| タイトル | Gamma Ray Burst Optical Counterpart Search Experiment (GROCSE) |
| 著者（英） | Wallace, S.; Akerlof, C.; Parker, E.; Lee, B.; Barthelmy, S.; Ott, L.; Butterworth, P.; Ables, E.; Park, H. S.; Bionta, R. M. |
| 著者所属（英） | Lawrence Livermore National Lab. |
| 発行日 | 1995-10-27 |
| 言語 | eng |
| 内容記述 | GROCSE (Gamma-Ray Optical Counterpart Search Experiments) is a system of automated telescopes that search for simultaneous optical activity associated with gamma ray bursts in response to real-time burst notifications provided by the BATSE/BACODINE network. The first generation system, GROCSE 1, is sensitive down to Mv (approximately) 8.5 and requires an average of 12 seconds to obtain the first images of the gamma ray burst error box defined by the BACODINE trigger. The collaboration is now constructing a second generation system which has a 4 second slewing time and can reach Mv (approximately) 14 with a 5 second exposure. GROCSE 2 consists of 4 cameras on a single mount. Each camera views the night sky through a commercial Canon lens (f/1.8, focal length 200 mm) and utilizes a 2K x 2K Loral CCD. Light weight and low noise custom readout electronics were designed and fabricated for these CCDs. The total field of view of the 4 cameras is 17.6 x 17.6 (degree). GROCSE 2 will be operated by the end of 1995. In this paper, the authors present an overview of the GROCSE system and the results of measurements with a GROCSE 2 prototype unit. |
| NASA分類 | Space Radiation |
| レポートNO | 96N30930
UCRL-JC-123539
CONF-9510332-6
DE96-009810 |
| 権利 | No Copyright |
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