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;
2009-01-01

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.
2009
Pubblicato
Rilevanza internazionale
Articolo
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
Articolo su rivista
File in questo prodotto:
File Dimensione Formato  
84.pdf

accesso aperto

Dimensione 281.71 kB
Formato Adobe PDF
281.71 kB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/15639
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
social impact