Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Amanda Maxham"'
Autor:
Henry I. Miller, Amanda Maxham
Publikováno v:
Journal of Commercial Biotechnology. 25
Recently the USDA proposed measures to “improve efficiencies” and help rural communities in “achieving prosperity.” The measures will not achieve such a goal. If “prosperity” is really USDA’s aim, we offer two suggestions to spur agricu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d30f848cec60feba9b6f23d3d6390b82
https://doi.org/10.5912/jcb870
https://doi.org/10.5912/jcb870
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 415:77-82
Recent observations of Gamma-Ray Bursts (GRBs) by the Fermi Large Area Telescope (LAT) revealed a power law decay feature of the high energy emission (above 100 MeV), which led to the suggestion that it originates from a (probably radiative) external
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::24107fb515979ca5521bec5af3b348c6
https://doi.org/10.1111/j.1365-2966.2011.18648.x
https://doi.org/10.1111/j.1365-2966.2011.18648.x
Autor:
Amanda Maxham, Patricia Schady, P. W. A. Roming, M. de Pasquale, Bing Zhang, K. L. Page, Bin-Bin Zhang, S. T. Holland, J. A. Kennea, N. P. M. Kuin, S. R. Oates, L. Vetere, C. A. Swenson
Publikováno v:
The Astrophysical Journal. 718:L14-L18
GRB 090926A was detected by both the GBM and LAT instruments on-board the Fermi Gamma-Ray Space Telescope. Swift follow-up observations began ~13 hours after the initial trigger. The optical afterglow was detected for nearly 23 days post trigger, pla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12feabac662da4ce32ed85fe0b343075
https://doi.org/10.1088/2041-8205/718/1/l14
https://doi.org/10.1088/2041-8205/718/1/l14
Autor:
Amanda Maxham, Bing Zhang
Publikováno v:
The Astrophysical Journal. 707:1623-1633
X-ray afterglow light curves have been collected for over 400 Swift gamma-ray bursts with nearly half of them having X-ray flares superimposed on the regular afterglow decay. Evidence suggests that gamma-ray prompt emission and X-ray flares share a c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::194c681b4ce1b797722df0f114c12e35
https://doi.org/10.1088/0004-637x/707/2/1623
https://doi.org/10.1088/0004-637x/707/2/1623
Publikováno v:
AIP Conference Proceedings.
We have developed a shell model code to address the question of how gamma‐ray prompt emission and x‐ray flares are produced within the framework of the internal shock model. The shell model creates randomized GRB explosions from the central engin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::647238a4a3327aa66edcdf1f6e8f08e5
https://doi.org/10.1063/1.2943489
https://doi.org/10.1063/1.2943489