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Jun 19, 1997 · GRB 970616 The transient X-ray XTE source reported below by F. Marshall et al. lies in the error box of a gamma-ray burst seen by BATSE on June 16.757 UT.
We report on near-infrared and optical obser- vations of the GRB 970616 error box and of the X-ray sources discovered by ASCA and ROSAT in the region.
- J. Gorosabel, A.J. Castro-Tirado, A.J. Castro-Tirado, Henrik Pedersen, J. Greiner, D. Thompson, M. G...
- 1999
Download scientific diagram | A coadded R-band image of the field of GRB 970616 obtained with the Danish 1.54-m telescope. The total exposure time is 19.5 hours and the limiting magnitude R =...
May 21, 1999 · We report on near-infrared and optical observations of the GRB 970616 error box and of the X-ray sources discovered by ASCA and ROSAT in the region. No optical transient was found either within...
- J. Gorosabel, A. J. Castro-Tirado, A. J. Castro-Tirado, H. Pedersen, J. Greiner, D. Thompson, M. Gue...
- arXiv:astro-ph/9905288
- 1999
- Astrophysics (astro-ph)
Gamma-ray Burst 970616. A very bright Gamma-Ray Burst (among the brightest 2%) was detected with BATSE on June 16.757 UT. The burst was multipeaked, with a total duration of about 200 s.
May 21, 1999 · We report on near-infrared and optical obser- vations of the GRB 970616 error box and of the X-ray sources discovered by ASCA and ROSAT in the region.
Jul 21, 1998 · We use these scaling laws to discuss the afterglows of GRB 970228 and GRB 970616, and find that if the spectral index of the electron distribution is p = 2.5, implied from the spectra of GRBs, the X-ray afterglow of GRB 970616 is well fitted by assuming k = 2.
