X/gamma-ray measurements of the faint GRB 020321

Details X/gamma-ray measurements of the faint GRB 020321 X/gamma-ray measurements of the faint GRB 020321

2003-05-20

arxiv.org/abs/astro-ph/0305359v1

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures, to be published in Proc. "GRBs in the afterglow era: 3rd Rome workshop (2002)", eds. L. Piro, F. Frontera,

Scientific paper

GRB 020321 is a faint GRB that received wide follow-up attention in X-rays (BeppoSAX/NFI, Chandra/ACIS-S, XMM-Newton), radio (ATCA) and optical (ESO, HST). We identify a weak X-ray afterglow by a combined study of the Chandra and XMM-Newton observations. Its decay index of 1.2 is typical for GRB afterglows. Inside the 4"-accurate error box there is a weak optical counterpart candidate with a much shallower decay index.

Affiliated with

Also associated with

No associations

Rating

X/gamma-ray measurements of the faint GRB 020321 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with X/gamma-ray measurements of the faint GRB 020321, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X/gamma-ray measurements of the faint GRB 020321 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-547455