DUSTYGAL
The formation of massive galaxies: the roles of dust-obscured starbursts and AGN activity
| Coordinatore | UNIVERSITY OF DURHAM
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
| # | ||||
|---|---|---|---|---|
| 1 |
UNIVERSITY OF DURHAM
Organization address
address: STOCKTON ROAD THE PALATINE CENTRE contact info |
UK (DURHAM) | hostInstitution | 2˙050˙123.00 |
| 2 |
UNIVERSITY OF DURHAM
Organization address
address: STOCKTON ROAD THE PALATINE CENTRE contact info |
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.'