Overview of the L A MMain research axes:• Formation and evolution of galaxies, Cosmology• Interstellar medium• Extra-solar planetsInstrumental developments: optics: UV, visible,

FIR, Ground based and spatial instrumentation

HST, ISO, GALEX, VIMOS, COROT, Herschel, TPF, SNAP, JWST, ELT

Research activities at LAM in relation with

MAGPOPGalaxy Evolution, Observational Cosmology~20 permanent researchers+PhD students & post-docs

Involved in MAGPOP: V.Buat, L. Tresse, S. Arnouts, A. Boselli, D Burgarella , J. Iglesias (LAM associate researcher) & M. Treyer

Research topics (overview)Physical properties of galaxies: spectral energy distributions, star

formation, dust attenuation, environmental effects etc…Statistical studies: number counts, photo-z, morphology, luminosity

functions, luminosity densities, correlation functions etc…

Expertise in data analysis

• Spectroscopic analyses, diagnostics• Multi-wavelength imaging: UV-opt-FIR• Redshift determinations: Zspec, Zphot• Luminosity functions and densities• Environment, clustering, correlation functions• Modeling: SFR,SFH, dust attenuation• Morphological analysis

In rela tion w ith MAG PO P: Spectra l Energy D istributions of ga la xies:evolution w ith z

SDSS2dF

Goldm ine

SW IRENIR & FIR

IRASFIR

ASTRO-F

GALEXFUV(1530A)NUV(2310A)

spectroscopic m ode

XM M VLA

SW IRENIR & FIR

VVDSUBVRI photom etry

visible spectroscopy

M ulti-w avelength analysis

MOUs between GALEX & VVDS, GALEX & SWIRE, VVDS & SWIRE, all the data are not public

GALEX: measuring the star formation history from z~0 to 1-2

(in UV)P.I. Chris Martin

All Sky Imaging Survey at 1530 Å (FUV) and 2315

Å (NUV)

20-21 ABmag

Deep Imaging Surveys (few hundreds deg2)

25.5 ABmag

Spectroscopic mode: 1300-3000 Å

Data are becoming public…

GALEX sensitivity

VVDS: VIMOS VLT Deep Survey

• PI: O. Le Fevre • Franco-italian consortium• Wide and Deep photometric and I selected

spectroscopic surveys • 4 wide fields to Iab=22.5 covering 16 deg2• 1 deep field to Iab=24 covering 1 deg2 (0<z<5) Low resolution mode : R~230

Current multi- analyses at LAM: GALEX, VVDS (and IRAS

& SWIRE)

Short presentations• Luminosity functions and densities Laurence Tresse

• Deep fields: UV-vis-NIR Stephane Arnouts

• SED analyses

UV-FIR Jorge Iglesias/ Véronique Buat

SED modeling Denis Burgarella/Véronique Buat

local universe, environment Alessandro Boselli

Within/in relation with MAGPOP

• Post-doc researcher (2 years at LAM+ 1 year at IAP): galex/swire/vvds data. SED analysis and modeling.

• SED analyses from low to hi z focusing on UV/FIR emission: SED/modeling

• Improving Zphot with new SEDs