用于宇宙学的 Q&U 测辐射热计 QUBIC 的现状
天体物理仪器与方法
2022-10-10 v1 宇宙学与河外天体物理
摘要
用于宇宙学的 Q&U 测辐射热干涉仪（QUBIC）是一种新型偏振计，专为测量宇宙微波背景（CMB）的 B 模偏振而优化，这是观测宇宙学的主要挑战之一。该信号预计为几十 nK 量级，易受仪器系统误差影响，并受到各种天体物理前景污染的干扰，只能通过多色观测加以控制。QUBIC 旨在通过一种新颖的方法解决这些观测问题，该方法将干涉仪在仪器系统误差控制方面的优势与测辐射热探测器在宽带、背景极限灵敏度方面的优势结合起来。
引用
@article{arxiv.2210.03161,
title = {Status of QUBIC, the Q&U Bolometer for Cosmology},
author = {L. Mousset and P. Ade and A. Almela and G. Amico and L. H. Arnaldi and J. Aumont and S. Banfi and E. S. Battistelli and B. Bélier and L. Bergé and J. -Ph. Bernard and P. de Bernardis and M. Bersanelli and J. Bonaparte and J. D. Bonilla and E. Bunn and D. Buzi and D. Camilieri and F. Cavaliere and P. Chanial and C. Chapron and S. Colombo and F. Columbro and A. Coppolecchia and B. Costanza and G. DÁlessandro and G. De Gasperis and M. De Leo and M. De Petris and N. Del Castillo and S. Dheilly and A. Etchegoyen and M. Famá and L. P. Ferreyro and C. Franceschet and M. M. Gamboa Lerena and K. M. Ganga and B. García and M. E. García Redondo and D. Gayer and J. M. Geria and M. Gervasi and M. Giard and V. Gilles and M. Gómez Berisso and M. González and M. Gradziel and L. Grandsire and J. -Ch. Hamilton and M. R. Hampel and G. Isopi and J. Kaplan and C. Kristukat and L. Lamagna and F. Lazarte and S. Loucatos and A. Mancilla and D. Mandelli and E. Manzan and S. Marnieros and W. Marty and S. Masi and A. May and J. Maya and M. McCulloch and L. Mele and D. Melo and A. Mennella and N. Mirón-Granese and L. Montier and N. Müller and J. D. Murphy and F. Nati and C. OŚullivan and A. Paiella and F. Pajot and S. Paradiso and A. Passerini and A. Pelosi and M. Perciballi and F. Pezzotta and F. Piacentini and M. Piat and L. Piccirillo and G. Pisano and M. Platino and G. Polenta and D. Prêle and D. Rambaud and E. Rasztocky and M. Régnier and C. Reyes and F. Rodríguez and C. A. Rodríguez and G. E. Romero and J. M. Salum and A. Schillaci and C. G. Scóccola and G. Stankowiak and A. D. Supanitsky and A. Tartari and J. -P. Thermeau and P. Timbie and S. A. Torchinsky and G. Tucker and C. Tucker and L. Vacher and F. Voisin and M. Wright and M. Zannoni and A. Zullo},
journal= {arXiv preprint arXiv:2210.03161},
year = {2022}
}
备注
Contribution to the 2022 Cosmology session of the 33rd Rencontres de Blois. arXiv admin note: substantial text overlap with arXiv:2203.08947