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Overview of the L A M

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P.I. Chris Martin. All Sky Imaging Survey at 1530 (FUV) and 2315 (NUV) 20-21 ABmag ... Post-doc researcher (2 years at LAM 1 year at IAP): galex/swire/vvds data. ... – PowerPoint PPT presentation

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Title: Overview of the L A M


1
Overview of the L A M
  • Main research axes
  • Formation and evolution of galaxies, Cosmology
  • Interstellar medium
  • Extra-solar planets
  • Instrumental developments optics UV, visible,
    FIR, Ground based and spatial instrumentation
  • HST, ISO, GALEX, VIMOS, COROT, Herschel, TPF,
    SNAP, JWST, ELT

2
Research activities at LAM in relation with MAGPOP
  • Galaxy 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

3
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

4
MOUs between GALEX VVDS, GALEX SWIRE, VVDS
SWIRE, all the data are not public
5
GALEX measuring the star formation history from
z0 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

6
GALEX sensitivity
7
(No Transcript)
8
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 Iab22.5 covering 16 deg2
  • 1 deep field to Iab24 covering 1 deg2
  • (0ltzlt5)
  • Low resolution mode R230

9
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

10
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
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