Document Type
Article
Publication Date
11-10-2007
Abstract
We 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 7-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/7-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. © 2007. The American Astronomical Society. All rights reserved.
Publication Source (Journal or Book title)
Astrophysical Journal
First Page
1107
Last Page
1114
Recommended Citation
Yost, S., Aharonian, F., Akerlof, C., Ashley, M., Barthelmy, S., Gehrels, N., Göǧüş, E., Güver, T., Horns, D., Kiziloǧlu, Ü., Krimm, H., McKay, T., Özel, 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. (2007). The dark side of rotse-III prompt GRB observations. Astrophysical Journal, 669 (2), 1107-1114. https://doi.org/10.1086/521668