3DLENS

3D spectroscopy of lensing cluster fields

 Coordinatore UNIVERSITE LYON 1 CLAUDE BERNARD 

 Organization address address: BOULEVARD DU 11 NOVEMBRE 1918 NUM43
city: VILLEURBANNE CEDEX
postcode: 69622

contact info
Titolo: Dr.
Nome: Javier
Cognome: Olaiz
Email: send email
Telefono: +33 4 72 69 76 00
Fax: +33 4 72 69 76 09

 Nazionalità Coordinatore France [FR]
 Totale costo 100˙000 €
 EC contributo 100˙000 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2011-CIG
 Funding Scheme MC-CIG
 Anno di inizio 2012
 Periodo (anno-mese-giorno) 2012-01-01   -   2015-12-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    UNIVERSITE LYON 1 CLAUDE BERNARD

 Organization address address: BOULEVARD DU 11 NOVEMBRE 1918 NUM43
city: VILLEURBANNE CEDEX
postcode: 69622

contact info
Titolo: Dr.
Nome: Javier
Cognome: Olaiz
Email: send email
Telefono: +33 4 72 69 76 00
Fax: +33 4 72 69 76 09

FR (VILLEURBANNE CEDEX) coordinator 100˙000.00

Mappa


 Word cloud

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

tenure    gravitational    physical       resolve    galaxy    position    pixel    galaxies    gt    alma    millimetre    lensed    distant    muse    facilities   

 Obiettivo del progetto (Objective)

'We propose to use new European astronomical facilities in conjunction with the power of massive galaxy clusters used as gravitational telescopes in order to explore the question of galaxy formation and evolution. In particular, new spectroimagers such as the Multi-Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope and the Atacama Large Millimetre Array (ALMA) allow to directly access and resolve the physical information inside distant galaxies on a pixel-to-pixel basis. The first part of the project will make use of MUSE to study the distribution, size, kinematics and physical properties of very distant galaxies (in particular at z>3), and the addition of gravitational lensing will bring these observations down to very faint luminosities. The second part of the project will characterize the multiwavelength properties of distant (z>1) galaxies, from optical to radio wavelengths, including a millimetre follow-up with ALMA. Only with the gravitational magnification in strongly lensed arcs will ALMA be able to already resolve different parts of high redshift galaxies during the Early Science phase. FInally, we will develop a dedicated software, called 3DLENS, in order to reconstruct the intrinsic properties of lensed sources observed with any spectroimager such as MUSE or ALMA. The proposed integration period will ensure that the researcher, who has just been hired as a tenure-track asssistant astronomer position, will access tenure position quickly in the institute. It will benefit his career as well as the scientific outcome of the European facilities mentioned.'

Altri progetti dello stesso programma (FP7-PEOPLE)

FIRST (2014)

"Fundamental investigations of high-resolution LA-ICPMS: Fast Imaging – Resolution, Sensitivity, and Time (FIRST)"

Read More  

EYEDEVELOPMENT (2009)

Molecular genetic regulation of eye field development

Read More  

AMSN (2007)

Adversarial Models in Sensor Networks

Read More