P. Vielva   E. Martínez-González   F. J. Casas   T. Matsumura   S. Henrot-Versillé   E. Komatsu   J. Aumont   R. Aurlien   C. Baccigalupi   A. J. Banday   R. B. Barreiro   N. Bartolo   E. Calabrese   K. Cheung   F. Columbro   A. Coppolecchia   P. De Bernardis   T. De Haan   E. De La Hoz   M. De Petris   S. Della Torre   P. Diego-Palazuelos   H. K. Eriksen   J. Errard   F. Finelli   C. Franceschet   U. Fuskeland   M. Galloway   K. Ganga   M. Gervasi   R. T. Génova-Santos   T. Ghigna   E. Gjerløw   A. Gruppuso   M. Hazumi   D. Herranz   E. Hivon   K. Kohri   L. Lamagna   C. Leloup   J. Macias-Perez   S. Masi   F. T. Matsuda   G. Morgante   R. Nakano   F. Nati   P. Natoli   S. Nerval   K. Odagiri   S. Oguri   L. Pagano   A. Paiella   D. Paoletti   F. Piacentini   G. Polenta   G. Puglisi   M. Remazeilles   A. Ritacco   J. A. Rubino-Martin   D. Scott   Y. Sekimoto   M. Shiraishi   G. Signorelli   H. Takakura   A. Tartari   K. L. Thompson   M. Tristram   L. Vacher   N. Vittorio   I. K. Wehus   M. Zannoni   
Journal of Cosmology and Astroparticle Physics 2022(4) 2022年4月
A methodology to provide the polarization angle requirements for different sets of detectors, at a given frequency of a CMB polarization experiment, is presented. The uncertainties in the polarization angle of each detector set are related to a gi...
Miki Kurihara   Masahiro Tsujimoto   Megan E. Eckart   Caroline A. Kilbourne   Frederick T. Matsuda   Brian McLaughlin   Shugo Oguri   Frederick S. Porter   Yoh Takei   Yoichi Kochibe   
SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY 12181 2022年
Electromagnetic interference (EMI) for low-temperature detectors is a serious concern in many missions. We investigate the EMI caused by the spacecraft components to the x-ray microcalorimeter of the Resolve instrument onboard the X-Ray Imaging an...
SPACE TELESCOPES AND INSTRUMENTATION 2022: OPTICAL, INFRARED, AND MILLIMETER WAVE 12180 2022年
LiteBIRD is a JAXA-led international project that aims to test representative inflationary models by performing an all-sky cosmic microwave background radiation (CMB) polarization survey for 3 years at the Sun-Earth Lagrangian point L2. We aim to ...