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20092026
most citedA Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies

466 citations · 4.4k across the 61 of their papers we have counts for

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17 papers · 1 filter

astro-ph.HE2024★ 1 cited

Rapid Response Mode observations of GRB 160203A: Looking for fine-structure line variability at z=3.52

G. Pugliese, A. Saccardi, V. D Elia +26

Gamma-ray bursts are the most energetic known explosions. Despite fading rapidly, they allow to measure redshift and important properties of their host-galaxies. We report the phot…

astro-ph.HE2023★ 1 cited

Resolving the explosion of supernova 2023ixf in Messier 101 within its complex circumstellar environment

E. A. Zimmerman, I. Irani, P. Chen +54

Observing a supernova explosion shortly after it occurs can reveal important information about the physics of stellar explosions and the nature of the progenitor stars of supernova…

astro-ph.HE2018★ 2 cited

A UV Resonance Line Echo from a Shell Around a Hydrogen-Poor Superluminous Supernova

R. Lunnan, C. Fransson, P. M. Vreeswijk +21

Hydrogen-poor superluminous supernovae (SLSN-I) are a class of rare and energetic explosions discovered in untargeted transient surveys in the past decade. The progenitor stars and…

astro-ph.HE2018★ 140 cited

Spectra of Hydrogen-Poor Superluminous Supernovae from the Palomar Transient Factory

Robert M. Quimby, Annalisa De Cia, Avishay Gal-Yam +20

Most Type I superluminous supernovae (SLSNe-I) reported to date have been identified by their high peak luminosities and spectra lacking obvious signs of hydrogen. We demonstrate t…

astro-ph.HE2017★ 32 cited

Far-UV HST Spectroscopy of An Unusual Hydrogen Poor Superluminous Supernova: SN2017egm

Lin Yan, D. A. Perley, A. De Cia +4

SN2017egm is the closest (z=0.03) H-poor superluminous supernova (SLSN-I) detected to date, and a rare example of an SLSN-I in a massive and metal-rich galaxy. Here we present the…

astro-ph.HE2017★ 144 cited

Light curves of hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory

Annalisa De Cia, A. Gal-Yam, A. Rubin +24

We investigate the light-curve properties of a sample of 26 spectroscopically confirmed hydrogen-poor superluminous supernovae (SLSNe-I) in the Palomar Transient Factory (PTF) surv…

astro-ph.HE2017★ 114 cited

Hydrogen-poor Superluminous Supernovae With Late-time H-alpha Emission: Three Events From the Intermediate Palomar Transient Factory

Lin Yan, R. Lunnan, D. Perley +20

We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H-alpha emission with line luminosities of (1-3)e+41…

astro-ph.HE2016★ 78 cited

On the early-time excess emission in hydrogen-poor superluminous supernovae

Paul M. Vreeswijk, Giorgos Leloudas, Avishay Gal-Yam +27

We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient Factory. Both show ex…

astro-ph.HE2016★ 237 cited

The Superluminous Transient ASASSN-15lh as a Tidal Disruption Event from a Kerr Black Hole

G. Leloudas, M. Fraser, N. C. Stone +47

When a star passes within the tidal radius of a supermassive black hole, it will be torn apart. For a star with the mass of the Sun () and a non-spinning black hole with a…

astro-ph.HE2016★ 208 cited

Host-Galaxy Properties of 32 Low-Redshift Superluminous Supernovae from the Palomar Transient Factory

Daniel A. Perley, Robert Quimby, Lin Yan +9

We present ultraviolet through near-infrared photometry and spectroscopy of the host galaxies of all superluminous supernovae (SLSNe) discovered by the Palomar Transient Factory pr…

astro-ph.HE2015★ 94 cited

Type II supernova energetics and comparison of light curves to shock-cooling models

Adam Rubin, Avishay Gal-Yam, Annalisa De Cia +37

During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding early-time SN light curves in the…

astro-ph.HE2015★ 58 cited

Optical and near-infrared observations of SN 2013dx associated with GRB 130702A

V. L. Toy, S. B. Cenko, J. M. Silverman +33

We present optical and near-infrared light curves and optical spectra of SN 2013dx, associated with the nearby (redshift 0.145) gamma-ray burst GRB 130702A. The prompt isotropic ga…

astro-ph.HE2014★ 113 cited

The hydrogen-poor superluminous supernova iPTF13ajg and its host galaxy in absorption and emission

Paul M. Vreeswijk, Sandra Savaglio, Avishay Gal-Yam +24

We present imaging and spectroscopy of a hydrogen-poor superluminous supernova (SLSN) discovered by the intermediate Palomar Transient Factory: iPTF13ajg. At a redshift of z=0.7403…

astro-ph.HE2014★ 364 cited

A Wolf-Rayet-like progenitor of supernova SN 2013cu from spectral observations of a wind

Avishay Gal-Yam, I. Arcavi, E. O. Ofek +17

The explosive fate of massive stripped Wolf-Rayet (W-R) stars is a key open question in stellar physics. An appealing option is that hydrogen-deficient W-R stars are the progenitor…

astro-ph.HE2014★ 466 cited

A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies

Iair Arcavi, Avishay Gal-Yam, Mark Sullivan +23

We present the results of a Palomar Transient Factory (PTF) archival search for blue transients which lie in the magnitude range between "normal" core-collapse and superluminous su…

astro-ph.HE2014★ 79 cited

Interaction-powered supernovae: Rise-time vs. peak-luminosity correlation and the shock-breakout velocity

E. O. Ofek, I. Arcavi, D. Tal +16

Interaction of supernova (SN) ejecta with the optically thick circumstellar medium (CSM) of a progenitor star can result in a bright, long-lived shock breakout event. Candidates fo…

astro-ph.HE2014★ 131 cited

GRB 120422A/SN 2012bz: Bridging the Gap between Low- And High-Luminosity GRBs

S. Schulze, D. Malesani, A. Cucchiara +62

At low redshift, a handful of gamma-ray bursts (GRBs) have been discovered with peak luminosities () substantially lower than the average…