1. Adelaide Research & Scholarship
  2. Schools and Disciplines
  3. School of Chemistry and Physics
  4. Chemistry and Physics publications
Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/44549
Citations
Scopus Web of Science® Altmetric
?
?
Full metadata record
DC FieldValueLanguage
dc.contributor.authorYost, S.-
dc.contributor.authorAharonian, F.-
dc.contributor.authorAkerlof, C.-
dc.contributor.authorAshley, M.-
dc.contributor.authorBarthelmy, S.-
dc.contributor.authorGehrels, N.-
dc.contributor.authorGogus, E.-
dc.contributor.authorGuver, T.-
dc.contributor.authorHorns, D.-
dc.contributor.authorKiziloglu, U.-
dc.contributor.authorKrimm, H.-
dc.contributor.authorMcKay, T.-
dc.contributor.authorOzel, M.-
dc.contributor.authorPhillips, A.-
dc.contributor.authorQuimby, R.-
dc.contributor.authorRowell, G.-
dc.contributor.authorRujopakarn, W.-
dc.contributor.authorRykoff, E.-
dc.contributor.authorSchaefer, B.-
dc.contributor.authorSmith, D.-
dc.contributor.authoret al.-
dc.date.issued2007-
dc.identifier.citationThe Astrophysical Journal: an international review of astronomy and astronomical physics, 2007; 669(2 Part 1):1107-1114-
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357-
dc.identifier.urihttp://hdl.handle.net/2440/44549-
dc.descriptionSubmitted to Cornell University's online archive www.arXiv.org in 2007 by Sarah A. Yost.-
dc.description.abstractWe present several cases of optical observations during γ-ray bursts (GRBs) which resulted in prompt limits but no detection of optical emission. These limits constrain the prompt optical flux densities and the optical brightness relative to the γ-ray emission. The derived constraints fall within the range of properties observed in GRBs with prompt optical detections, although at the faint end of optical/γ-ray flux ratios. The currently accessible prompt optical limits do not require a different set of intrinsic or environmental GRB properties, relative to the events with prompt optical detections.-
dc.description.statementofresponsibilityS. A. Yost, F. Aharonian, C. W. Akerlof, M. C. B. Ashley, S. Barthelmy, N. Gehrels, E. Göğüş, T. Güver, D. Horns, Ü. Kızılolu, H. A. Krimm, T. A. McKay, M. Özel, A. Phillips, R. M. Quimby, G. Rowell, W. Rujopakarn, E. S. Rykoff, B. E. Schaefer, D. A. Smith, H. F. Swan, W. T. Vestrand, J. C. Wheeler, J. Wren and F. Yuan-
dc.language.isoen-
dc.publisherUniv Chicago Press-
dc.rightsCopyright © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.-
dc.source.urihttp://dx.doi.org/10.1086/521668-
dc.subjectAstrophysics (astro-ph)-
dc.titleThe dark side of ROTSE-III prompt GRB observations-
dc.typeJournal article-
dc.identifier.doi10.1086/521668-
pubs.publication-statusPublished-
dc.identifier.orcidRowell, G. [0000-0002-9516-1581]-
Appears in Collections:Aurora harvest 6
Chemistry and Physics publications

Files in This Item:
There are no files associated with this item.
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.