The Cosmology Large Angular Scale Surveyor (CLASS) Telescope Architecture

We describe the instrument architecture of the Johns Hopkins University-led CLASS instrument, a groundbased cosmic microwave background (CMB) polarimeter that will measure the large-scale polarization of the CMB in several frequency bands to search for evidence of inflation.

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Bibliographische Detailangaben
Hauptverfasser:	Chuss, David T., Ali, Aamir, Amiri, Mandana, Appel, John W., Araujo, Derek, Bennett, Charles L., Boone, Fletcher, Chan, Manwei, Cho, Hsiao-Mei, Colazo, Felipe, Crowe, Erik, Denis, Kevin L., Dunner, Rolando, Eimer, Joseph, Essinger-Hileman, Thomas, Gothe, Dominik, Halpern, Mark, Harrington, Kathleen, Hilton, Gene, Hinshaw, Gary F., Huang, Caroline, Irwin, Kent, Jones, Glenn, Karakla, John, Kogut, Alan J., Larson, David, Limon, Michele, Lowry, Lindsay, Marriage, Tobias, Mehrle, Nicholas, Stevenson, Thomas, Miller, Nathan J., Moseley, Samuel H., U-Yen, Kongpop, Wollack, Edward
Format:	Tagungsbericht
Sprache:	eng
Schlagworte:	Astrophysics
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Beschreibung
Zusammenfassung:	We describe the instrument architecture of the Johns Hopkins University-led CLASS instrument, a groundbased cosmic microwave background (CMB) polarimeter that will measure the large-scale polarization of the CMB in several frequency bands to search for evidence of inflation.