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VII/184 Survey of 108 E-S0 galaxies (Michard+, 1993-94)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
rsafram rsamorp rsaphot rsamuls1 rsamuls2 rsamuls3 rsamuls4 rsaresu1
rsaresu2
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VII/184
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drwxr-xr-x 257 cats archive 8192 Feb 8 10:28 [Up]
drwxr-xr-x 3 cats archive 4096 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 526 Dec 19 2022 .message
-r--r--r-- 1 cats archive 18473 Aug 23 2017 ReadMe
-rw-r--r-- 1 cats archive 596 Aug 23 2017 +footg5.gif
-rw-r--r-- 1 cats archive 3939 Aug 23 2017 +footg8.gif
-r--r--r-- 1 cats archive 3879 Sep 20 1994 rsafram.gz [Uncompressed]
-r--r--r-- 1 cats archive 2520 Jul 18 1994 rsamorp.gz [Uncompressed]
-r--r--r-- 1 cats archive 6796 Sep 14 1994 rsamuls1.gz [Uncompressed]
-r--r--r-- 1 cats archive 184647 Sep 14 1994 rsamuls2.gz [Uncompressed]
-r--r--r-- 1 cats archive 162463 Sep 16 1994 rsamuls3.gz [Uncompressed]
-r--r--r-- 1 cats archive 157390 Sep 14 1994 rsamuls4.gz [Uncompressed]
-r--r--r-- 1 cats archive 2957 Oct 22 1997 rsaphot.gz [Uncompressed]
-r--r--r-- 1 cats archive 8120 Sep 14 1994 rsaresu1.gz [Uncompressed]
-r--r--r-- 1 cats archive 452997 Sep 14 1994 rsaresu2.gz [Uncompressed]
Beginning of ReadMe :VII/184 Survey of 108 E-S0 galaxies (Michard+, 1993-94)
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Survey of 108 E-S0 RSA galaxies
Michard R., Marchal J.
<Astron. Astrophys. Suppl. Ser. 98, 29 (1993)>
<Astron. Astrophys. 283, 779 (1994)>
<Astron. Astrophys. Suppl. Ser. 105, 481 (1994)>
=1993A&AS...98...29M
=1994A&A...283..779M
=1994A&AS..105..481M
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ADC_Keywords: Galaxies, Markarian; Morphology; Photometry
Description:
Detailed data are available from our survey, results of which were
published in A&A, in a series of papers.
Abstract:
A survey has been performed of the morphological and photometric
properties of 108 E-S0 galaxies out of a complete sample of 112: this
sample is built from the Revised Shapley-Ames Catalogue (RSA) keeping
objects with delta>-10deg and V_0_<3000km/s, rejecting SB0's and
Local Group dwarfs. The data were mainly derived from our CCD
observations at Observatoire de Haute-Provence: the camera allowed
fields of 4x7arcmin (or 7x7 from the last run), the seeing being
generally in the 2-3arcsec FWHM range. The measurements include the
isophotal analysis according to Carter's (1978) principles, and the
photometric profiles along the two main axis. Opposite semi-axis are
measured separately to detect asymmetries.