Zobrazeno 1 - 8
of 8
pro vyhledávání: '"A. D. P. Hands"'
Autor:
D. Wade Hands
Publikováno v:
Œconomia, Vol 9, Iss 3, Pp 595-605 (2019)
Externí odkaz:
https://doaj.org/article/0ef68eec4b8c4bc7b4a2d58c274ee356
Autor:
C. S. Dyer, K. A. Ryden, P. A. Morris, A. D. P. Hands, P. J. McNulty, J. -R. Vaille, L. Dusseau, G. Cellere, A. Paccagnella, H. J. Barnaby, A. R. Benedetto, R. Velazco, R. Possamai Bastos, D. Brewer, J. L. Barth, K. A. LaBel, M. J. Campola, Y. Zheng, M. A. Xapsos
Publikováno v:
IEEE Transactions on Nuclear Science. 70:200-215
Autor:
D. Wade Hands
Publikováno v:
Œconomia, Vol 7, Iss 3, Pp 409-438 (2017)
Externí odkaz:
https://doaj.org/article/1e6b8816d32a4586bec2be8e007fb00d
Publikováno v:
Space Weather. 20
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 343:995-1001
An analysis is presented of the soft X-ray background spectrum measured by the EPIC MOS cameras on XMM-Newton in three observations targeted on the North Polar Spur (NPS). Three distinct Galactic plasma components are identified, a cool Local Hot Bub
Autor:
A. D. P. Hands, L. G. I. Bennett, Brent J. Lewis, B.H. Bennett, I. L. Getley, C. S. Dyer, M. L. Duldig
Publikováno v:
Space Weather. 8
[1] With the development of next generation aircraft designs capable of ultralong-range flight and extended flight endurance, new experimental dosimetry equipment has been specifically designed to enable aircrew to monitor and respond to airborne ale
We present the first results from the \xmm Galactic Plane Survey (XGPS). In the first phase of the programme, 22 pointings were used to cover a region of approximately three square degrees between 19\deg -- 22\deg in Galactic longitude and $\pm$0.6\d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2ca7ec578d68d1389700009ff306ee7
http://arxiv.org/abs/astro-ph/0403304
http://arxiv.org/abs/astro-ph/0403304
Autor:
Martin Ward, P. Lira, R. S. Warwick, P. T. O'Brien, Timothy P.L. Roberts, A. D. P. Hands, Michael R. Goad
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2001, Vol.325(2), pp.L7-L11 [Peer Reviewed Journal]
We report the identification of a possible optical counterpart to the super-Eddington X-ray source NGC 5204 X-1. New Chandra data shows that the X-ray source is point-like, with a luminosity of 5.2 x 10^39 erg/s (0.5 - 8 keV). It displays medium- and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09ac8909222703fab9650475a64b9c63
http://dro.dur.ac.uk/1596/1/1596.pdf
http://dro.dur.ac.uk/1596/1/1596.pdf