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Rapid searches for counterparts of GRB 930131

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dc.contributor.author Schaefer, Bradley. E
dc.contributor.author Barthelmy, Scott. D
dc.contributor.author Palmer, David. M
dc.contributor.author Cline, Thomas. L
dc.contributor.author Hurley, Kevin. C
dc.contributor.author Sommer, Michael
dc.contributor.author Boer, Michel
dc.contributor.author Niel, Michel
dc.contributor.author Fishman, Gerald. J
dc.contributor.author Kouveliotou, Chryssa
dc.contributor.author Meegan, Charles. A
dc.contributor.author Coe, M. J
dc.contributor.author Elmegreen, Bruce. G
dc.contributor.author McNamara, Bernard. J
dc.contributor.author Harrison, Thomas
dc.contributor.author Owens, Alan
dc.contributor.author Sollee, Neyle
dc.contributor.author Stull, John
dc.contributor.author Palermiti, Michael
dc.contributor.author Schwartz, Richard
dc.contributor.author Brooks, Jack
dc.contributor.author Vanderspek, Roland
dc.contributor.author Ricker, George. R
dc.contributor.author Krimm, Hans. A
dc.contributor.author Wenzel, Wolfgang
dc.contributor.author Greiner, Jochen
dc.contributor.author Hudec, Rene
dc.contributor.author Novak, Miroslav
dc.contributor.author Borovicka, Jiri
dc.contributor.author Predota, Miroslav
dc.contributor.author Bailyn, Charles. D
dc.contributor.author Hanlon, Lorraine. O
dc.contributor.author Bennett, K
dc.contributor.author Spoelstra, Titus. A. Th
dc.contributor.author Smette, Alain
dc.contributor.author Pedersen, Holger
dc.contributor.author Florentin, Ralph
dc.contributor.author Pollas, Christian
dc.contributor.author Steinle, Helmut
dc.contributor.author Schramm, K. J
dc.contributor.author Iyengar, K. V. K
dc.contributor.author Prabhu, T. P
dc.date.accessioned 2008-07-14T08:56:21Z
dc.date.available 2008-07-14T08:56:21Z
dc.date.issued 1994-02
dc.identifier.citation Astrophysical Journal Part 2 - Letters, Vol. 422, No. 2, pp. L71 - L74 en
dc.identifier.issn 0004-637X
dc.identifier.uri http://hdl.handle.net/2248/2670
dc.description.abstract A fading counterpart to a gamma-ray burst (GRB) would appear as a point source inside a GRB error region soon after the burst which dims on a timescale from minutes to days. The favorable circumstances of the burst GRB 930131 allowed for an international campaign to search for fading counterparts starting 6.8 hr after the burst. We report observations from many optical sites, two radio telescopes, and archival ROSAT data, including deep Schmidt exposures 35, 44, and 64 hr after the burst. No fading counterparts were detected with our observations. en
dc.format.extent 792105 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher American Astronomical Society en
dc.relation.uri http://adsabs.harvard.edu/abs/1994ApJ...422L..71S en
dc.subject Gamma Ray Bursts en
dc.subject Point Sources en
dc.subject Sky Surveys (Astronomy) en
dc.subject Wave Attenuation en
dc.subject Annihilation Reactions en
dc.subject Error Analysis en
dc.subject Pair Production en
dc.subject Radio Telescopes en
dc.title Rapid searches for counterparts of GRB 930131 en
dc.type Article en


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