DUSTYGAL

The formation of massive galaxies: the roles of dust-obscured starbursts and AGN activity

Coordinatore	UNIVERSITY OF DURHAM    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	United Kingdom [UK]
Totale costo	2˙050˙123 €
EC contributo	2˙050˙123 €
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-2012-ADG_20120216
Funding Scheme	ERC-AG
Anno di inizio	2013
Periodo (anno-mese-giorno)	2013-01-01   -   2017-12-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	UNIVERSITY OF DURHAM  Organization address address: STOCKTON ROAD THE PALATINE CENTRE city: DURHAM postcode: DH1 3LE contact info Titolo: Ms. Nome: Wendy Cognome: Harle Email: send email Telefono: +44 191 3344635 Fax: +44 191 3344634	UK (DURHAM)	hostInstitution	2˙050˙123.00
2	UNIVERSITY OF DURHAM  Organization address address: STOCKTON ROAD THE PALATINE CENTRE city: DURHAM postcode: DH1 3LE contact info Titolo: Prof. Nome: Ian Robert Cognome: Smail Email: send email Telefono: +44 191 3343605 Fax: +44 1913343645	UK (DURHAM)	hostInstitution	2˙050˙123.00

Mappa

 Word cloud

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 Obiettivo del progetto (Objective)

'I propose an integrated programme to determine the role of dust-obscured starburst activity and AGN growth in the formation and evolution of galaxies. This programme will exploit three, new cutting-edge observational facilities: the SCUBA-2 submillimetre camera, which will provide the first panoramic surveys of luminous, but highly obscured, sources out to the highest redshifts; the Atacama Large Millimeter Array (ALMA), which will provide sub-kpc imaging of the distribution of dust and gas within these sources to understand the physics of their activity; the e-MERLIN radio telescope, which will map the distribution of star formation and AGN activity at sub-kpc scales in these systems. I lead major international surveys on all three facilities and I propose to develop and combine these projects to provide a single focused programme to understand the processes which trigger obscured activity at high redshifts and their role in determining the properties of galaxies at the present day.'