/ftp/cats/V/151



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V/151               VANDELS High-Redshift Galaxy Evolution       (McLure+, 2017)
The following files can be converted to FITS (extension .fit or fit.gz)
	cdfs.dat uds.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=V/151
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drwxr-xr-x 146 cats archive 4096 Aug 1 2023 [Up] drwxr-xr-x 3 cats archive 336 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 466 Dec 19 2022 .message -r--r--r-- 1 cats archive 6355 May 2 2018 ReadMe -rw-r--r-- 1 cats archive 1013 Jun 15 2020 +footg5.gif -rw-r--r-- 1 cats archive 3039 Jun 15 2020 +footg8.gif -r--r--r-- 1 cats archive 67645 Nov 27 2017 cdfs.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 75632 Nov 27 2017 uds.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2395406 Nov 21 2017 vandels_release_doc_110917_v4.pdf
Beginning of ReadMe : V/151 VANDELS High-Redshift Galaxy Evolution (McLure+, 2017) ================================================================================ VANDELS High-Redshift Galaxy Evolution: Spectroscopic and Photometric Redshifts in the CANDELS UDS and CDFS Fields McLure R., Pentericci L., VANDELS Team <The Messenger, vol. 167, 31-35 (2017)> =2017Msngr.167...31M =2017yCat.5151....0M ================================================================================ ADC_Keywords: Surveys ; Photometry, SDSS ; Photometry, infrared ; Redshifts Mission_Name: ESO Abstract: VANDELS is a new ESO spectroscopic Public Survey targeting the high-redshift Universe. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the survey is obtaining ultra-deep optical spectroscopy of around 2100 galaxies in the redshift interval 1.0<z<7.0, with 85% of its targets selected to be at z>=3. The fundamental aim of the survey is to provide the high signal-to-noise spectra necessary to measure key physical properties such as stellar population ages, metallicities and outflow velocities from detailed absorption-line studies. By targeting two extragalactic survey fields with superb multi-wavelength imaging data, VANDELS will produce a unique legacy dataset for exploring the physics underpinning high-redshift galaxy evolution. Description: This is the first data release (DR1) of the VANDELS survey, an ESO public spectroscopy survey targeting the high-redshift Universe. The VANDELS survey uses the VIMOS spectrograph on ESO's VLT to obtain ultra-deep, medium resolution, optical spectra of galaxies within the UKIDSS Ultra Deep Survey (UDS) and Chandra Deep Field South (CDFS) survey fields (0.2 sq. degree total area). Using robust photometric redshift pre-selection, VANDELS is targeting  2100 galaxies in the redshift interval 1.0<z<7.0, with 85% of its targets selected to be at z>=3. In addition, VANDELS is targeting a substantial number of passive galaxies in the redshift interval 1.0<z<2.5. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the survey is obtaining ultra-deep optical spectroscopy with the VIMOS MR grism and GG475 order-sorting filter, which covers the wavelength range 4800-10000AA at a dispersion of 2.5AA/pix and a spectral resolution of R 600. Each galaxy receives between a minimum of 20-hours and a maximum of 80-hours of on-source integration time. The fundamental aim of the survey is to provide the high signal-to-noise spectra necessary to measure key physical properties such as stellar population ages, metallicities and outflow velocities from detailed absorption-line studies. By targeting two extra-galactic survey fields with superb multi-wavelength imaging data, VANDELS is designed to produce a unique legacy dataset for exploring the physics underpinning high-redshift galaxy evolution.