Zobrazeno 1 - 10
of 380
pro vyhledávání: '"Band, D"'
Autor:
Band, D. L., Axelsson, M., Baldini, L., Barbiellini, G., Baring, M. G., Bastieri, D., Battelino, M., Bellazzini, R., Bissaldi, E., Bogaert, G., Bonnel, J., Chiang, J., Cohen-Tanugi, J., Connaughton, V., Cutini, S., de Palma, F., Dingus, B. L., Silva, E. do Couto e, Fishman, G., Galli, A., Gehrels, N., Giglietto, N., Granot, J., Guiriec, S., Hughes, R. E., Kamae, T., Komin, N., Kuehn, F., Kuss, M., Longo, F., Lubrano, P., Kippen, R. M., Mazziotta, M. N., McEnery, J. E., McGlynn, S., Moretti, E., Nakamori, T., Norris, J. P., Ohno, M., Olivo, M., Omodei, N., Pelassa, V., Piron, F., Preece, R., Razzano, M., Russell, J. J., Ryde, F., Parkinson, P. M. Saz, Scargle, J. D., Sgrò, C., Shimokawabe, T., Smith, P. D., Spandre, G., Spinelli, P., Stamatikos, M., Winer, B. L., Yamazaki, R.
Publikováno v:
Astrophys.J.701:1673-1694,2009
The LAT instrument on the Fermi mission will reveal the rich spectral and temporal gamma-ray burst phenomena in the > 100 MeV band. The synergy with Fermi's GBM detectors will link these observations to those in the well explored 10-1000 keV range; t
Externí odkaz:
http://arxiv.org/abs/0906.0991
Autor:
Band, D. L., Grindlay, J. E., Hong, J., Fishman, G., Hartmann, D. H., Garson III, A., Krawczynski, H., Barthelmy, S., Gehrels, N., Skinner, G.
We use semi-analytic techniques to evaluate the burst sensitivity of designs for the EXIST hard X-ray survey mission. Applying these techniques to the mission design proposed for the Beyond Einstein program, we find that with its very large field-of-
Externí odkaz:
http://arxiv.org/abs/0710.4602
Autor:
Kashlinsky, A., Band, D.
Publikováno v:
AIP Conf.Proc.921:243-245,2007
Cosmic infrared background (CIB) includes emissions from objects inaccessible to current telescopic studies, such as the putative Population III, the first stars. Recently, strong direct evidence for significant CIB levels produced by the first stars
Externí odkaz:
http://arxiv.org/abs/0704.0225
Autor:
Goad, M. R., Page, K. L., Godet, O., Beardmore, A., Osborne, J. P., O'Brien, P. T., Starling, R., Holland, S., Band, D., Gehrels, N., Falcone, A., Burrows, D. N., Nousek, J. A., Roming, P. W. A., Moretti, A., Perri, M.
We report on the temporal and spectral characteristics of the early X-ray emission from the Gamma Ray Burst 051117A as observed by Swift. The superb quality of the early X-ray light-curve and spectra of this source, one of the brightest seen by the X
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612661
Autor:
Blustin, A. J., Band, D., Barthelmy, S., Boyd, P., Capalbi, M., Holland, S. T., Marshall, F. E., Mason, K. O., Perri, M., Poole, T., Roming, P., Rosen, S., Schady, P., Still, M., Zhang, B.
Publikováno v:
Astrophys.J.637:901-913,2006
The bright gamma-ray burst GRB050525a has been detected with the Swift observatory, providing unique multiwavelength coverage from the very earliest phases of the burst. The X-ray and optical/UV afterglow decay light curves both exhibit a steeper slo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507515
Using the lag-luminosity relation and various BATSE catalogs we create a large catalog of burst redshifts, peak luminosities and emitted energies. These catalogs permit us to evaluate the lag-luminosity relation, and to study the burst energy distrib
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312336
The GLAST Burst Monitor (GBM) will detect and localize bursts for the GLAST mission, and provide the spectral and temporal context in the traditional 10 keV to 25 MeV band for the high energy observations by the Large Area Telescope (LAT). The GBM wi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312335
Autor:
Kotani, T., Trushkin, S., Denissyuk, E. K., Kawakita, N., Kinugasa, K., Safi-Harb, S., Band, D.
The detection of a massive jet-ejection event from SS433 with RXTE is reported. SS433 in its high state has been monitored with RXTE from 2001/11/09 (MJD = 52222) to 2001/11/25 (MJD = 52238), following a radio flare on 2001/11/02 (MJD = 52215). An ir
Externí odkaz:
http://arxiv.org/abs/astro-ph/0208250
We present the main results of a study of time-resolved spectra of 43 intense GRBs detected by BATSE. We considered the 4-parameter Band model and the Optically Thin Synchrotron Shock model (OTSSM). We find that the large majority of time-resolved sp
Externí odkaz:
http://arxiv.org/abs/astro-ph/0002207
Autor:
Williams, G. G., Hartmann, D. H., Park, H. S., Porrata, R. A., Ables, E., Bionta, R., Band, D. L., Barthelmy, S. D., cline, T., Gehrels, N., Ferguson, D. H., Fishman, G., Kippen, R. M., Kouveliotou, C., Hurley, K., Nemiroff, R., Sasseen, T.
GRB 990123 established the existence of prompt optical emission from gamma-ray bursts (GRBs). The Livermore Optical Transient Imaging System (LOTIS) has been conducting a fully automated search for this kind of simultaneous low energy emission from G
Externí odkaz:
http://arxiv.org/abs/astro-ph/9912402