J/MNRAS/412/727    SDSS red gal. automated morph. classification  (Cheng+, 2011)

Automated morphological classification of Sloan Digital Sky Survey red sequence galaxies. Cheng J.Y., Faber S.M., Simard L., Graves G.J., Lopez E.D., Yan R., Cooper M.C. <Mon. Not. R. Astron. Soc., 412, 727-747 (2011)> =2011MNRAS.412..727C 2011MNRAS.412..727C (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Galaxies, photometry ; Morphology Keywords: galaxies: bulges - galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: structure Abstract: In the last decade, the advent of enormous galaxy surveys has motivated the development of automated morphological classification schemes to deal with large data volumes. Existing automated schemes can successfully distinguish between early- and late-type galaxies and identify merger candidates, but are inadequate for studying detailed morphologies of red sequence galaxies. To fill this need, we present a new automated classification scheme that focuses on making finer distinctions between early types roughly corresponding to Hubble types E, S0 and Sa. We visually classify a sample of 984 non-star-forming Sloan Digital Sky Survey galaxies with apparent sizes >14-arcsec. We then develop an automated method to closely reproduce the visual classifications, which both provides a check on the visual results and makes it possible to extend morphological analysis to much larger samples. We visually classify the galaxies into three bulge classes (BC) by the shape of the light profile in the outer regions: discs have sharp edges and bulges do not, while some galaxies are intermediate. We separately identify galaxies with features: spiral arms, bars, clumps, rings and dust. Description: The sample is extracted from the spectroscopic catalogue of galaxies in Data Release 4 (DR4) of the SDSS. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 205 984 Visual classifications and automated parameters for 984 galaxies -------------------------------------------------------------------------------- See also: J/MNRAS/385/2097 : NUV-J colours of red-sequence galaxies (Rawle+, 2008) J/A+A/525/A157 : SDSS automated morph. classification (Huertas-Company+ 2011) http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- Plate SDSS plate number 8- 12 I5 d MJD SDSS MJD number 16- 18 I3 --- Fiber SDSS Fibre number 22- 40 A19 --- ObjID SDSS ObjID designation 43- 49 F7.3 deg RAdeg Right ascension in decimal degrees (J2000) 52- 58 F7.3 deg DEdeg Declination in decimal degrees (J2000) 61- 67 F7.3 mag uMAG K-corrected absolute u magnitude 70- 76 F7.3 mag gMAG K-corrected absolute g magnitude 79- 85 F7.3 mag rMAG K-corrected absolute r magnitude 88- 94 F7.3 mag iMAG K-corrected absolute i magnitude 97-103 F7.3 mag zMAG K-corrected absolute z magnitude 106-112 F7.3 mag NUVMAG GALEX K-corrected absolute NUV magnitude 114-121 F8.3 mag FUVMAG GALEX K-corrected absolute FUV magnitude 125-130 F6.3 arcsec R50 SDSS Petrosian radius that encompass 50% of the total Petrosian flux 134-139 F6.3 arcsec R90 SDSS Petrosian radius that encompass 90% of the total Petrosian flux 144-148 F5.3 --- b/a Axis ratio b/a 153-157 F5.3 --- B/T GIM2d bulge fraction B/T 162-166 F5.3 --- s2 Smoothness parameter 170-175 F6.3 deg Incl Inclination 178 I1 --- BC [1/3] Visual Classification from bulge class caracteristics (BC) (1) 181 I1 --- FE [1/3] Visual Classification from features caracteristics (FEAT) (1) 184 I1 --- AR [1/3] Visual Classification from spiral arms caracteristics (ARMS) (1) 187 I1 --- BA [1/3] Visual Classification from bars caracteristics (BAR) (1) 190 I1 --- CL [1/3] Visual Classification from clumps caracteristics (CLUMPS) (1) 193 I1 --- RI [1/3] Visual Classification from ring caracteristics (RING) (1) 196 I1 --- DU [1/3] Visual Classification from dust caracteristics (DUST) (1) 199 I1 --- DI [1/3] Visual Classification from disturbed caracteristics (DIST) (1) 202 I1 --- IN [1/3] Visual Classification from interacting caracteristics (INT) (1) 205 I1 --- Class Automated classification (1) -------------------------------------------------------------------------------- Note (1): Automated classification code as follows: 1 = one-bulge 2 = two-intermediate 3 = three-disc -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 26-Sep-2011
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