas-phase metallicity is a key…

High Energy Astrophysical Phenomena · Physics 2025-12-11 Shotaro Yamasaki , Tetsuya Hashimoto , Haruka Kusakabe , Tomotsugu Goto

Extragalactic fast X-ray transients (FXTs) are a class of soft (0.3-10 keV) X-ray transients lasting a few hundred seconds to several hours. Several progenitor mechanisms have been suggested to produce FXTs, including supernova shock…

In the past decade, several rapidly-evolving transients have been discovered whose timescales and luminosities are not easily explained by traditional supernovae (SN) models. The sample size of these objects has remained small due, at least…

Luminous Fast Blue Optical Transients (LFBOTs) are a class of extragalactic transients notable for their rapid rise and fade times, blue colour and accompanying luminous X-ray and radio emission. Only a handful have been studied in detail…

High Energy Astrophysical Phenomena · Physics 2024-12-04 A. A. Chrimes , D. L. Coppejans , P. G. Jonker , A. J. Levan , P. J. Groot , A. Mummery , E. R. Stanway

We develop a new statistical framework for studying the host galaxies of astrophysical sources that accounts for both redshift evolution and the multi-variate nature of host-galaxy properties. These aspects are critical when dealing with…

High Energy Astrophysical Phenomena · Physics 2025-11-14 Asaf Horowicz , Ben Margalit

We report on a search for host galaxies of a subset of Rotating Radio Transients (RRATs) that possess a dispersion measure (DM) near or above the maximum Galactic value in their direction. These RRATs could have an extragalactic origin and…

High Energy Astrophysical Phenomena · Physics 2017-01-24 Akshaya Rane , Abraham Loeb

This theoretical work investigates different models to predict the redshift of Fast Radio Bursts (FRBs) from their observed dispersion measure (DM) and other reported properties. We performed an extensive revision of the FRBs with confirmed…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-13 Luz Ángela García , Eduard Piratova-Moreno , Felipe González-Alarcón , Jhonier Rangel

The Large Synoptic Survey Telescope (LSST) will open a discovery frontier for faint and fast transients with its ability to detect variable flux components down to $\sim$24.5 mag in a $\sim$30 second exposure. Spectroscopic follow-up of…

Long gamma-ray bursts (LGRBs) and superluminous supernovae (SLSNe) are both explosive transients with very massive progenitor stars. Clues about the nature of the progenitors can be found by investigating environments in which such…

High Energy Astrophysical Phenomena · Physics 2016-10-05 J. Japelj , S. D. Vergani , R. Salvaterra , L. K. Hunt , F. Mannucci

We present the first data release (DR1) of the Spectroscopic Classification of Astronomical Transients (SCAT) survey, covering the first $\approx 5$ years of observations (March 2018 - January 2023). DR1 includes 1810 spectra of 1330…

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