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pro vyhledávání: '"Gruber D"'
Autor:
Kopf, T., Glück, T., Gruber, D., Staderini, V., Eugui, P., Fritze, G., Mansouri, A., Schnall, M., Meyer-Heye, P.
Publikováno v:
In Journal of Manufacturing Processes 30 September 2024 126:12-23
Akademický článek
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Autor:
Collazzi, A. C., Kouveliotou, C., van der Horst, A. J., Younes, G. A., Kaneko, Y., Gogus, E., Lin, L., Granot, J., Finger, M. H., Chaplin, V. L., Huppenkothen, D., Watts, A. L., von Kienlin, A., Baring, M. G., Gruber, D., Bhat, P. N., Gibby, M. H., Gehrels, N., McEnery, J., van der Klis, M., Wijers, R. A. M. J.
Since launch in 2008, the Fermi Gamma-ray Burst Monitor (GBM) has detected many hundreds of bursts from magnetar sources. While the vast majority of these bursts have been attributed to several known magnetars, there is also a small sample of magneta
Externí odkaz:
http://arxiv.org/abs/1503.04152
Autor:
Connaughton, V., Briggs, M. S., Goldstein, A., Meegan, C. A., Paciesas, W. S., Preece, R. D., Wilson-Hodge, C. A., Gibby, M. H., Greiner, J., Gruber, D., Jenke, P., Kippen, R. M., Pelassa, V., Xiong, S., Yu, H. -F., Bhat, P. N., Burgess, J. M., Byrne, D., Fitzpatrick, G., Foley, S., Giles, M. M., Guiriec, S., van der Horst, A. J., von Kienlin, A., McBreen, S., McGlynn, S., Tierney, D., Zhang, B. -B.
The Fermi Gamma-ray Burst Monitor (GBM) has detected over 1400 Gamma-Ray Bursts (GRBs) since it began science operations in July, 2008. We use a subset of over 300 GRBs localized by instruments such as Swift, the Fermi Large Area Telescope, INTEGRAL,
Externí odkaz:
http://arxiv.org/abs/1411.2685
Autor:
Younes, G., Kouveliotou, C., van der Horst, A. J., Baring, M. G., Granot, J., Watts, A. L., Bhat, P. N., Collazzi, A., Gehrels, N., Gorgone, N., Gogus, E., Gruber, D., Grunblatt, S., Huppenkothen, D., Kaneko, Y., von Kienlin, A., van der Klis, M., Lin, L., Mcenery, J., van Putten, T., Wijers, R. A. M. J.
We report on time-resolved spectroscopy of the 63 brightest bursts of SGR J1550-5418, detected with Fermi/Gamma-ray Burst Monitor during its 2008-2009 intense bursting episode. We performed spectral analysis down to 4 ms time-scales, to characterize
Externí odkaz:
http://arxiv.org/abs/1402.6015
Autor:
Elliott, J., Yu, H. -F., Schmidl, S., Greiner, J., Gruber, D., Oates, S., Kobayashi, S., Zhang, B., Cummings, J. R., Filgas, R., Gehrels, N., Grupe, D., Kann, D. A., Klose, S., Krühler, T., Guelbenzu, A. Nicuesa, Rau, A., Rossi, A., Siegel, M., Schady, P., Sudilovsky, V., Tanga, M., Varela, K.
Since the advent of the Swift satellite it has been possible to obtain precise localisations of GRB positions of sub-arcsec accuracy within seconds, facilitating ground-based robotic telescopes to automatically slew to the target within seconds. This
Externí odkaz:
http://arxiv.org/abs/1312.5099
Autor:
Elliott, J., Yu, H. -F., Schmidl, S., Greiner, J., Gruber, D., Oates, S., Kobayashi, S., Zhang, B., Cummings, J. R., Filgas, R., Gehrels, N., Grupe, D., Kann, D. A., Klose, S., Krühler, T., Guelbenzu, A. Nicuesa, Rau, A., Rossi, A., Siegel, M., Schady, P., Sudilovsky, V., Tanga, M., Varela, K.
