/ftp/cats/A+A/417/499



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J/A+A/417/499       Spectrophotometry of Virgo cluster galaxies (Gavazzi+, 2004)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table6.dat table7.dat table8.dat table9.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/417/499
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drwxr-xr-x 20 cats archive 4096 Jan 14 2013 [Up] drwxr-xr-x 3 cats archive 4096 Feb 2 2023 [TAR file] -rw-r--r-- 1 cats archive 504 Dec 19 2022 .message -r--r--r-- 1 cats archive 11015 Jun 26 2004 ReadMe -rw-r--r-- 1 cats archive 528 Apr 16 2018 +footg5.gif -rw-r--r-- 1 cats archive 2854 Apr 16 2018 +footg8.gif drwxr-xr-x 2 cats archive 12288 May 4 2004 spectra -r--r--r-- 1 cats archive 43405 Jun 26 2004 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 54946 Feb 10 2004 table7.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 14233 Feb 10 2004 table8.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2924 Feb 10 2004 table9.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 924400 Feb 10 2004 vccspec_2.ps.gz [Uncompressed]
Beginning of ReadMe : J/A+A/417/499 Spectrophotometry of Virgo cluster galaxies (Gavazzi+, 2004) ================================================================================ Spectrophotometry of galaxies in the Virgo cluster. II: The data. Gavazzi G., Zaccardo A., Sanvito G., Bonfanti C., Boselli A. <Astron. Astrophys. 417, 499 (2004)> =2004A&A...417..499G ================================================================================ ADC_Keywords: Clusters, galaxy ; Galaxies, spectra ; Galaxies, photometry Keywords: galaxies: clusters: individual: Virgo - techniques: spectroscopic - catalogs Abstract: Drift-scan mode (3600-6800AA) spectra with 500<R<1000 resolution are presented for 333 galaxies members to nearby clusters, covering the whole Hubble sequence. The majority (225) were obtained for galaxies in the Virgo cluster where a completeness of 36%, if all Hubble types are considered, and of 5 %, restricting to late-types, was reached at mp<=16. Our data can be therefore considered representative of the integrated spectral properties of giant and dwarf galaxies in this cluster. Intensities and equivalent widths (EWs) are derived for the principal lines, both in emission and in absorption. Deblending of the underlying absorption from emission was achieved in most cases. Description: Long-slit spectra of 333 galaxies, obtained during approximately 50 nights distributed in 6 years (1998-2003) using the 1.93m telescope of the Observatoire de Haute Provence (OHP), the ESO 3.6m telescope, the Loiano 1.52m telescope and the San Pedro Martir (SPM) 2.1m telescope are presented. The observations were taken in the "drift-scan" mode, i.e. with the slit, generally parallel to the galaxy major axis, drifting over the optical surface of the galaxy.