activity
20082024
most citedSOUSA: the Swift Optical/Ultraviolet Supernova Archive

257 citations · 1.3k across the 23 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

12 papers · 1 filter

astro-ph.HE2024

Swift-BAT GUANO follow-up of gravitational-wave triggers in the third LIGO-Virgo-KAGRA observing run

Gayathri Raman, Samuele Ronchini, James Delaunay +1819

We present results from a search for X-ray/gamma-ray counterparts of gravitational-wave (GW) candidates from the third observing run (O3) of the LIGO-Virgo-KAGRA (LVK) network usin…

astro-ph.HE2020★ 124 cited

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.HE2018★ 37 cited

Dramatic change in the boundary layer in the symbiotic recurrent nova T Coronae Borealis

G. J. M. Luna, K. Mukai, J. L. Sokoloski +6

A sudden increase in the rate at which material reaches the most internal part of an accretion disk, i.e. the boundary layer, can change its structure dramatically. We have witness…

astro-ph.HE2017★ 7 cited

Colour variations in the GRB 120327A afterglow

A. Melandri, S. Covino, E. Zaninoni +42

We present a comprehensive temporal and spectral analysis of the long Swift GRB 120327A afterglow data to investigate the possible causes of the observed early time colour variatio…

astro-ph.HE2017★ 2 cited

Multiwavelength picture of the blazar S5 0716+714 during its brightest outburst

Marina Manganaro, Giovanna Pedaletti, Marlene Doert +24

S5 0716+714 is a well known BL Lac object, one of the brightest and most active blazars. The discovery in the Very High Energy band (VHE, E > 100 GeV) by MAGIC happened in 2008. In…

astro-ph.HE2014★ 257 cited

SOUSA: the Swift Optical/Ultraviolet Supernova Archive

Peter J. Brown, Alice A. Breeveld, Stephen Holland +2

The Ultra-Violet Optical Telescope on the Swift spacecraft has observed hundreds of supernovae, covering all major types and most subtypes. Here we introduce the Swift Optical/Ultr…

astro-ph.HE2014★ 46 cited

Ultraviolet Observations of Super-Chandrasekhar Mass Type Ia Supernova Candidates with Swift UVOT

Peter J. Brown, Paul Kuin, Richard Scalzo +6

Among Type Ia supernovae (SNe~Ia) exist a class of overluminous objects whose ejecta mass is inferred to be larger than the canonical Chandrasekhar mass. We present and discuss the…

astro-ph.HE2013★ 134 cited

GRB 130427A: a Nearby Ordinary Monster

A. Maselli, A. Melandri, L. Nava +63

Long-duration Gamma-Ray Bursts (GRBs) are an extremely rare outcome of the collapse of massive stars, and are typically found in the distant Universe. Because of its intrinsic lumi…

astro-ph.HE2013★ 253 cited

A panchromatic view of the restless SN2009ip reveals the explosive ejection of a massive star envelope

R. Margutti, D. Milisavljevic, A. M. Soderberg +54

The 2012 explosion of SN2009ip raises questions about our understanding of the late stages of massive star evolution. Here we present a comprehensive study of SN2009ip during its r…

astro-ph.HE2013★ 13 cited

G306.3-0.9: A newly discovered young galactic supernova remnant

Mark Reynolds, Shyeh Loi, Tara Murphy +14

We present X-ray and radio observations of the new Galactic supernova remnant (SNR) G306.3-0.9, recently discovered by Swift. Chandra imaging reveals a complex morphology, dominate…

astro-ph.HE2012★ 37 cited

The Long-Lived UV "Plateau" of SN 2012aw

Amanda J. Bayless, Tyler Pritchard, Peter W. A. Roming +9

Observations with the Swift UVOT have unambiguously uncovered for the first time a long-lived, UV "plateau" in a Type II-P supernova (SN). Although this flattening in slope is hint…

astro-ph.HE2011★ 49 cited

Panchromatic observations of the textbook GRB 110205A: constraining physical mechanisms of prompt emission and afterglow

W. Zheng, R. F. Shen, T. Sakamoto +56

We present a comprehensive analysis of a bright, long duration (T90 ~ 257 s) GRB 110205A at redshift z= 2.22. The optical prompt emission was detected by Swift/UVOT, ROTSE-IIIb and…