/ftp/cats/J_other/MNRAS/414/28



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J/MNRAS/414/28      VLT LBG redshift survey. II.            (Crighton+, 2011)
The following files can be converted to FITS (extension .fit or fit.gz)
	tablec1.dat tablec3.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/414/28
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drwxr-xr-x 29 cats archive 4096 Mar 12 2018 [Up] drwxr-xr-x 3 cats archive 298 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 479 Dec 19 2022 .message -r--r--r-- 1 cats archive 6788 Aug 23 2014 ReadMe -rw-r--r-- 1 cats archive 472 Dec 20 2012 +footg5.gif -rw-r--r-- 1 cats archive 2450 Dec 20 2012 +footg8.gif -r--r--r-- 1 cats archive 23926 Nov 16 2012 tablec1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 9328 Jan 9 2012 tablec3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/MNRAS/414/28 VLT Lyman-break galaxy redshift survey. II. (Crighton+, 2011) ================================================================================ The VLT LBG redshift survey. II. Interactions between galaxies and the IGM at z   3. Crighton N.H.M., Bielby R., Shanks T., Infante L., Bornancini C.G., Bouche N., Lambas D.G., Lowenthal J.D., Minniti D., Morris S.L., Padilla N., Peroux C., Petitjean P., Theuns T., Tummuangpak P., Weilbacher P.M., Wisotzki L., Worseck G. <Mon. Not. R. Astron. Soc., 414, 28-49 (2011)> =2011MNRAS.414...28C ================================================================================ ADC_Keywords: QSOs ; Redshifts ; Equivalent widths Keywords: galaxies: high-redshift - intergalactic medium Abstract: We have measured redshifts for 243 z  3 quasars in nine Very Large Telescope (VLT) Visible Imaging and Multi-Object Spectrograph (VIMOS) Lyman-break galaxy (LBG) redshift survey areas, each of which is centred on a known bright quasar. Using the spectra of these quasars, we measure the cross-correlation between neutral hydrogen gas causing the Lyalpha forest and 1020 LBGs at z  3. Description: We obtained galaxy spectra for this project using the VIMOS multi-object spectrograph on the VLT.