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J/A+A/448/893 Photometry and lines of (z 0.2-1.0) galaxies (Lamareille+, 2006)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
objects.dat 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/448/893
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drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 516 Dec 19 2022 .message
-r--r--r-- 1 cats archive 12021 May 31 2006 ReadMe
-rw-r--r-- 1 cats archive 469 Sep 19 2007 +footg5.gif
-rw-r--r-- 1 cats archive 2535 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 7755 May 6 2006 objects.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 13395 Nov 22 2005 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 3666 Nov 22 2005 table7.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 17625 Nov 22 2005 table8.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 17766 Nov 22 2005 table9.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/A+A/448/893 Photometry and lines of (z 0.2-1.0) galaxies (Lamareille+, 2006)
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Spectrophotometric properties of galaxies at intermediate redshifts (z 0.2-1.0).
I. Sample description, photometric properties and spectral measurements.
Lamareille F., Contini T., Le Borgne J.-F., Brinchmann J., Charlot S.,
Richard J.
<Astron. Astrophys. 448, 893 (2006)>
=2006A&A...448..893L
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ADC_Keywords: Galaxies, photometry ; Photometry, UBVRI ; Photometry, ugriz ;
Spectroscopy ; Redshifts
Keywords: galaxies: abundances - galaxies: evolution -
galaxies: fundamental parameters - galaxies: starburst
Abstract:
We present the spectrophotometric properties of a sample of 141
emission-line galaxies at redshifts in the range 0.2<z<1.0 with a peak
around 0.2<=z<=0.4. The analysis is based on medium resolution
(Rs=500-600), optical spectra obtained at VLT and Keck. The targets
are mostly "Canada-France Redshift Survey" (VII/225) emission-line
galaxies, with the addition of field galaxies randomly selected behind
lensing clusters. We complement this sample with galaxy spectra from
the "Gemini Deep Deep Survey" (J/AJ/127/2455) public data release.
We have computed absolute magnitudes of the galaxies and measured the
line fluxes and equivalent widths of the main emission/absorption
lines. The last two have been measured after careful subtraction of
the fitted stellar continuum using the platefit software originally
developed for the SDSS and adapted to our data. We present a careful
comparison of this software with the results of manual measurements.