LOFARCORE

Unravelling the Cosmic Reionization History

Coordinatore	"STICHTING ASTRON, NETHERLANDS INSTITUTE FOR RADIO ASTRONOMY"    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	Netherlands [NL]
Totale costo	3˙348˙468 €
EC contributo	3˙348˙468 €
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-2013-ADG
Funding Scheme	ERC-AG
Anno di inizio	2014
Periodo (anno-mese-giorno)	2014-04-01   -   2019-03-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	RIJKSUNIVERSITEIT GRONINGEN  Organization address address: Broerstraat 5 city: GRONINGEN postcode: 9712CP contact info Titolo: Dr. Nome: Dick Cognome: Veldhuis Email: send email Telefono: +31 50 363 4142	NL (GRONINGEN)	beneficiary	1˙012˙006.80
2	"STICHTING ASTRON, NETHERLANDS INSTITUTE FOR RADIO ASTRONOMY"  Organization address address: Oude Hoogeveensedijk 4 city: DWINGELOO postcode: 7991PD contact info Titolo: Mrs. Nome: Janneke Cognome: Wubs-Komdeur Email: send email Telefono: 31521595224 Fax: 31521595101	NL (DWINGELOO)	hostInstitution	2˙336˙461.20
3	"STICHTING ASTRON, NETHERLANDS INSTITUTE FOR RADIO ASTRONOMY"  Organization address address: Oude Hoogeveensedijk 4 city: DWINGELOO postcode: 7991PD contact info Titolo: Prof. Nome: Antonius Gerardus Cognome: De Bruyn Email: send email Telefono: 31521595100 Fax: 31521595101	NL (DWINGELOO)	hostInstitution	2˙336˙461.20

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 Obiettivo del progetto (Objective)

'One of the frontier cosmological research themes of the past decade has been the Epoch of Reionization (EoR). This era marked the start of the formation of visible baryonic structures: stars, (dwarf-)galaxies, clusters and the cosmic web. Some top level questions surrounding COsmic REionization are: 'When did it start ?”, “How long did it take ?”, “What were the main ionizing sources ?”, and “What did the Universe look like during this crucial evolutionary phase ?' Simulations of reionization suggest how it may have proceeded, but hard observational facts on the EoR are few and far between. At the start of the EoR all hydrogen was cold and neutral. At redshift z=6 the transition to an ionized Universe was completed. The 21cm line, redshifted to much longer wavelength, is a key diagnostic during this phase. LOFAR, the European LOw Frequency Array, will be the premier instrument to explore this epoch, simultaneously over the full redshift range from z=6.5-11.5 ! The required angular resolution is also well matched to the 2.5 km CORE of LOFAR. Detecting redshifted HI from the EoR is generally acknowledged as the most difficult radio astronomical project ever attempted. As PI of the LOFAR EoR Key Science Project and as LOFAR Calibration Project scientist, I have worked hard for 10 years to prepare LOFAR and myself for this endeavour. In November 2012 LOFAR commenced a long (> 3-5 years) observing campaign, generating several PB of data per year. A new phase, with extraordinary challenges, still lies ahead. ERC funding for the LOFARCORE team will permit me to ramp up the execution of this program, and in a timely manner (we have competition from US, Australian and Indian groups), solve problems along the way, and analyze and publish what will be ground-breaking results on the COsmic REionization history. The LOFAR EoR project will be the pathfinder for even more daunting future explorations, using SKA, of the phases preceeding the EoR, i.e. Cosmic Dawn.'