J/other/JAD/12.1  Catalog of galaxy structures based on the MRSS  (Panko+, 2006)

A catalogue of galaxy clusters and groups based on the Muenster Red Sky Survey. Panko E., Flin P. <J. Astron. Data, 12, 1-9 (2006)> =2006JAD....12....1P 2006JAD....12....1P
ADC_Keywords: Clusters, galaxy ; Magnitudes ; Morphology Keywords: galaxy clusters - catalogues Abstract: We present a catalogue of galaxy structures (groups and clusters) found in an area of 5000 square degrees in the southern hemisphere. The catalogue, which we call the PF Catalogue, was created by making use of galaxy positions and magnitudes given in the Muenster Red Sky Survey (MRSS, 2003JAD.....9....1U 2003JAD.....9....1U). We applied an automated procedure for structure finding, involving the Voronoi tessellation. The completeness limit for galaxies in the MRSS is rF=18.3m. Therefore, the present version of the PF Catalogue is based on galaxies brighter than this limit. In order to be included in the PF Catalogue, a structure must have at least 10 members in a magnitude range m3, m3+3m. We found 6188 structures which are listed in the present catalogue. The PF Catalogue contains positions, radii, areas, number of galaxies within the magnitude limit m3, m3+3m, a number estimation of background galaxies; ellipticity and position angle for each structure, as well as the magnitudes of the first, the third and the tenth galaxies in a structure, taken from the MRSS. Description: We selected the Voronoi tessellation technique (Voronoi, G. 1908, J. Reine Angew. Math. 134, 198) for cluster detection. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file pfcat.dat 126 6188 The PF Catalogue (version PFcat18, see erratum.pdf) erratum.pdf 148 89 Text of the erratum -------------------------------------------------------------------------------- See also: B/eso : ESO Science Archive Catalog (ESO, 2012) J/ApJ/723/985 : Orientation of galaxies in galaxy clusters (Godlowski+, 2010) Byte-by-byte Description of file (2 headlines): pfcat.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- PF Structure identification (HHhh-DDdd) 11- 20 F10.7 h RAhour Right Ascension in decimal hours (J2000) 22- 31 F10.6 deg DEdeg Right Ascension in decimal degrees (J2000) 33- 36 I4 arcsec Rad Equivalent radius for full area of structure 38- 45 I8 arcsec2 S The area of structure in square arcseconds 47- 49 I3 --- N Number of all galaxies in the field of structure 51- 53 I3 --- Nm Number of galaxies in the field of structure within the magnitude limits [m3, m3+3] 55- 57 I3 --- Nbg Estimated number of background galaxies 63- 66 I4 arcsec amaj Major semiaxis of the fitted ellipse 68- 71 I4 arcsec bmin Minor semiaxis of the fitted ellipse 73- 76 F4.2 --- Ell Ellipticity of the structure 79- 83 F5.1 deg PA Position angle of major axis of structure (1) 88- 92 F5.2 mag m1 MRSS magnitude of the brightest galaxy 94- 98 F5.2 mag m3 The third-brightest galaxy as given in MRSS 100-104 F5.2 mag m10 The tenth-brightest galaxy as given in MRSS 111-115 F5.1 deg PA1 The position angle of the brightest galaxy major axis (from MRSS) 117-120 F4.2 --- Ellm Average mean ellipticity for galaxies (calculated from MRSS data) 122-126 F5.1 deg PAm Mean position angle of galaxies in structure (calculated from MRSS data) -------------------------------------------------------------------------------- Note (1): The angle is counted clockwise from direction to the North Pole, same as the PA for galaxies in the MRSS (Muenster Red Sky Survey) -------------------------------------------------------------------------------- History: * 13-Aug-2012: From http://www.vub.ac.be/STER/JAD/JAD12/jad12_1/jad12_1.htm * 29-Jul-2013: Erratum communicated by the author (Elena Panko), with a new version of the catalog (PFcat18), with fixed values of the mean position angle (PAm).
(End) Emmanuelle Perret, Francois Ochsenbein [CDS] 28-Jul-2013
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line