CaltechAUTHORS
Published April 14, 2003 | Version Published
Book Section - Chapter Open

GRB 000911: Evidence for an Associated Supernova?

Creators

  • 1. ROR icon Brera Astronomical Observatory
  • 2. ROR icon University of Cambridge
  • 3. ROR icon California Institute of Technology
  • 4. ROR icon Arcetri Astrophysical Observatory
  • 5. ROR icon International School for Advanced Studies
  • 6. ROR icon University of Insubria
  • 7. ROR icon Astronomical Observatory of Rome

Contributors

Abstract

We present photometric and spectroscopic observations of the late afterglow of GRB 000911. We detect a moderately significant re-brightening in the R, I and J lightcurves, associated with a sizable reddening of the spectrum. This can be explained through the presence of an underlying supernova, outshining the afterglow ~ 30 days after the burst event.

Additional Information

© 2003 American Institute of Physics. Issue Date: 14 April 2003.

Attached Files

Published - COVaipcp03.pdf

Files

COVaipcp03.pdf

Files (145.0 kB)

Name Size
md5:39f1c00791a6ba97b7e348946f7cd71c
145.0 kB Preview Download

Additional details

Identifiers

Eprint ID
27441
Resolver ID
CaltechAUTHORS:20111026-102659377

Dates

Created
2011-10-26
Created from EPrint's datestamp field
Updated
2021-11-09
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)
Series Name
AIP Conference Proceedings
Series Volume or Issue Number
662