Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Hurkett, C."'
Autor:
Starling, R. L. C., Wiersema, K., Levan, A. J., Sakamoto, T., Bersier, D., Goldoni, P., Oates, S. R., Rowlinson, A., Campana, S., Sollerman, J., Tanvir, N. R., Malesani, D., Fynbo, J. P. U., Covino, S., D'Avanzo, P., O'Brien, P. T., Page, K. L., Osborne, J. P., Vergani, S. D., Barthelmy, S., Burrows, D. N., Cano, Z., Curran, P. A., De Pasquale, M., D'Elia, V., Evans, P. A., Flores, H., Fruchter, A. S., Garnavich, P., Gehrels, N., Gorosabel, J., Hjorth, J., Holland, S. T., van der Horst, A. J., Hurkett, C. P., Jakobsson, P., Kamble, A. P., Kouveliotou, C., Kuin, N. P. M., Kaper, L., Mazzali, P. A., Nugent, P. E., Pian, E., Stamatikos, M., Thoene, C. C., Woosley, S. E.
Publikováno v:
Mon. Not. Roy. Astron. Soc. 411 (2011) 2792-2803
We report the Swift discovery of nearby long, soft gamma-ray burst GRB 100316D, and the subsequent unveiling of its low redshift host galaxy and associated supernova. We derive the redshift of the event to be z = 0.0591 +/- 0.0001 and provide accurat
Externí odkaz:
http://arxiv.org/abs/1004.2919
Autor:
Hurkett, C. P., Vaughan, S., Osborne, J. P., O'Brien, P. T., Page, K. L., Beardmore, A., Godet, O., Burrows, D. N., Capalbi, M., Evans, P., Gehrels, N., Goad, M. R., Hill, J. E., Kennea, J., Mineo, T., Perri, M., Starling, R.
Prior to the launch of the Swift mission several X-ray line detections were reported in Gamma Ray Burst afterglow spectra. To date, these pre-Swift era results have not been conclusively confirmed. The most contentious issue in this area is the choic
Externí odkaz:
http://arxiv.org/abs/0802.0441
Autor:
Levan, A. J., Jakobsson, P., Hurkett, C., Tanvir, N. R., Gorosabel, J., Vreeswijk, P., Rol, E., Chapman, R., Gehrels, N., O'Brien, P. T., Osborne, J. P., Priddey, R. S., Kouveliotou, C., Starling, R., Berk, D. Vanden, Wiersema, K.
Publikováno v:
Mon.Not.Roy.Astron.Soc.378:1439-1446,2007
We investigate the origin of the GRB 060912A, which has observational properties that make its classification as either a long or short burst ambiguous. Short duration GRBs (SGRBs) are thought to have typically lower energies than long duration burst
Externí odkaz:
http://arxiv.org/abs/0704.2525
Autor:
Curran, P. A., van der Horst, A. J., Beardmore, A. P., Page, K. L., Rol, E., Melandri, A., Steele, I. A., Mundell, C. G., Gomboc, A., O'Brien, P. T., Bersier, D. F., Bode, M. F., Carter, D., Guidorzi, C., Hill, J. E., Hurkett, C. P., Kobayashi, S., Monfardini, A., Mottram, C. J., Smith, R. J., Wijers, R. A. M. J., Willingale, R.
We present our analysis of the multiwavelength photometric & spectroscopic observations of GRB 060210 and discuss the results in the overall context of current GRB models. All available optical data underwent a simultaneous temporal fit, while X-ray
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701087
Autor:
Burleigh, M. R., Marsh, T. R., Gansicke, B. T., Goad, M. R., Dhillon, V. S., Littlefair, S. P., Wells, M., Bannister, N. P., Hurkett, C. P., Martindale, A., Dobbie, P. D., Casewell, S. L., Baker, D. E. A., Duke, J., Farihi, J., Irwin, M. J., Hewett, P. C., Roche, P., Lewis, F.
Publikováno v:
Mon.Not.Roy.Astron.Soc.373:1416-1422,2006
Optical time series photometry of the short period magnetic white dwarf + probable brown dwarf binary SDSS 121209.31+013627.7 reveals pulse-like variability in all bands from i' to u', peaking at u'. These modulations are most likely due to a self-ec
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607389
Autor:
Krimm, H. A., Hurkett, C., Pal'shin, V., Norris, J. P., Zhang, B., Barthelmy, S. D., Burrows, D. N., Gehrels, N., Golenetskii, S., Osborne, J. P., Parsons, A. M., Perri, M., Willingale, R.