The mechanism that causes the prompt-emission episode of gamma-ray bursts (GRBs) is still widely debated despite there being thousands of prompt detections. The favoured internal shock model relates this emission to synchrotron radiation. However, it
Externí odkaz:
http://arxiv.org/abs/1312.4547
Autor:
Preece, R., Burgess, J. Michael, von Kienlin, A., Bhat, P. N., Briggs, M. S., Byrne, D., Chaplin, V., Cleveland, W., Collazzi, A. C., Connaughton, V., Diekmann, A., Fitzpatrick, G., Foley, S., Gibby, M., Giles, M., Goldstein, A., Greiner, J., Gruber, D., Jenke, P., Kippen, R. M., Kouveliotou, C., McBreen, S., Meegan, C., Paciesas, W. S., Pelassa, V., Tierney, D., van der Horst, A. J., Wilson-Hodge, C., Xiong, S., Younes, G., Yu, H. -F., Ackermann, M., Ajello, M., Axelsson, M., Baldini, L., Barbiellini, G., Baring, M. G., Bastieri, D., Bellazzini, R., Bissaldi, E., Bonamente, E., Bregeon, J., Brigida, M., Bruel, P., Buehler, R., Buson, S., Caliandro, G. A., Cameron, R. A., Caraveo, P. A., Cecchi, C., Charles, E., Chekhtman, A., Chiang, J., Chiaro, G., Ciprini, S., Claus, R., Cohen-Tanugi, J., Cominsky, L. R., Conrad, J., D'Ammando, F., de Angelis, A., de Palma, F., Dermer, C. D., Desiante, R., Digel, S. W., Di Venere, L., Drell, P. S., Drlica-Wagner, A., Favuzzi, C., Franckowiak, A., Fukazawa, Y., Fusco, P., Gargano, F., Gehrels, N., Germani, S., Giglietto, N., Giordano, F., Giroletti, M., Godfrey, G., Granot, J., Grenier, I. A., Guiriec, S., Hadasch, D., Hanabata, Y., Harding, A. K., Hayashida, M., Iyyani, S., Jogler, T., Jóannesson, G., Kawano, T., Knödlseder, J., Kocevski, D., Kuss, M., Lande, J., Larsson, J., Larsson, S., Latronico, L., Longo, F., Loparco, F., Lovellette, M. N., Lubrano, P., Mayer, M., Mazziotta, M. N., Michelson, P. F., Mizuno, T., Monzani, M. E., Moretti, E., Morselli, A., Murgia, S., Nemmen, R., Nuss, E., Nymark, T., Ohno, M., Ohsugi, T., Okumura, A., Omodei, N., Orienti, M., Paneque, D., Perkins, J. S., Pesce-Rollins, M., Piron, F., Pivato, G., Porter, T. A., Racusin, J. L., Rainò, S., Rando, R., Razzano, M., Razzaque, S., Reimer, A., Reimer, O., Ritz, S., Roth, M., Ryde, F., Sartori, A., Scargle, J. D., Schulz, A., Sgrò, C., Siskind, E. J., Spandre, G., Spinelli, P., Suson, D. J., Tajima, H., Takahashi, H., Thayer, J. G., Thayer, J. B., Tibaldo, L., Tinivella, M., Torres, D. F., Tosti, G., Troja, E., Usher, T. L., Vandenbroucke, J., Vasileiou, V., Vianello, G., Vitale, V., Werner, M., Winer, B. L., Wood, K. S., Zhu, S.
Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 s is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of the peak e
Externí odkaz:
http://arxiv.org/abs/1311.5581
Autor:
Burgess, J. M., Preece, R. D., Connaughton, V., Briggs, M. S., Goldstein, A., Bhat, P. N., Greiner, J., Gruber, D., Kienlin, A., Kouveliotou, C., McGlynn, S., Meegan, C. A., Paciesas, W. S., Rau, A., Xiong, S., Axelsson, M., Baring, M. G., Dermer, C. D., Iyyani, S., Kocevski, D., Omodei, N., Ryde, F., Vianello, G.
Publikováno v:
ApJ 784:17 (2014)
Time-resolved spectroscopy is performed on eight bright, long gamma-ray bursts (GRBs) dominated by single emission pulses that were observed with the {\it Fermi Gamma-ray Space Telescope}. Fitting the prompt radiation of GRBs by empirical spectral fo
Externí odkaz:
http://arxiv.org/abs/1304.4628
Autor:
Cenko, S. Bradley, Kulkarni, S. R., Horesh, Assaf, Corsi, Alessandra, Fox, Derek B., Carpenter, John, Frail, Dale A., Nugent, Peter E., Perley, Daniel A., Gruber, D., Gal-Yam, Avishay, Groot, Paul J., Hallinan, G., Ofek, Eran O., Rau, Arne, MacLeod, Chelsea L., Miller, Adam A., Bloom, Joshua S., Filippenko, Alexei V., Kasliwal, Mansi M., Law, Nicholas M., Morgan, Adam N., Polishook, David, Poznanski, Dovi, Quimby, Robert M., Sesar, Branimir, Shen, Ken J., Silverman, Jeffrey M., Sternberg, Assaf
We report the discovery by the Palomar Transient Factory (PTF) of the transient source PTF11agg, which is distinguished by three primary characteristics: (1) bright, rapidly fading optical transient emission; (2) a faint, blue quiescent optical count
Externí odkaz:
http://arxiv.org/abs/1304.4236