The Dark Side of ROTSE-III Prompt GRB Observations
We present several cases of optical observations during gamma-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 gamma-ray emission. The derived constraints fall w...
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| Veröffentlicht in: | arXiv.org 2007-07 |
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| creator | Yost, S A Aharonian, F Akerlof, C W Ashley, M C B Barthelmy, S Gehrels, N Gogus, E Guver, T Horns, D Kiziloglu, U Krimm, H A McKay, T A Ozel, M Phillips, A Quimby, R M Rowell, G Rujopakarn, W Rykoff, E S Schaefer, B E Smith, D A Swan, H F Vestrand, W T Wheeler, J C Wren, J Yuan, F |
| description | We present several cases of optical observations during gamma-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 gamma-ray emission. The derived constraints fall within the range of properties observed in GRBs with prompt optical detections, though at the faint end of optical/gamma flux ratios. The presently accessible prompt optical limits do not require a different set of intrinsic or environmental GRB properties, relative to the events with prompt optical detections. |
| doi_str_mv | 10.48550/arxiv.0707.3132 |
| format | Article |
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These limits constrain the prompt optical flux densities and the optical brightness relative to the gamma-ray emission. The derived constraints fall within the range of properties observed in GRBs with prompt optical detections, though at the faint end of optical/gamma flux ratios. The presently accessible prompt optical limits do not require a different set of intrinsic or environmental GRB properties, relative to the events with prompt optical detections.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0707.3132</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Emissions control ; Gamma ray bursts ; Gamma rays ; Optical properties ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><ispartof>arXiv.org, 2007-07</ispartof><rights>Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the associated terms available at http://arxiv.org/abs/0707.3132.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,777,781,882,27906</link.rule.ids><backlink>$$Uhttps://doi.org/10.1086/521668$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.0707.3132$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Yost, S A</creatorcontrib><creatorcontrib>Aharonian, F</creatorcontrib><creatorcontrib>Akerlof, C W</creatorcontrib><creatorcontrib>Ashley, M C B</creatorcontrib><creatorcontrib>Barthelmy, S</creatorcontrib><creatorcontrib>Gehrels, N</creatorcontrib><creatorcontrib>Gogus, E</creatorcontrib><creatorcontrib>Guver, T</creatorcontrib><creatorcontrib>Horns, D</creatorcontrib><creatorcontrib>Kiziloglu, U</creatorcontrib><creatorcontrib>Krimm, H A</creatorcontrib><creatorcontrib>McKay, T A</creatorcontrib><creatorcontrib>Ozel, M</creatorcontrib><creatorcontrib>Phillips, A</creatorcontrib><creatorcontrib>Quimby, R M</creatorcontrib><creatorcontrib>Rowell, G</creatorcontrib><creatorcontrib>Rujopakarn, W</creatorcontrib><creatorcontrib>Rykoff, E S</creatorcontrib><creatorcontrib>Schaefer, B E</creatorcontrib><creatorcontrib>Smith, D A</creatorcontrib><creatorcontrib>Swan, H F</creatorcontrib><creatorcontrib>Vestrand, W T</creatorcontrib><creatorcontrib>Wheeler, J C</creatorcontrib><creatorcontrib>Wren, J</creatorcontrib><creatorcontrib>Yuan, F</creatorcontrib><title>The Dark Side of ROTSE-III Prompt GRB Observations</title><title>arXiv.org</title><description>We present several cases of optical observations during gamma-ray bursts (GRBs) which resulted in prompt limits but no detection of optical emission. 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These limits constrain the prompt optical flux densities and the optical brightness relative to the gamma-ray emission. The derived constraints fall within the range of properties observed in GRBs with prompt optical detections, though at the faint end of optical/gamma flux ratios. The presently accessible prompt optical limits do not require a different set of intrinsic or environmental GRB properties, relative to the events with prompt optical detections.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0707.3132</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Emissions control Gamma ray bursts Gamma rays Optical properties Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | The Dark Side of ROTSE-III Prompt GRB Observations |
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