Zobrazeno 1 - 10
of 92
pro vyhledávání: '"J. B. Peterson"'
Autor:
M. F. Baumgardner, J. B. Peterson
Publikováno v:
International Agronomy Training & Education
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c4f3ad82172b44723f100ae79f1638b6
https://doi.org/10.2134/asaspecpub15.c2
https://doi.org/10.2134/asaspecpub15.c2
Autor:
J. B. Peterson
Publikováno v:
Agronomy in Today's Society
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::79d4f4c9a0bf71b84983c655aeb5a2ce
https://doi.org/10.2134/asaspecpub33.c2
https://doi.org/10.2134/asaspecpub33.c2
Autor:
Marisa A. Wiktor, Stacy J. B. Peterson, A. Chronic Pain, Michelle Miller, B. Conversion Disorders
Publikováno v:
Pediatric Rehabilitation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a78633670f8b5f4f2cd628e93be563e9
https://doi.org/10.1891/9781617052255.0020
https://doi.org/10.1891/9781617052255.0020
Autor:
M. Lueker, Peter A. R. Ade, D. Woolsey, M. Newcomb, W. L. Holzapfel, Chao-Lin Kuo, Carlo R. Contaldi, Dmitry Pogosyan, A. K. Romer, J. H. Goldstein, E. Torbet, J Ruhle, Christopher Cantalupo, Andrew E. Lange, J. R. Bond, J. J. Bock, J. B. Peterson, M. D. Daub, M. C. Runyan, Percy Gomez
Publikováno v:
NASA Astrophysics Data System
The Arcminute Cosmology Bolometer Array Receiver (Acbar) is a multifrequency millimeter-wave receiver optimized for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich (SZ) effect in clusters of galaxies. Acbar was instal
Autor:
J. H. Goldstein, M. C. Runyan, M. D. Daub, C. Cantalupo, E. Torbet, M. Lueker, W. L. Holzapfel, M. Newcomb, J. B. Peterson, Chao-Lin Kuo, P. A. R. Ade, James J. Bock, Andrew E. Lange, J. E. Ruhl
Publikováno v:
The Astrophysical Journal. 600:32-51
We report the first measurements of anisotropy in the cosmic microwave background (CMB) radiation with the Arcminute Cosmology Bolometer Array Receiver (ACBAR). The instrument was installed on the 2.1m Viper telescope at the South Pole in January 200
Autor:
M. D. Daub, C. Cantalupo, M. Newcomb, J. B. Peterson, J. E. Ruhl, D. Pogosyan, E. Torbet, Andrew E. Lange, Chao-Lin Kuo, P. A. R. Ade, James J. Bock, M. C. Runyan, W. L. Holzapfel, M. Lueker, J. R. Bond, Carlo R. Contaldi, J. H. Goldstein
Publikováno v:
The Astrophysical Journal. 599:773-785
We report an investigation of cosmological parameters based on the measurements of anisotropy in the cosmic microwave background radiation (CMB) made by ACBAR. We use the ACBAR data in concert with other recent CMB measurements to derive Bayesian est
Autor:
Jessie L. Dotson, M. Newcomb, David T. Chuss, Giles Novak, D. Pernic, T. Renbarger, R. F. Loewenstein, G. S. Griffin, J. B. Peterson
Publikováno v:
Proceedings of the Galactic Center Workshop 2002: The Central 300 parsecs of the Milky Way
We present new submillimeter polarimetric observations of the Galactic center region, made using the SPARO polarimeter that operates at the South Pole. Compared with previous submillimeter polarimetry of this region, our measurements cover much more
Autor:
David T. Chuss, M. Newcomb, D. Pernic, G. S. Griffin, R. F. Loewenstein, T. Renbarger, J. B. Peterson, Giles Novak, Jessie L. Dotson
Publikováno v:
The Astrophysical Journal. 583:L83-L86
We have observed the linear polarization of 450 micron continuum emission from the Galactic center, using a new polarimetric detector system that is operated on a 2 m telescope at the South Pole. The resulting polarization map extends ~ 170 pc along
Autor:
Gregory S. Tucker, Naoshi Sugiyama, G. S. Griffin, J. B. Peterson, Bharat Ratra, K. Ganga, H. T. Nguyen
Publikováno v:
The Astrophysical Journal. 505:8-11
We use data from the White Dish experiment to set limits on cosmic microwave background radiation anisotropies in open and spatially-flat-Lambda cold dark matter cosmogonies. We account for the White Dish calibration uncertainty, and marginalize over
Publikováno v:
The Astrophysical Journal. 475:L1-L4
The third year of observations with the Python microwave background experiment densely sample a $5.5^o\times 22^o$ region of sky that includes the fields measured during the first two years of observations with this instrument. The sky is sampled in