THE AFTERGLOWS OF<i>SWIFT</i>-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-<i>SWIFT</i>AND<i>SWIFT</i>-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS
Д. А. Канн(Thüringer Landessternwarte Tautenburg), D. Xu(Zhejiang Chinese Medical University)
Cited by 354
Related Papers
A CONTINUUM OF H- TO He-RICH TIDAL DISRUPTION CANDIDATES WITH A PREFERENCE FOR E+A GALAXIES
|The Astrophysical Journal|2014|459
No supernovae associated with two long-duration γ-ray bursts
|Nature|2006|445
SWIFT J2058.4+0516: DISCOVERY OF A POSSIBLE SECOND RELATIVISTIC TIDAL DISRUPTION FLARE?
|The Astrophysical Journal|2012|392
LOW-RESOLUTION SPECTROSCOPY OF GAMMA-RAY BURST OPTICAL AFTERGLOWS: BIASES IN THE <i>SWIFT</i> SAMPLE AND CHARACTERIZATION OF THE ABSORBERS
|The Astrophysical Journal Supplement Series|2009|377
PTF 11kx: A Type Ia Supernova with a Symbiotic Nova Progenitor
|Science|2012|353