Publikováno v:
AIP Conf.Proc.836:141-144,2006; Astrophys.J.648:1117-1124,2006
The long burst GRB 050717 was observed simultaneously by the Burst Alert Telescope (BAT) on Swift and the Konus instrument on Wind. Significant hard to soft spectral evolution was seen. Early gamma-ray and X-ray emission was detected by both BAT and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605507
Autor:
Hurkett, C. P., Osborne, J. P., Page, K. L., Rol, E., Goad, M. R., O'Brien, P. T., Beardmore, A., Godet, O., Burrows, D. N., Tanvir, N. R., Levan, A., Zhang, B., Malesani, D., Hill, J. E., Kennea, J. A., Chapman, R., La Parola, V., Perri, M., Romano, P., Smith, R., Gehrels, N.
Publikováno v:
Mon.Not.Roy.Astron.Soc.368:1101-1109,2006
We report the discovery and subsequent multi-wavelength afterglow behaviour of the high redshift (z = 4.27) Gamma Ray Burst GRB 050505. This burst is the third most distant burst, measured by spectroscopic redshift, discovered after GRB 000131 (z = 4
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602236
Autor:
O'Brien, P. T., Willingale, R., Osborne, J., Goad, M. R., Page, K. L., Vaughan, S., Rol, E., Beardmore, A., Godet, O., Hurkett, C., Wells, A., Zhang, B., Kobayashi, S., Burrows, D. N., Nousek, J. A., Kennea, J. A., Falcone, A., Grupe, D., Gehrels, N., Barthelmy, S., Cannizzo, J., Cummings, J., Hill, J., Krimm, H., Chincarini, G., Tagliaferri, G., Campana, S., Moretti, A., Giommi, P., Perri, M., Mangano, V., LaParola, V.
Publikováno v:
Astrophys.J.647:1213-1237,2006
We present observations of the early X-ray emission for a sample of 40 gamma-ray bursts (GRBs) obtained using the Swift satellite for which the narrow-field instruments were pointed at the burst within 10 minutes of the trigger. Using data from the B
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601125
Autor:
Nousek, J. A., Kouveliotou, C., Grupe, D., Page, K., Granot, J., Ramirez-Ruiz, E., Patel, S. K., Burrows, D. N., Mangano, V., Barthelmy, S., Beardmore, A. P., Campana, S., Capalbi, M., Chincarini, G., Cusumano, G., Falcone, A. D., Gehrels, N., Giommi, P., Goad, M., Godet, O., Hurkett, C., Kennea, J. A., Moretti, A., O'Brien, P., Osborne, J., Romano, P., Tagliaferri, G., Wells, A.
Publikováno v:
Astrophys.J.642:389-400,2006
We present new observations of the early X-ray afterglows of the first 27 gamma-ray bursts (GRBs) detected with the Swift X-ray Telescope (XRT). The early X-ray afterglows show a canonical behavior, where the light curve broadly consists of three dis
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508332
Publikováno v:
Physics community and cooperation: selected contributions: GIREP-EPEC & PHEC 2009 International Conference, August 17-21, University of Leicester, UK, 76-90
STARTPAGE=76;ENDPAGE=90;TITLE=Physics community and cooperation: selected contributions: GIREP-EPEC & PHEC 2009 International Conference, August 17-21, University of Leicester, UK
STARTPAGE=76;ENDPAGE=90;TITLE=Physics community and cooperation: selected contributions: GIREP-EPEC & PHEC 2009 International Conference, August 17-21, University of Leicester, UK
How can we use Watts’ frameworks (Watts, 1988) for talking about energy to design education on the subject of energy? We showed 6 pictures also used by Watts and gave a writing assignment to 17 fifteen year olds prior to any physics education on en
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::29e4f8ec2104709906f9f53bb54eed3f
https://dare.uva.nl/personal/pure/en/publications/frameworks-for-talking-about-energy--mutually-exclusive(0819f892-ba7b-4ab1-a925-f0fc027d54d4).html
https://dare.uva.nl/personal/pure/en/publications/frameworks-for-talking-about-energy--mutually-exclusive(0819f892-ba7b-4ab1-a925-f0fc027d54d4).html