Statistical simulations of the dust foreground to cosmic microwave background polarization (vol 603, A62, 2017)

被引：7
|
作者：
Vansyngel, F. [1 ]
Boulanger, F. [1 ]
Ghosh, T. [1 ,2 ]
Wandelt, B. [3 ,4 ,5 ]
Aumont, J. [1 ]
Bracco, A. [1 ,6 ]
Levrier, F. [7 ]
Martin, P. G. [8 ]
Montier, L. [9 ]
机构：
[1] Univ Paris Saclay, Univ Paris Sud, CNRS, Inst Astrophys Spatiale, Bat 121, F-91405 Orsay, France
[2] CALTECH, Pasadena, CA 91125 USA
[3] UPMC Univ Paris, Sorbonne Univ, 98 Bis Bd Arago, F-75014 Paris, France
[4] CNRS, UMR 7095, Inst Astrophys Paris, 98 Bis Bd Arago, F-75014 Paris, France
[5] Sorbonne Univ, ILP, 98 Bis Blvd Arago, F-75014 Paris, France
[6] Univ Paris Diderot, CEA Saclay, Lab AIM, IRFU,Serv Astrophys,CEA,DSM,CNRS, Bat 709, F-91191 Gif Sur Yvette, France
[7] UPMC Univ Paris 06, Sorbonne Univ, PSL Res Univ, LERMA,Observat Paris,CNRS,Ecole Normale Super, F-75005 Paris, France
[8] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada
[9] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France
来源：
ASTRONOMY & ASTROPHYSICS | 2018年 / 618卷
关键词：
polarization; ISM: general; comic background radiation; submillimeter: ISM; errata; addenda;
D O I：
10.1051/0004-6361/201629992e
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页数：1
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