Samantha F. Edgington, Ph.D.
Affiliations: | 2004 | California Institute of Technology, Pasadena, CA |
Area:
cosmic microwave backgroundGoogle:
"Samantha Edgington"Mean distance: 14.8 | S | N | B | C | P |
Parents
Sign in to add mentorAndrew Evan Lange | grad student | 2004 | Caltech | |
(A galaxy cluster survey using the Sunyaev Zel'dovich effect.) |
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Publications
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Sayers J, Golwala SR, Ade PAR, et al. (2010) Studies of millimeter-wave atmospheric noise above mauna kea Astrophysical Journal. 708: 1674-1691 |
Sayers J, Golwala SR, Rossinot P, et al. (2009) ERRATUM: “A SEARCH FOR COSMIC MICROWAVE BACKGROUND ANISOTROPIES ON ARCMINUTE SCALES WITH BOLOCAM” (2009, ApJ, 690, 1597) The Astrophysical Journal. 692: 942-942 |
Sayers J, Golwala SR, Rossinot P, et al. (2009) A search for cosmic microwave background anisotropies on arcminute scales with bolocam Astrophysical Journal. 690: 1597-1620 |
Sayers J, Golwala SR, Ade PAR, et al. (2008) Studies of atmospheric noise on Mauna Kea at 143 GHz with Bolocam Proceedings of Spie - the International Society For Optical Engineering. 7020 |
MaLoney PR, Glenn J, Aguirre JE, et al. (2005) A fluctuation analysis of the Bolocam 1.1 mm Lockman Hole Survey Astrophysical Journal. 635: 1044-1052 |
Haig DJ, Ade PAR, Aguirre JE, et al. (2004) Bolocam: Status and observations Proceedings of Spie - the International Society For Optical Engineering. 5498: 78-94 |
Glenn J, Chattopadhyay G, Edgington SF, et al. (2002) Numerical optimization of integrating cavities for diffraction-limited millimeter-wave bolometer arrays. Applied Optics. 41: 136-42 |
Glenn J, Ade PAR, Amarie M, et al. (2002) Current status of Bolocam: A large-format millimeter-wave bolometer camera Proceedings of Spie - the International Society For Optical Engineering. 4855: 30-40 |
Bhatia RS, Chase ST, Edgington SF, et al. (2000) A three-stage helium sorption refrigerator for cooling of infrared detectors to 280 mK Cryogenics. 40: 685-691 |
Glenn J, Bock JJ, Chattopadhyay G, et al. (1998) Bolocam: A millimeter-wave bolometric camera Proceedings of Spie - the International Society For Optical Engineering. 3357: 326-334 |