PASCAL

Probabilistic And Statistical methods for Cosmological AppLications

Coordinatore	UNIVERSITA DEGLI STUDI DI ROMA TOR VERGATA    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	Italy [IT]
Totale costo	1˙193˙000 €
EC contributo	1˙193˙000 €
Programma	FP7-IDEAS-ERC Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	ERC-2011-StG_20101014
Funding Scheme	ERC-SG
Anno di inizio	2011
Periodo (anno-mese-giorno)	2011-11-01   -   2016-10-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	UNIVERSITA DEGLI STUDI DI ROMA TOR VERGATA  Organization address address: VIA ORAZIO RAIMONDO 18 city: ROMA postcode: 173 contact info Titolo: Prof. Nome: Domenico Cognome: Marinucci Email: send email Telefono: 390673000000 Fax: 390673000000	IT (ROMA)	hostInstitution	1˙193˙000.00
2	UNIVERSITA DEGLI STUDI DI ROMA TOR VERGATA  Organization address address: VIA ORAZIO RAIMONDO 18 city: ROMA postcode: 173 contact info Titolo: Prof. Nome: Giuseppe Cognome: Novelli Email: send email Telefono: 390673000000 Fax: 39067236605	IT (ROMA)	hostInstitution	1˙193˙000.00

Mappa

 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

 Obiettivo del progetto (Objective)

'This is an interdisciplinary project at the interface between Mathematical Statistics, Probability and Cosmological Applications. The principal focus is on the harmonic analysis for isotropic, mean square continuous spherical random fields, with a view to applications to Cosmic Microwave Background radiation data analysis. We will focus in particular on the following issues: 1) the characterizations of isotropy in harmonic space, the analysis of higher order polyspectra and their applications to non-Gaussianity analysis; 2) the constructions of spherical needlets/wavelets and their stochastic properties; 3) the analysis of random sections of spin fiber bundles on the sphere, as motivated by the analysis of CMB polarization and weak gravitational lensing 4) adaptive density estimation for directional data, as motivated by Cosmic Rays data analysis.'