Zobrazeno 1 - 10
of 167
pro vyhledávání: '"Barthelemy, S."'
Autor:
Bompaire, F., Barthelemy, S., Monin, J., Quirins, M., Marion, L., Smith, C., Boulogne, S., Auxemery, Y.
Publikováno v:
In European Journal of Trauma & Dissociation February 2021 5(1)
Autor:
Hong, J., Allen, B., Grindlay, J., Barthelemy, S., Baker, R., Garson, A., Krawczynski, H., Apple, J., Cleveland, W. H.
We successfully carried out the first high-altitude balloon flight of a wide-field hard X-ray coded-aperture telescope ProtoEXIST1, which was launched from the Columbia Scientific Balloon Facility at Ft. Sumner, New Mexico on October 9, 2009. ProtoEX
Externí odkaz:
http://arxiv.org/abs/1107.5573
Autor:
Hong, J., Allen, B., Grindlay, J., Chammas, N., Barthelemy, S., Baker, R., Gehrels, N., Nelson, K. E., Labov, S., Collins, J., Cook, W. R., McLean, R., Harrison, F.
Publikováno v:
Nucl.Instrum.Meth.A605:364-373,2009
We have constructed a moderately large area (32 cm2), fine pixel (2.5 mm pixel, 5 mm thick) CZT imaging detector which constitutes the first section of a detector module (256 cm2) developed for a balloon-borne wide-field hard X-ray telescope, ProtoEX
Externí odkaz:
http://arxiv.org/abs/0903.5363
Autor:
Cusumano, G., Mangano, V., Chincarini, G., Panaitescu, A., Burrows, D. N., La Parola, V., Sakamoto, T., Campana, S., Mineo, T., Tagliaferri, G., Angelini, L., Barthelemy, S. D., Beardmore, A. P., Boyd, P. T., Cominsky, L., Gronwall, C., Fenimore, E. E., Gehrels, N., Giommi, P., Goad, M., Hurley, K., Immler, S., Kennea, J. A., Mason, K. O., Marshall, F., Meszaros, P., Nousek, J. A., Osborne, J. P., Palmer, D. M., Roming, P. W. A., Wells, A., White, N. E., Zhang, B.
Publikováno v:
Astron.Astrophys.462:73,2007
Swift discovered the high redshift (z=6.29) GRB050904 with the Burst Alert Telescope (BAT) and began observing with its narrow field instruments 161 s after the burst onset. This gamma-ray burst is the most distant cosmic explosion ever observed. Bec
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610570
Autor:
Cusumano, G., Mangano, V., Chincarini, G., Panaitescu, A., Burrows, D. N., La Parola, V., Sakamoto, T., Campana, S., Mineo, T., Tagliaferri, G., Angelini, L., Barthelemy, S. D., Beardmore, A. P., Boyd, P. T., Cominsky, L., Gronwall, C., Fenimore, E. E., Gehrels, N., Giommi, P., Goad, M., Hurley, K., Kennea, J. A., Mason, K. O., Marshall, F., Meszaros, P., Nousek, J. A., Osborne, J. P., Palmer, D. M., Roming, P. W. A., Wells, A., White, N. E., Zhang, B.
Gamma-ray Bursts (GRBs) are bright flashes of high energy photons that can last from about 10 milliseconds to 10 minutes. Their origin and nature have puzzled the scientific community for about 25 years until 1997, when the first X-ray afterglows of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509737
Publikováno v:
In Journal of Hydrology July 2018 562:623-634
Autor:
Fenimore, E. E., McLean, K., Palmer, D., Barthelemy, S., Gehrels, N., Krimm, H., Markwardt, C., Parsons, A., Stephens, M., Tueller, J.
The Swift satellite will be a self-contained observatory that will bring new capabilities to the observing of the early afterglow emission of Gamma-ray Bursts. Swift is completely autonomous and will do all of the observations without help from the g
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408513
Publikováno v:
In Journal of Hydrology September 2017 552:210-224
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