Zobrazeno 1 - 6
of 6
pro vyhledávání: '"D. N. Spergel"'
Autor:
R. Drimmel, D. N. Spergel
Publikováno v:
The Astrophysical Journal. 556:181-202
We present a three dimensional model for the Milky Way fit to the far-infrared (FIR) and near-infrared (NIR) data from the COBE/DIRBE instrument for Galactic latitudes |b| < 30 degrees and to within 20 degrees of the Galactic center. Because of the l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d0b5d97af4e92a287b48e998784c9056
https://doi.org/10.1086/321556
https://doi.org/10.1086/321556
Publikováno v:
The Astrophysical Journal, 735:38 (20pp), 2011 July 1.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=erc_________::fcdda3e39af49063fe3703e1ed94b425
Autor:
Arlie O. Petters, D. N. Spergel
Publikováno v:
Gravitational Lenses ISBN: 9783540557975
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6daee85edc96b6094f45c634a8ceab30
https://doi.org/10.1007/3-540-55797-0_142
https://doi.org/10.1007/3-540-55797-0_142
Autor:
M. R. Nolta, J. Dunkley, R. S. Hill, G. Hinshaw, E. Komatsu, D. Larson, L. Page, D. N. Spergel, C. L. Bennett, B. Gold, N. Jarosik, N. Odegard, J. L. Weiland, E. Wollack, M. Halpern, A. Kogut, M. Limon, S. S. Meyer, G. S. Tucker, E. L. Wright
We present the temperature and polarization angular power spectra of the cosmic microwave background (CMB) derived from the first 5 years of WMAP data. The 5-year temperature (TT) spectrum is cosmic variance limited up to multipole l=530, and individ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1dc6ea6cb6291600ba249681f4d5559f
Publikováno v:
Dark Matter in the Universe ISBN: 9789027723574
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6e07b02e81c672624a88e994a328109
https://doi.org/10.1007/978-94-009-4772-6_93
https://doi.org/10.1007/978-94-009-4772-6_93
Publikováno v:
Symposium - International Astronomical Union. 117:490-490
We consider the use of superheated superconducting colloids as detectors of weakly interacting galactic halo candidate particles (e.g. photinos, massive neutrinos, and scalar neutrinos). These low temperature detectors are sensitive to the deposition
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c913294dcc3da06cadcfd7a8a2ee2659
https://doi.org/10.1017/s0074180900150703
https://doi.org/10.1017/s0074180900150703