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Rapid optical follow-up observations of SGR events with ROTSE-I

dc.contributor.authorBalsano, RIchard Jen_US
dc.contributor.authorAkerlof, Carl W.en_US
dc.contributor.authorBarthelmy, Scotten_US
dc.contributor.authorBloch, J.en_US
dc.contributor.authorButterworth, Paulen_US
dc.contributor.authorCasperson, Donald E.en_US
dc.contributor.authorCline, T.en_US
dc.contributor.authorFletcher, S.en_US
dc.contributor.authorGisler, Galen R.en_US
dc.contributor.authorHills, Jack G.en_US
dc.contributor.authorKehoe, Robert L.en_US
dc.contributor.authorLee, Brian C.en_US
dc.contributor.authorMarshall, Stuart L.en_US
dc.contributor.authorMcKay, Timothy A.en_US
dc.contributor.authorPawl, Andrewen_US
dc.contributor.authorPriedhorsky, William C.en_US
dc.contributor.authorSeldomridge, N.en_US
dc.contributor.authorSzymanski, John J.en_US
dc.contributor.authorWren, James A.en_US
dc.date.accessioned2011-11-15T16:01:11Z
dc.date.available2011-11-15T16:01:11Z
dc.date.issued2000-09-08en_US
dc.identifier.citationBalsano, R.; Akerlof, C.; Barthelmy, S.; Bloch, J.; Butterworth, P.; Casperson, D.; Cline, T.; Fletcher, S.; Gisler, G.; Hills, J.; Kehoe, R.; Lee, B.; Marshall, S.; McKay, T.; Pawl, A.; Priedhorsky, W.; Seldomridge, N.; Szymanski, J.; Wren, J. (2000). "Rapid optical follow-up observations of SGR events with ROTSE-I." AIP Conference Proceedings 526(1): 804-808. <http://hdl.handle.net/2027.42/87446>en_US
dc.identifier.otherAPCPCS-526-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87446
dc.description.abstractThe primary mission of the Robotic Optical Transient Search Experiment (ROTSE) is to search for contemporaneous optical emission from GRBs. Among the triggers ROTSE receives via the GRB Coordinates Network (GCN), there are a number from Soft-Gamma Repeater (SGR) events. Since beginning operations in March 1998, ROTSE-I has triggered on 16 observable SGR events. Ten of these events had useful data, eight events from SGR 1900+14SGR1900+14 and two events from SGR 1806−20.SGR1806−20. The error regions for these SGRs are a small fraction of the ROTSE 16°×16°16°×16° field of view and have been searched for new or variable objects. Limits on optical transient counterparts are in the range mROTSE ≈ 12.5–15.5mROTSE≈12.5–15.5 during the period 10 seconds to 1 hour after the observed SGR events. © 2000 American Institute of Physics.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleRapid optical follow-up observations of SGR events with ROTSE-Ien_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87446/2/804_1.pdf
dc.identifier.doi10.1063/1.1361645en_US
dc.identifier.sourceGAMMA-RAY BURSTS: 5th Huntsville Symposiumen_US
dc.owningcollnamePhysics, Department of


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