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The CFHTLS Real Time Analysis System "Optically Selected GRB Afterglows"
Malacrino F., Atteia J.-L., Boer M., Klotz A., Veillet C., Cuillandre J.-C.
Astronomy and Astrophysics 459 (2006) 465-475 - http://hal.archives-ouvertes.fr/hal-00077592
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Article in peer-reviewed journal
Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics
Sciences of the Universe/Astrophysics
The CFHTLS Real Time Analysis System "Optically Selected GRB Afterglows"
Frederic Malacrino () 1, Jean-Luc Atteia 1, Michel Boer 2, Alain Klotz 3, Christian Veillet 4, Jean-Charles Cuillandre 4
1:  Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT)
http://webast.ast.obs-mip.fr
CNRS : UMR5572 – INSU – Observatoire Midi-Pyrénées – Université Paul Sabatier [UPS] - Toulouse III
14, avenue Edouard Belin 31400 Toulouse
France
2:  Observatoire de Haute-Provence (OHP)
http://www.obs-hp.fr
CNRS : USR2207 – INSU – Université de Provence - Aix-Marseille I
04870 ST MICHEL L OBSERVATOIRE
France
3:  Centre d'étude spatiale des rayonnements (CESR)
http://www.cesr.fr
CNRS : UMR5187 – Observatoire Midi-Pyrénées – INSU – Université Paul Sabatier [UPS] - Toulouse III
9 Av du colonel Roche - BP 4346 31028 TOULOUSE CEDEX 4
France
4:  Canada-France-Hawaii Telescope (CFHT)
CFHT
United States
We describe a wide and deep search for optical GRB afterglows on images taken with MegaCAM at the Canada France Hawaii Telescope, within the framework of the CFHT Legacy Survey. This search is performed in near real-time thanks to a Real Time Analysis System called "Optically Selected GRB Afterglows", which has been completely realized and installed on a dedicated computer in Hawaii. This pipeline automatically and quickly analyzes Megacam images and extracts from them a list of astrometrically and photometrically variable objects which are displayed on a web page for validation by a member of the collaboration. In this paper, we comprehensively describe the RTAS process. We also present statistical results based on nearly one full year of operation, showing the quality of the images and the performance of the RTAS. Finally, we compare the efficiency of this study with similar searches, propose an ideal observational strategy using simulations, and discuss general considerations on the searches for GRB afterglows independently of the prompt emission. This is the first of a series of two papers. A second paper will discuss the characterization of variable objects we have found, as well as the GRB afterglow candidates and their nature. We will also estimate or at least constrain the collimation factor of GRB using the totality of the Very Wide Survey observations.
English

Astronomy and Astrophysics (Astron. Astrophys.)
Publisher EDP Sciences
ISSN 0004-6361 (eISSN : 1432-0756)
international
2006-11-01
459
465-475

Gamma rays: bursts – Methods: data analysis – Techniques: image processing
11 pages, 10 Figures, 5 Tables

GRB RTAS
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