We present observations of the optically dark burst GRB 060108, the 100th Swift burst. We find that the most likely explanation for the observed darkness is a combination of intrinsic faintness, a hard optical to X-ray spectrum and dust extinction
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Abstract. Dark gamma-ray bursts (GRBs) are sources with a low optical-to-X-ray flux ratio. Proposed ...
[出版社版]Observations were made of the optical afterglow of GRB 051028 with the Lulin observatory 1.0 m...
We present a multiwavelength study of GRB 060108 - the 100th gamma-ray burst discovered by Swift. Th...
We present a multiwavelength study of GRB 060108 – the 100th gamma-ray burst discovered by Swift. Th...
GRB 090417B was an unusually long burst with a T(90) duration of at least 2130 s and a multi-peaked ...
GRB 090417B was an unusually long burst with a T(90) duration of at least 2130 s and a multi-peaked ...
Context. Dark gamma-ray bursts (GRBs) are sources with no or faint optical/near infrared (NIR) after...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
5 pages, 7 figures. Accepted in Astronomy and AstrophysicsWe present multiwavelength observations of...
We report the first detection of an optical afterglow of a GRB (060108) that would have been classif...
5 pages, 7 figures. Accepted in Astronomy and AstrophysicsWe present multiwavelength observations of...
We present Swift and XMM observations of GRB 050326, detected by Swift-BAT. The fluence was 7.7x10^-...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Abstract. Dark gamma-ray bursts (GRBs) are sources with a low optical-to-X-ray flux ratio. Proposed ...
[出版社版]Observations were made of the optical afterglow of GRB 051028 with the Lulin observatory 1.0 m...
We present a multiwavelength study of GRB 060108 - the 100th gamma-ray burst discovered by Swift. Th...
We present a multiwavelength study of GRB 060108 – the 100th gamma-ray burst discovered by Swift. Th...
GRB 090417B was an unusually long burst with a T(90) duration of at least 2130 s and a multi-peaked ...
GRB 090417B was an unusually long burst with a T(90) duration of at least 2130 s and a multi-peaked ...
Context. Dark gamma-ray bursts (GRBs) are sources with no or faint optical/near infrared (NIR) after...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
5 pages, 7 figures. Accepted in Astronomy and AstrophysicsWe present multiwavelength observations of...
We report the first detection of an optical afterglow of a GRB (060108) that would have been classif...
5 pages, 7 figures. Accepted in Astronomy and AstrophysicsWe present multiwavelength observations of...
We present Swift and XMM observations of GRB 050326, detected by Swift-BAT. The fluence was 7.7x10^-...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very...
Abstract. Dark gamma-ray bursts (GRBs) are sources with a low optical-to-X-ray flux ratio. Proposed ...
[出版社版]Observations were made of the optical afterglow of GRB 051028 with the Lulin observatory 1.0 m...