dc.contributor.author | Swan, H. F. | |
dc.contributor.author | Quimby, R. M. | |
dc.contributor.author | Rowell, G. | |
dc.contributor.author | Rujopakarn, W. | |
dc.contributor.author | Schaefer, B. E. | |
dc.contributor.author | Smith, D. A. | |
dc.contributor.author | Vestrand, W. T. | |
dc.contributor.author | Guver, Tolga | |
dc.contributor.author | Yuan, F. | |
dc.contributor.author | Wren, J. | |
dc.contributor.author | Wheeler, J. C. | |
dc.contributor.author | Yost, S. A. | |
dc.contributor.author | Rykoff, E. S. | |
dc.contributor.author | Aharonian, F. | |
dc.contributor.author | Akerlof, C. W. | |
dc.contributor.author | Ashley, M. C. B. | |
dc.contributor.author | Barthelmy, S. | |
dc.contributor.author | Gehrels, N. | |
dc.contributor.author | Gogus, E. | |
dc.contributor.author | Horns, D. | |
dc.contributor.author | Kiziloglu, U. | |
dc.contributor.author | Krimm, H. A. | |
dc.contributor.author | Mckay, T. A. | |
dc.contributor.author | Mirabal, N. | |
dc.contributor.author | Ozel, M. | |
dc.contributor.author | Phillips, A. | |
dc.date.accessioned | 2021-03-02T23:24:21Z | |
dc.date.available | 2021-03-02T23:24:21Z | |
dc.identifier.citation | Yost S. A. , Rykoff E. S. , Aharonian F., Akerlof C. W. , Ashley M. C. B. , Barthelmy S., Gehrels N., Gogus E., Guver T., Horns D., et al., "ROITSE-III performance in the swift era", 16th Annual Astrophysics Conference, Washington, Kiribati, 29 Kasım - 02 Aralık 2005, cilt.836, ss.349-350 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.other | av_123619f1-f2e6-4aaa-ba76-15c3e2e78055 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/17706 | |
dc.description.abstract | We report the successful performance of the Robotic Optical Transient Search Experiment (ROTSE) to promptly-disseminated Swift GRB triggers. ROTSE-III is a worldwide network of 4 unfiltered 0.45m optical telescopes. The telescopes operate robotically, automatically responding to GRB position triggers with a preset observations sequence. Including weather and other downtime, ROTSE-III can immediately respond to similar to 40% of Swift trigger positions, with shutter open within approximately 6-8 seconds from the trigger dissemination. We discuss improvements made possible in the automated response the the small, accurate Swift error boxes. We report ROTSE-III's general results, including OTs discovered or confirmed, the distribution of imaging start times relative to the GRB duration, and an overview of OT lightcurves. | |
dc.language.iso | eng | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | FİZİK, MULTİDİSİPLİNER | |
dc.subject | Fizik | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Temel Bilimler | |
dc.subject | Disiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.subject | Uzay bilimi | |
dc.title | ROITSE-III performance in the swift era | |
dc.type | Bildiri | |
dc.contributor.department | University of Michigan System , , | |
dc.identifier.volume | 836 | |
dc.contributor.firstauthorID | 720303 | |