collaborators

6 papers

astro-ph.HE2020

The Zwicky Transient Facility Bright Transient Survey. II. A Public Statistical Sample for Exploring Supernova Demographics

Daniel A. Perley, Christoffer Fremling, Jesper Sollerman +34

We present a public catalog of transients from the Zwicky Transient Facility (ZTF) Bright Transient Survey (BTS), a magnitude-limited (m<19 mag in either the g or r filter) survey…

astro-ph.HE2020

Bright, months-long stellar outbursts announce the explosion of interaction-powered supernovae

Nora L. Strotjohann, Eran O. Ofek, Avishay Gal-Yam +53

Interaction-powered supernovae (SNe) explode within an optically-thick circumstellar medium (CSM) that could be ejected during eruptive events. To identify and characterize such pr…

astro-ph.HE2020

An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz

M. Nicholl, T. Wevers, S. R. Oates +42

At 66 Mpc, AT2019qiz is the closest optical tidal disruption event (TDE) to date, with a luminosity intermediate between the bulk of the population and iPTF16fnl. Its proximity all…

astro-ph.HE2020

The Zwicky Transient Facility Census of the Local Universe I: Systematic search for Calcium rich gap transients reveal three related spectroscopic sub-classes

Kishalay De, Mansi M. Kasliwal, Anastasios Tzanidakis +47

(Abridged) Using the Zwicky Transient Facility alert stream, we are conducting a large campaign to spectroscopically classify all transients occurring in galaxies in the Census of…

astro-ph.HE2019

SN 2018fif: The Explosion of a Large Red Supergiant Discovered in Its Infancy by the Zwicky Transient Facility

Maayane T. Soumagnac, Noam Ganot, Ido Irani +32

High cadence transient surveys are able to capture supernovae closer to their first light than before. Applying analytical models to such early emission, we can constrain the proge…

astro-ph.HE2019

SN 2016hil-- a Type II supernova in the remote outskirts of an elliptical host and its origin

Ido Irani, Steve Schulze, Avishay Gal-Yam +14

Type II supernovae (SNe) stem from the core collapse of massive () stars. Owing to their short lifespan, we expect a very low rate of such events in elliptical host…