Published October 22, 2008 | Version Published
Book Section - Chapter Open

The Robotic Palomar 60-Inch Optical Afterglow Catalog: 2007

Abstract

We present here the photometric results of the Robotic Palomar 60-inch Telescope (P60) observations for GRB optical afterglows. The quick response time and the size of the telescope allows us to observe the optical transients through V, R, I, g', i', z' filters, sometimes as early as 0.01 day after the trigger. Comparing the data obtained with the various filters we were able to compute color indices for the 1 day after the trigger epoch. The observations lasts until the OT fades below the detection threshold.

Additional Information

© 2008 American Institute of Physics. Issue Date: 22 October 2008. This research was partially supported by the Hungarian Space Office (Janos Kelemen).

Attached Files

Published - KELaipcp08.pdf

Files

KELaipcp08.pdf

Files (154.4 kB)

Name Size
md5:27653f21579a33f932b75ac6dc6301aa
154.4 kB Preview Download

Additional details

Identifiers

Eprint ID
12282
Resolver ID
CaltechAUTHORS:KELaipcp08

Funding

Hungarian Space Office

Dates

Created
2008-11-03
Created from EPrint's datestamp field
Updated
2021-11-08
Created from EPrint's last_modified field

Caltech Custom Metadata

Series Name
American Institute of Physics Conference Proceedings
Series Volume or Issue Number
1065