ROTSE-III performance in the Swift era

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.date.accessioned2025-01-27T18:53:04Z
dc.date.available2025-01-27T18:53:04Z
dc.date.issued2006
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference -- 29 November 2005 through 2 December 2005 -- Washington, D.C. --
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 ?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. © 2006 American Institute of Physics.
dc.identifier.doi10.1063/1.2207919
dc.identifier.endpage352
dc.identifier.isbn0735403260
dc.identifier.isbn978-073540326-0
dc.identifier.issn1551-7616
dc.identifier.scopus2-s2.0-33845596242
dc.identifier.scopusqualityQ4
dc.identifier.startpage349
dc.identifier.urihttps://doi.org/10.1063/1.2207919
dc.identifier.urihttps://hdl.handle.net/20.500.12428/12571
dc.identifier.volume836
dc.indekslendigikaynakScopus
dc.language.isoen
dc.relation.ispartofAIP Conference Proceedings
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_Scopus_20250125
dc.subjectGamma-rays: bursts; Optical instruments
dc.titleROTSE-III performance in the Swift era
dc.typeConference Object

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