Modeling and characterization of the SPIDER half-wave plate
Modeling and characterization of the SPIDER half-wave plate
复制标题
SPIDER 半波片的建模和表征
DOI:
10.1117/12.857837
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发表时间:
2010
期刊:
影响因子:
--
通讯作者:
Bryan S
中科院分区:
文献类型:
--
作者:
Bryan S
Spider is a balloon-borne array of six telescopes that will observe the Cosmic Microwave Background. The 2624 antenna-coupled bolometers in the instrument will make a polarization map of the CMB with approximately one-half degree resolution at 145 GHz. Polarization modulation is achieved via a cryogenic sapphire half-wave plate (HWP) skyward of the primary optic. We have measured millimeter-wave transmission spectra of the sapphire at room and cryogenic temperatures. The spectra are consistent with our physical optics model, and the data gives excellent measurements of the indices of A-cut sapphire. We have also taken preliminary spectra of the integrated HWP, optical system, and detectors in the prototype Spider receiver. We calculate the variation in response of the HWP between observing the CMB and foreground spectra, and estimate that it should not limit the Spider constraints on inflation.
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影响因子:
1.9
作者:
G. Savini;G. Pisano;P. Ade
通讯作者:
G. Savini;G. Pisano;P. Ade
影响因子:
6.4
作者:
J. Filippini;P. Ade;M. Amiri;S. Benton;R. Bihary;J. Bock;J. Bock;J. Bond;J. A. Bonetti;S. Bryan;B. Burger;H. Chiang;C. Contaldi;B. Crill;O. Doré;O. Doré;M. Farhang;L. Fissel;N. Gandilo;S. Golwala;J. Gudmundsson;M. Halpern;M. Hasselfield;G. Hilton;W. Holmes;V. Hristov;K. Irwin;W. Jones;C. Kuo;C. MacTavish;P. Mason;T. Montroy;T. Morford;C. Netterfield;D. O'Dea;A. Rahlin;C. Reintsema;J. Ruhl;M. Runyan;M. Schenker;J. Shariff;J. Soler;A. Trangsrud;C. Tucker;R. Tucker;A. Turner
通讯作者:
A. Turner
DOI:
10.1117/12.787446
发表时间:
2008-07
期刊:
--
影响因子:
--
作者:
B. Crill;P. Ade;E. Battistelli;S. Benton;R. Bihary;J. Bock;J. Bock;J. Bond;J. Brevik;S. Bryan;C. Contaldi;O. Doré;M. Farhang;L. Fissel;S. Golwala;M. Halpern;G. Hilton;W. Holmes;V. Hristov;K. Irwin;W. Jones;W. Jones;C. Kuo;A. Lange;C. Lawrie;C. MacTavish;T. G. Martin;P. Mason;T. Montroy;C. Netterfield;E. Pascale;D. Riley;J. Ruhl;M. Runyan;A. Trangsrud;C. Tucker;A. Turner;M. Viero;D. Wiebe
通讯作者:
B. Crill;P. Ade;E. Battistelli;S. Benton;R. Bihary;J. Bock;J. Bock;J. Bond;J. Brevik;S. Bryan;C. Contaldi;O. Doré;M. Farhang;L. Fissel;S. Golwala;M. Halpern;G. Hilton;W. Holmes;V. Hristov;K. Irwin;W. Jones;W. Jones;C. Kuo;A. Lange;C. Lawrie;C. MacTavish;T. G. Martin;P. Mason;T. Montroy;C. Netterfield;E. Pascale;D. Riley;J. Ruhl;M. Runyan;A. Trangsrud;C. Tucker;A. Turner;M. Viero;D. Wiebe
DOI:
10.1117/12.857715
发表时间:
2010
期刊:
--
影响因子:
--
作者:
Runyan M
通讯作者:
Runyan M
DOI:
10.1117/12.857925
发表时间:
2010
期刊:
Astronomical Telescopes + Instrumentation
影响因子:
--
作者:
J. Gudmundsson;P. Ade;M. Amiri;S. Benton;R. Bihary;J. Bock;J. Bond;J. A. Bonetti;S. Bryan;B. Burger;H. Chiang;C. Contaldi;B. Crill;O. Doré;M. Farhang;J. Filippini;L. Fissel;N. Gandilo;S. Golwala;M. Halpern;M. Hasselfield;G. Hilton;W. Holmes;V. Hristov;K. Irwin;W. Jones;C. Kuo;C. MacTavish;P. Mason;T. Montroy;T. Morford;C. Netterfield;D. O'Dea;A. Rahlin;C. Reintsema;J. Ruhl;M. Runyan;M. Schenker;J. Shariff;J. Soler;A. Trangsrud;C. Tucker;R. Tucker;A. Turner
通讯作者:
A. Turner