activity
20072023
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations · 2.4k across the 25 of their papers we have counts for

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Showing 2014Show all

10 papers · 1 filter

astro-ph.HE2014105 cited

Circular polarization in the optical afterglow of GRB 121024A

K. Wiersema, S. Covino, K. Toma +37

Gamma-ray bursts (GRBs) are most probably powered by collimated relativistic outflows (jets) from accreting black holes at cosmological distances. Bright afterglows are produced wh…

astro-ph.GA201455 cited

The mysterious optical afterglow spectrum of GRB140506A at z=0.889

J. P. U. Fynbo, T. Krühler, K. Leighly +40

Context. Gamma-ray burst (GRBs) afterglows probe sightlines to star-forming regions in distant star-forming galaxies. Here we present a study of the peculiar afterglow spectrum of…

astro-ph.GA201417 cited

Discovery of Dramatic Optical Variability in SDSS J1100+4421: A Peculiar Radio-Loud Narrow-Line Seyfert 1 Galaxy?

Masaomi Tanaka, Tomoki Morokuma, Ryosuke Itoh +55

We present our discovery of dramatic variability in SDSS J1100+4421 by the high-cadence transient survey Kiso Supernova Survey (KISS). The source brightened in the optical by at le…

astro-ph.SR201442 cited

Kiso Supernova Survey (KISS): Survey Strategy

Tomoki Morokuma, Nozomu Tominaga, Masaomi Tanaka +58

The Kiso Supernova Survey (KISS) is a high-cadence optical wide-field supernova (SN) survey. The primary goal of the survey is to catch the very early light of a SN, during the sho…

astro-ph.SR201456 cited

Abundance stratification in Type Ia Supernovae - IV: the luminous, peculiar SN 1991T

Michele Sasdelli, Paolo A. Mazzali, Elena Pian +4

The abundance distribution of the elements in the ejecta of the peculiar, luminous Type Ia supernova (SN Ia) 1991T is obtained modelling spectra from before maximum light until a y…

astro-ph.HE201426 cited

A quiescent galaxy at the position of the long GRB 050219A

A. Rossi, S. Piranomonte, S. Savaglio +25

Long-duration gamma-ray bursts (LGRBs) are produced by the collapse of very massive stars. Due to the short lifetime of their progenitors, LGRBs pinpoint star-forming galaxies. We…