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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2670
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dc.contributor.authorSchaefer, Bradley. E-
dc.contributor.authorBarthelmy, Scott. D-
dc.contributor.authorPalmer, David. M-
dc.contributor.authorCline, Thomas. L-
dc.contributor.authorHurley, Kevin. C-
dc.contributor.authorSommer, Michael-
dc.contributor.authorBoer, Michel-
dc.contributor.authorNiel, Michel-
dc.contributor.authorFishman, Gerald. J-
dc.contributor.authorKouveliotou, Chryssa-
dc.contributor.authorMeegan, Charles. A-
dc.contributor.authorCoe, M. J-
dc.contributor.authorElmegreen, Bruce. G-
dc.contributor.authorMcNamara, Bernard. J-
dc.contributor.authorHarrison, Thomas-
dc.contributor.authorOwens, Alan-
dc.contributor.authorSollee, Neyle-
dc.contributor.authorStull, John-
dc.contributor.authorPalermiti, Michael-
dc.contributor.authorSchwartz, Richard-
dc.contributor.authorBrooks, Jack-
dc.contributor.authorVanderspek, Roland-
dc.contributor.authorRicker, George. R-
dc.contributor.authorKrimm, Hans. A-
dc.contributor.authorWenzel, Wolfgang-
dc.contributor.authorGreiner, Jochen-
dc.contributor.authorHudec, Rene-
dc.contributor.authorNovak, Miroslav-
dc.contributor.authorBorovicka, Jiri-
dc.contributor.authorPredota, Miroslav-
dc.contributor.authorBailyn, Charles. D-
dc.contributor.authorHanlon, Lorraine. O-
dc.contributor.authorBennett, K-
dc.contributor.authorSpoelstra, Titus. A. Th-
dc.contributor.authorSmette, Alain-
dc.contributor.authorPedersen, Holger-
dc.contributor.authorFlorentin, Ralph-
dc.contributor.authorPollas, Christian-
dc.contributor.authorSteinle, Helmut-
dc.contributor.authorSchramm, K. J-
dc.contributor.authorIyengar, K. V. K-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2008-07-14T08:56:21Z-
dc.date.available2008-07-14T08:56:21Z-
dc.date.issued1994-02-
dc.identifier.citationAstrophysical Journal Part 2 - Letters, Vol. 422, No. 2, pp. L71 - L74en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2670-
dc.description.abstractA 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.extent792105 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1994ApJ...422L..71Sen
dc.subjectGamma Ray Burstsen
dc.subjectPoint Sourcesen
dc.subjectSky Surveys (Astronomy)en
dc.subjectWave Attenuationen
dc.subjectAnnihilation Reactionsen
dc.subjectError Analysisen
dc.subjectPair Productionen
dc.subjectRadio Telescopesen
dc.titleRapid searches for counterparts of GRB 930131en
dc.typeArticleen
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