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dc.contributor.authorSwan, H. F.
dc.contributor.authorQuimby, R. M.
dc.contributor.authorRowell, G.
dc.contributor.authorRujopakarn, W.
dc.contributor.authorSchaefer, B. E.
dc.contributor.authorSmith, D. A.
dc.contributor.authorVestrand, W. T.
dc.contributor.authorGuver, Tolga
dc.contributor.authorYuan, F.
dc.contributor.authorWren, J.
dc.contributor.authorWheeler, J. C.
dc.contributor.authorYost, S. A.
dc.contributor.authorRykoff, E. S.
dc.contributor.authorAharonian, F.
dc.contributor.authorAkerlof, C. W.
dc.contributor.authorAshley, M. C. B.
dc.contributor.authorBarthelmy, S.
dc.contributor.authorGehrels, N.
dc.contributor.authorGogus, E.
dc.contributor.authorHorns, D.
dc.contributor.authorKiziloglu, U.
dc.contributor.authorKrimm, H. A.
dc.contributor.authorMckay, T. A.
dc.contributor.authorMirabal, N.
dc.contributor.authorOzel, M.
dc.contributor.authorPhillips, A.
dc.date.accessioned2021-03-02T23:24:21Z
dc.date.available2021-03-02T23:24:21Z
dc.identifier.citationYost 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.othervv_1032021
dc.identifier.otherav_123619f1-f2e6-4aaa-ba76-15c3e2e78055
dc.identifier.urihttp://hdl.handle.net/20.500.12627/17706
dc.description.abstractWe 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.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.titleROITSE-III performance in the swift era
dc.typeBildiri
dc.contributor.departmentUniversity of Michigan System , ,
dc.identifier.volume836
dc.contributor.firstauthorID720303


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