The field of Cosmic Microwave Background (CMB) data analysis is a smashing source of computational problems. Here we discuss the ROMA map making code. Originally designed to generate a map of the CMB anisotropy and polarization fields using optimal statistical methods, ROMA can be applied also to other microwave oriented surveys. The computational details of the subject will be set forth.

Natoli, P., Botti, M., DE GASPERIS, G., DE TROIA, G., & Massaioli, F. (2009). The GLS approach to CMB map making, 13, 84.

The GLS approach to CMB map making.

NATOLI, PAOLO;DE GASPERIS, GIANCARLO;DE TROIA, GRAZIA;
2009

Abstract

The field of Cosmic Microwave Background (CMB) data analysis is a smashing source of computational problems. Here we discuss the ROMA map making code. Originally designed to generate a map of the CMB anisotropy and polarization fields using optimal statistical methods, ROMA can be applied also to other microwave oriented surveys. The computational details of the subject will be set forth.
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Rilevanza internazionale
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Nessuno
Settore FIS/05 - Astronomia e Astrofisica
English
Con Impact Factor ISI
Natoli, P., Botti, M., DE GASPERIS, G., DE TROIA, G., & Massaioli, F. (2009). The GLS approach to CMB map making, 13, 84.
Natoli, P; Botti, M; DE GASPERIS, G; DE TROIA, G; Massaioli, F
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/2108/15639
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