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J/A+A/512/A12 VLT/VIMOS spectroscopy in GOODS-South field (Balestra+, 2010)
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Beginning of ReadMe :J/A+A/512/A12 VLT/VIMOS spectroscopy in GOODS-South field (Balestra+, 2010)
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The Great Observatories Origins Deep Survey.
VLT/VIMOS spectroscopy in the GOODS-South field: part II.
Balestra I., Mainieri V., Popesso P., Dickinson M., Nonino M., Rosati P.,
Teimoorinia H., Vanzella E., Cristiani S., Cesarsky C., Fosbury R.A.E.,
Kuntschner H., Rettura A.
<Astron. Astrophys., 512, A12-12 (2010)>
=2010A&A...512A..12B
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ADC_Keywords: Surveys ; Galaxies, photometry ; Redshifts ; Spectroscopy
Keywords: large scale structure of Universe - catalogs - surveys -
galaxies: evolution - galaxies: high-redshift -
cosmology: observations
Abstract:
We present the full data set of the VIsible Multi-Object Spectrograph
(VIMOS) spectroscopic campaign of the ESO/GOODS program in the Chandra
Deep Field South (CDFS), which complements the FORS2 ESO/GOODS
spectroscopic campaign.
The ESO/GOODS spectroscopic programs are aimed at reaching
signal-to-noise ratios adequate to measure redshifts for galaxies with
AB magnitudes in the range 24-25 in the B and R band using VIMOS, and
in the z band using FORS2.
Description:
The GOODS/VIMOS spectroscopic campaign is structured in two separate
surveys using two different VIMOS grisms. The VIMOS Low Resolution
Blue (LR-Blue) and Medium Resolution (MR) orange grisms have been used
to cover different redshift ranges. The LR-Blue campaign is aimed at
observing galaxies mainly at 1.8<z<3.5, while the MR campaign mainly
aims at galaxies at z<1 and Lyman Break Galaxies (LBGs) at z>3.5.