Corrigendum
Statistical simulations of the dust foreground to cosmic microwave background polarization (Corrigendum)
1
Institut d'Astrophysique Spatiale, CNRS, Université Paris-Sud, Université Paris-Saclay,
Bât. 121,
91405
Orsay Cedex,
France
2
California Institute of Technology,
Pasadena,
CA
91125,
USA
3
Sorbonne Universités, UPMC Université Paris 6 et CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98 bis bd Arago,
75014
Paris,
France
4
Sorbonne Universités, Institut Lagrange de Paris (ILP),
98 bis Boulevard Arago,
75014
Paris,
France
5
Laboratoire AIM, IRFU/Service d'Astrophysique, CEA/DSM, CNRS, Université Paris Diderot,
Bât. 709, CEA-Saclay,
91191
Gif-sur-Yvette Cedex,
France
6
LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Université Paris 06, Ecole normale supérieure,
75005,
Paris,
France
7
CITA, University of Toronto,
60 St. George St.,
Toronto,
ON M5S 3H8,
Canada
8
CNRS, IRAP,
9 Av. Colonel Roche, BP 44346,
31028
Toulouse Cedex 4,
France
Key words: polarization / ISM: general / comic background radiation / submillimeter: ISM / errata, addenda
The caption of Fig. 8 had a confusing description of the material shown in the plots. The correct caption together with the figure is given below.
© ESO 2018
All Figures
 |
Fig. 8 High-resolution power spectra on the LR63 region; simulation vs. data. From top to bottom: TE, EE; and BB power spectra of the Planck 353 GHz, CMB-corrected maps (red crosses), and one high-resolution (Nside = 2048, FWHM = 10') realization of the model (blue squares). |
| Open with DEXTER | |
| In the text | |