Zobrazeno 1 - 10
of 114
pro vyhledávání: '"Hurley, Kevin P."'
Autor:
Ahumada, Tomas, Singer, Leo P., Anand, Shreya, Coughlin, Michael W., Kasliwal, Mansi M., Ryan, Geoffrey, Andreoni, Igor, Cenko, S. Bradley, Fremling, Christoffer, Kumar, Harsh, Pang, Peter T. H., Burns, Eric, Cunningham, Virginia, Dichiara, Simone, Dietrich, Tim, Svinkin, Dmitry S., Almualla, Mouza, Castro-Tirado, Alberto J., De, Kishalay, Dunwoody, Rachel, Gatkine, Pradip, Hammerstein, Erica, Iyyani, Shabnam, Mangan, Joseph, Perley, Dan, Purkayastha, Sonalika, Bellm, Eric, Bhalerao, Varun, Bolin, Bryce, Bulla, Mattia, Cannella, Christopher, Chandra, Poonam, Duev, Dmitry A., Frederiks, Dmitry, Gal-Yam, Avishay, Graham, Matthew, Ho, Anna Y. Q., Hurley, Kevin, Karambelkar, Viraj, Kool, Erik C., Kulkarni, S. R., Mahabal, Ashish, Masci, Frank, McBreen, Sheila, Pandey, Shashi B., Reusch, Simeon, Ridnaia, Anna, Rosnet, Philippe, Rusholme, Benjamin, Carracedo, Ana Sagues, Smith, Roger, Soumagnac, Maayane, Stein, Robert, Troja, Eleonora, Tsvetkova, Anastasia, Walters, Richard, Valeev, Azamat F.
Gamma-ray bursts (GRBs) are among the brightest and most energetic events in the universe. The duration and hardness distribution of GRBs has two clusters, now understood to reflect (at least) two different progenitors. Short-hard GRBs (SGRBs; T90 <2
Externí odkaz:
http://arxiv.org/abs/2105.05067
Autor:
Hurley, Kevin C.
We study the characteristics of Near-Earth-Networks (NENs) of gamma-ray burst (GRB) detectors, with the objective of defining a network with all-sky, full-time localization capability for multi-messenger astrophysics. We show that a minimum network c
Externí odkaz:
http://arxiv.org/abs/2010.04229
Autor:
Singer, Leo P., Kasliwal, Mansi M., Cenko, S. Bradley, Perley, Daniel A., Anderson, Gemma E., Anupama, G. C., Arcavi, Iair, Bhalerao, Varun, Bue, Brian D., Cao, Yi, Connaughton, Valerie, Corsi, Alessandra, Cucchiara, Antonino, Fender, Rob P., Fox, Derek B., Gehrels, Neil, Goldstein, Adam, Gorosabel, J., Horesh, Assaf, Hurley, Kevin, Johansson, Joel, Kann, D. A., Kouveliotou, Chryssa, Huang, Kuiyun, Kulkarni, S. R., Masci, Frank, Nugent, Peter, Rau, Arne, Rebbapragada, Umaa D., Staley, Tim D., Svinkin, Dmitry, Thöne, C. C., Postigo, A. de Ugarte, Urata, Yuji, Weinstein, Alan
Publikováno v:
2015 ApJ 806 52
The Fermi Gamma-ray Space Telescope has greatly expanded the number and energy window of observations of gamma-ray bursts (GRBs). However, the coarse localizations of tens to a hundred square degrees provided by the Fermi GRB Monitor instrument have
Externí odkaz:
http://arxiv.org/abs/1501.00495
Autor:
Bartos, Imre, Veres, Peter, Nieto, Daniel, Connaughton, Valerie, Humensky, Brian, Hurley, Kevin, Marka, Szabolcs, Meszaros, Peter, Mukherjee, Reshmi, O'Brien, Paul, Osborne, Julian P.
The first gravitational-wave (GW) observations will greatly benefit from the detection of coincident electromagnetic counterparts. Electromagnetic follow-ups will nevertheless be challenging for GWs with poorly reconstructed directions. GW source loc
Externí odkaz:
http://arxiv.org/abs/1403.6119
Autor:
Chakraborti, Sayan, Soderberg, Alicia, Chomiuk, Laura, Kamble, Atish, Yadav, Naveen, Ray, Alak, Hurley, Kevin, Margutti, Raffaella, Milisavljevic, Dan, Bietenholz, Michael, Brunthaler, Andreas, Pignata, Giuliano, Pian, Elena, Mazzali, Paolo, Fransson, Claes, Bartel, Norbert, Hamuy, Mario, Levesque, Emily, MacFadyen, Andrew, Dittmann, Jason, Krauss, Miriam, Briggs, M. S., Connaughton, V., Yamaoka, K., Takahashi, T., Ohno, M., Fukazawa, Y., Tashiro, M., Terada, Y., Murakami, T., Goldsten, J., Barthelmy, S., Gehrels, N., Cummings, J., Krimm, H., Palmer, D., Golenetskii, S., Aptekar, R., Frederiks, D., Svinkin, D., Cline, T., Mitrofanov, I. G., Golovin, D., Litvak, M. L., Sanin, A. B., Boynton, W., Fellows, C., Harshman, K., Enos, H., von Kienlin, A., Rau, A., Zhang, X., Savchenko, V.
Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly usually within days, because their low-mass ejecta rapidly sweep up a
Externí odkaz:
http://arxiv.org/abs/1402.6336
Jet heating via nuclear collisions may be the main mechanism for gamma-ray burst (GRB) emission. Besides producing the observed gamma-rays, collisional heating must generate 10-100 GeV neutrinos, implying a close relation between the neutrino and gam
Externí odkaz:
http://arxiv.org/abs/1301.4232
Autor:
Rea, Nanda, Israel, GianLuca, Turolla, Roberto, Esposito, Paolo, Mereghetti, Sandro, Gotz, Diego, Zane, Silvia, Tiengo, Andrea, Hurley, Kevin, Feroci, Marco, Still, Martin, Yershov, Vladimir, Winkler, Christoph, Perna, Rosalba, Bernardini, Federico, Ubertini, Pietro, Stella, Luigi, Campana, Sergio, van der Klis, Michiel, Woods, Peter M.
We report here on the outburst onset and evolution of the new Soft Gamma Repeater SGR 0501+4516. We monitored the new SGR with XMM-Newton starting on 2008 August 23, one day after the source became burst-active, and continuing with 4 more observation
Externí odkaz:
http://arxiv.org/abs/0904.2413
Autor:
Updike, Adria C., Haislip, Joshua B., Nysewander, Melissa C., Fruchter, Andrew S., Kann, D. Alexander, Klose, Sylvio, Milne, Peter A., Williams, G. Grant, Zheng, Weikang, Hergenrother, Carl W., Prochaska, Jason X., Halpern, Jules P., Mirabal, Nestor, Thorstensen, John R., van der Horst, Alexander J., Starling, Rhaana L. C., Racusin, Judith L., Burrows, David N., Kuin, N. P. M., Roming, Peter W. A., Bellm, Eric, Hurley, Kevin, Li, Weidong, Filippenko, Alexei V., Blake, Cullen, Starr, Dan, Falco, Emilio E., Brown, Warren R., Dai, Xinyu, Deng, Jinsong, Xin, Liping, Qiu, Yulei, Wei, Jianyan, Urata, Yuji, Nanni, Domenico, Maiorano, Elisabetta, Palazzi, Eliana, Greco, Giuseppe, Bartolini, Corrado, Guarnieri, Adriano, Piccioni, Adalberto, Pizzichini, Graziella, Terra, Federica, Misra, Kuntal, Bhatt, B. C., Anupama, G. C., Fan, X., Jiang, L., Wijers, Ralph A. M. J., Reichart, Dan E., Eid, Hala A., Bryngelson, Ginger, Puls, Jason, Goldthwaite, R. C., Hartmann, Dieter H.
We report on multi-wavelength observations, ranging from the X-ray to radio wave bands, of the IPN-localized gamma-ray burst GRB 070125. Spectroscopic observations reveal the presence of absorption lines due to O I, Si II, and C IV, implying a likely
Externí odkaz:
http://arxiv.org/abs/0805.1094
Autor:
Shirasaki, Yuji, Yoshida, Atsumasa, Kawai, Nobuyuki, Tamagawa, Toru, Sakamoto, Takanori, Suzuki, Motoko, Nakagawam, Yujin, Kobayashi, Akina, Sugita, Satoshi, Takahashi, Ichiro, Arimoto, Makoto, Shimokawabe, Takashi, Pazmino, Nicolas Vasquez, Ishimura, Takuto, Sato, Rie, Matsuoka, Masaru, Fenimore, Edward E., Galassi, Mark, Lamb, Donald Q., Graziani, Carlo, Donaghy, Timothy Q., Atteia, Jean-Luc, Pelangeon, Alexandre, Vanderspek, Roland, Crew, Geoffrey B., Doty, John P., Villasenor, Joel, Prigozhin, Gregory, Butler, Nat, Ricker, George R., Hurley, Kevin, Woosley, Stanford E., Pizzichini, Graziella
Publikováno v:
Publ.Astron.Soc.Jap.60:919,2008
GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. This GRB displays a soft X-ray emission, a precursor before the onset of the main event, and also a soft X-ray tail after the end of the main peak. The light curves in four differen
Externí odkaz:
http://arxiv.org/abs/0802.1649
Autor:
Ohno, Masanori, Fukazawa, Yasushi, Takahashi, Takuya, Yamaoka, Kazutaka, Sugita, Satoshi, Pal'shin, Valentin, Sakamoto, Takanori, Sato, Goro, Hurley, Kevin, Frederiks, Dmitry, Oleynik, Philipp, Ulanov, Mikhail, Tashiro, Makoto, Urata, Yuji, Onda, Kaori, Tamagawa, Toru, Terada, Yukikatsu, Suzuki, Motoko, Soojing, Hong
We have performed a joint analysis of prompt emission from four bright short gamma-ray bursts (GRBs) with the Suzaku-WAM and the Konus-Wind experiments. This joint analysis allows us to investigate the spectral properties of short-duration bursts ove
Externí odkaz:
http://arxiv.org/abs/0801.2432