GRBs Optical follow - up observation at Lulin observatory , Taiwan ( ∗ )
نویسندگان
چکیده
— The Lulin GRB program, using the Lulin One-meter Telescope (LOT) in Taiwan started in July 2003. Its scientific aims are to discover optical counterparts of XRFs and short and long GRBs, then to quickly observe them in multiple bands. Thirteen follow-up observations were provided by LOT between July 2003 and Feb. 2005. One host galaxy was found at GRB 031203. Two optical afterglows were detected for GRB 040924 and GRB 041006. In addition, the optical observations of GRB 031203 and a discussion of the non-detection of the optical afterglow of GRB 031203 are also reported in this article. PACS 95.55.Cs – Ground-based ultraviolet, optical and infrared telescopes. PACS 98.70.Rz – gamma-ray source; gamma-ray bursts. A parallel effort based on the Kiso GRB optical observation system [1, 2], was started in July 2003 using the Lulin One-meter Telescope (LOT) at Taiwan. The scientific aims of our Lulin GRB program are: (1) to discover optical counterparts of XRFs, and short-and long-duration GRBs; (2) to perform multi-band observations that will unlock the temporal and spectral evolution of the corresponding optical afterglows.
منابع مشابه
Kiso Observations of 20 Grbs in the Hete - 2 Era
— We established a GRB follow-up observation system at the Kiso observatory (Japan) in 2001. Since prior to this the east Asian area had been a blank for in GRB follow-up observational network, this observational system is very important for studying the temporal and spectral evolution of early afterglows. We have thus been able to make quick observations of early phase optical afterglows based...
متن کاملGrb Follow - up Observations in the East - Asian Region
— In 2004, we established a Japan-Taiwan-China collaboration for GRB study in the East-Asian region. This serves as a valuable addition to the worldwide optical and infrared follow-up network, because the East-Asia region would otherwise be blank. We have been carrying out imaging and spectroscopic follow-up observations at Lulin (Taiwan), Kiso (Japan), WIDGET (Japan) and Xinglong (China). From...
متن کاملar X iv : a st ro - p h / 05 06 23 2 v 1 1 0 Ju n 20 05 Optical Afterglow Observations of the Unusual Short - Duration Gamma - Ray Burst 040924
The 1-m telescope at Lulin Observatory and the 0.76-m Katzman Automatic Imaging Telescope at Lick Observatory were used to observe the optical afterglow of the short-duration (1.2–1.5 s) gamma-ray burst (GRB) 040924. This object has a soft high-energy spectrum, thus making it an exceptional case, perhaps actually belonging to the short-duration tail of the long-duration GRBs. Our data, combined...
متن کاملPhotometry and imaging of comet C / 2004 Q 2 ( Machholz ) at Lulin and La Silla
Aims. We have investigated the development of the dust and gas coma of the comet C/2004 Q2 (Machholz) from December 2004 to January 2005 using observations obtained at the Lulin Observatory, Taiwan and the European Southern Observatory at La Silla, Chile. Methods. We determined the dust-activity parameter A fρ and the dust color and derived Haser production rates and scale lengths of C2 and NH2...
متن کاملECLAIRs: A microsatellite for the prompt optical and X-ray emission of Gamma-Ray Bursts
The prompt γ-ray emission of Gamma-Ray Bursts (GRBs) is currently interpreted in terms of radiation from electrons accelerated in internal shocks in a relativistic fireball. On the other hand, the origin of the prompt (and early afterglow) optical and X-ray emission is still debated, mostly because very few data exist for comparison with theoretical predictions. It is however commonly agreed th...
متن کامل