Archives Spectrophotométriques Publiques Intégrées au CeSAM

VUDS survey VUDS web site

The VIMOS Ultra Deep Survey Data Release 1 (DR1) is a public release of all spectroscopic data in the region of overlap between the CANDELS HST imaging survey and VUDS. The data release for 698 objects is distributed over the COSMOS-CANDELS field at around RA(2000)=10h00m28.2s, DEC(2000)=02deg21'36", and the ECDFS around RA(2000)=03h32m30s, DEC(2000)=-27deg48'00".

VVDS survey VVDS web site

The VIMOS VLT Deep Survey (VVDS) is a comprehensive deep galaxy spectroscopic redshift survey conducted by the VIMOS collaboration with the VIMOS multi-slit spectrograph at the ESO-VLT. The VVDS is a combination of 3 nested purely magnitude selected surveys: Wide (17.5 ≤ iAB ≤ 22.5; 8.6 deg²), Deep (17.5 ≤ iAB ≤ 24; 0.6 deg²), Ultra-Deep (23 ≤ iAB ≤ 24.75; 512 arcmin²), with a total of 22434, 12051, 1041 galaxies with measured redshifts in the range 0 < z < 6.7. The final catalog contains 35 016 galaxies and type-I AGN with measured spectroscopic redshifts covering all epochs up to redshift z ~ 6.7, as well as 12 430 Galactic stars, in areas from 0.142 to 8.7 square degrees, and volumes from 0.5 × 106 to 2 × 107 h-3 Mpc3. The release includes the 1D calibrated spectra, measured spectroscopic redshifts and their reliability, as well as all available photometric data matched to the VVDS targets.

zCOSMOS survey zCOSMOS web site

zCOSMOS is an approved Large Program on the ESO VLT. 600 hours of observation are used to carry out a major redshift survey with the VIMOS spectrograph on the COSMOS field to yield spectra for:

• approximately 28,000 galaxies at 0.2 < z < 1.2 selected to have I_AB < 22.5 at a sampling rate of 70%
• approximately 12,000 galaxies at 1.2 < z < 3 with B_AB < 25 and
• chosen by two colour-selection criteria (B-Z) vs. (Z-K) and (U-B) vs. (V-R) at a sampling rate of 70%

GAMA survey GAMA (DR3) web site

GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions.
Also based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 179.A-2004 & 177.A-3016.

Baldry et al. 2018, 2018MNRAS.474.3875B
Liske et al. 2015, 2015MNRAS.452.2087L

We completed GAMA data for the G02 field with LAM Y-band data described in:
Pipien et al. 2018, 2018A&A...616A..55P

6dF Galaxy survey 6dF web site

The third and final data release for the 6dF Galaxy Survey (6dFGS DR3) was made 1st April 2009. The survey comprises 125,071 galaxy redshifts.