Jeffery D. Childers, Ph.D. - Publications

Affiliations: 
2006 University of California, Santa Barbara, Santa Barbara, CA, United States 
Area:
Astrophysics and Cosmology

3/5 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2008 Levy AR, Leonardi R, Ansmann M, Bersanelli M, Childers J, Cole TD, D'Arcangelo O, Davis GV, Lubin PM, Marvil J, Meinhold PR, Miller G, O'Neill H, Stavola F, Stebor NC, et al. The White Mountain Polarimeter telescope and an upper limit on cosmic microwave background polarization Astrophysical Journal, Supplement Series. 177: 419-430. DOI: 10.1086/588784  0.36
2005 Childers J, Bersanelli M, Figueiredo N, Gaier TC, Halevi D, Kangas M, Levy A, Lubin PM, Malaspina M, Mandolesi N, Marvil J, Meinhold PR, Mejía J, Natoli P, O'Neill H, et al. The background Emission Anisotropy Scanning Telescope (BEAST) instrument description and performances Astrophysical Journal, Supplement Series. 158: 124-138. DOI: 10.1086/429092  0.36
2000 Tegmark M, De Oliveira-Costa A, Staren JW, Meinhold PR, Lubin PM, Childers JD, Figueiredo N, Gaier T, Lim MA, Seiffert MD, Villela T, Wuensche CA. Cosmic microwave background maps from the HACME experiment Astrophysical Journal. 541: 535-541. DOI: 10.1086/309442  0.36
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2005 Figueiredo N, Bersanelli M, Childers J, D’Arcangelo O, Halevi D, Janssen M, Kedward K, Lemaster N, Lubin P, Mandolesi N, Marvil J, Meinhold P, Mejia J, Mennella A, Natoli P, et al. The Optical Design of the Background Emission Anisotropy Scanning Telescope (BEAST) The Astrophysical Journal Supplement Series. 158: 118-123. DOI: 10.1086/429091  0.01
1985 Duvvury C, Childers JD. INSIGHT INTO A DYNAMIC RANDOM ACCESS MEMORY Journal of the Institution of Engineers. India. Electronics and Telecommunication Engineering Division. 66: 1-9.  0.01
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