Super-LOTIS: A High-Sensitive Optical Counterpart Search Experiment
| dc.creator | Park, H. S. | |
| dc.creator | Ables, E. | |
| dc.creator | Band, D. L. | |
| dc.creator | Barthelmy, S. D. | |
| dc.creator | Bionta, R. M. | |
| dc.creator | Butterworth, P. S. | |
| dc.creator | Cline, T. L. | |
| dc.creator | Ferguson, D. H. | |
| dc.creator | Fishman, G. J. | |
| dc.creator | Gehrels, N. | |
| dc.creator | Hartmann, D. | |
| dc.creator | Hurley, K. | |
| dc.creator | Kouveliotou, C. | |
| dc.creator | Meegan, C. A. | |
| dc.creator | Ott, L. | |
| dc.creator | Parker, E. | |
| dc.creator | Williams, G. G. | |
| dc.date | 1997-11-14 | |
| dc.date.accessioned | 2026-07-07T02:25:06Z | |
| dc.date.available | 2026-07-07T02:25:06Z | |
| dc.description | We are constructing a 0.6 meter telescope system to search for early time gamma-ray burst(GRB) optical counterparts. Super-LOTIS (Super-Livermore Optical Transient Imaging System) is an automated telescope system that has a 0.8 x 0.8 deg field-of-view, is sensitive to Mv ~ 19 and responds to a burst trigger within 5 min. This telescope will record images of the gamma-ray burst coordinates that is given by the GCN (GRB Coordinate Network). A measurement of GRB light curves at early times will greatly enhance our understanding of GRB physics. | |
| dc.description | LaTeX, 4 pages, 2 figures, requires aipproc.sty and epsfig.sty, To appear in the Proceedings of the 4th Huntsville Gamma-Ray Burst Symposium | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9711170 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9711170 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11805 | |
| dc.subject | Astrophysics | |
| dc.title | Super-LOTIS: A High-Sensitive Optical Counterpart Search Experiment | |
| dc.type | text |