The dark side of ROTSE-III prompt GRB observations

Yost, S.; Aharonian, F.; Akerlof, C.; Ashley, M.; Barthelmy, S.; Gehrels, N.; Goegues, E.; Guever, TOLGA; Horns, D.; Kiziloglu, Ue.; Krimm, H.; Mckay, T.; Oezel, M.; Phillips, A.; Quimby, R.; Rowell, G.; Rujopakarn, W.; Rykoff, E.; Schaefer, B.; Smith, D.; Swan, H.; Vestrand, W.; Wheeler, J.; Wren, J.; Yuan, F.

doi:10.1086/521668

The dark side of ROTSE-III prompt GRB observations

Yost S. A., Aharonian F., Akerlof C. W., Ashley M. C. B., Barthelmy S., Gehrels N., ...Daha Fazla

ASTROPHYSICAL JOURNAL, cilt.669, sa.2, ss.1107-1114, 2007 (SCI-Expanded, Scopus)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 669 Sayı: 2
Basım Tarihi: 2007
Doi Numarası: 10.1086/521668
Dergi Adı: ASTROPHYSICAL JOURNAL
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.1107-1114
İstanbul Üniversitesi Adresli: Evet

Özet

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, although at the faint end of optical/gamma-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.