Published October 22, 2008
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The Robotic Palomar 60-Inch Optical Afterglow Catalog: 2007
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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.
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© 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
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KELaipcp08.pdf
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- Eprint ID
- 12282
- Resolver ID
- CaltechAUTHORS:KELaipcp08
Funding
- Hungarian Space Office
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- Created
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2008-11-03Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
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- Series Name
- American Institute of Physics Conference Proceedings
- Series Volume or Issue Number
- 1065