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The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters
Autor:
Appel, John W., Ali, Aamir, Amiri, Mandana, Araujo, Derek, Bennett, Charles L., Boone, Fletcher, Chan, Manwei, Cho, Hsiao-Mei, Chuss, David T., Colazo, Felipe, Crowe, Erik, Denis, Kevin, 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, Miller, Amber D., Miller, Nathan, Moseleyb, Samuel H., Novakh, Giles, Reintsemad, Carl, Rostemab, Karwan, Stevensonb, Thomas, Towner, Deborah, U-Yen, Kongpop, Wagner, Emily, Watts, Duncan, Wollack, Edward, Xu, Zhilei, Zeng, Lingzhen
The Cosmology Large Angular Scale Surveyor (CLASS) experiment aims to map the polarization of the Cosmic Microwave Background (CMB) at angular scales larger than a few degrees. Operating from Cerro Toco in the Atacama Desert of Chile, it will observe
Externí odkaz:
http://arxiv.org/abs/1408.4789
