J/AJ/130/1502    NGC 5846 group: photometry and spectroscopy    (Mahdavi+, 2005)

The NGC 5846 group: dynamics and the luminosity function to mR=-12. Mahdavi A., Trentham N., Tully R.B. <Astron. J., 130, 1502-1515 (2005)> =2005AJ....130.1502M 2005AJ....130.1502M
ADC_Keywords: Clusters, galaxy ; Magnitudes ; Redshifts Keywords: clusters: individual (NGC 5846) - galaxies: dwarf - galaxies: halos - galaxies: kinematics and dynamics - galaxies: luminosity function, mass function - X-rays: galaxies Abstract: We conduct a photometric and spectroscopic survey of a 10°2 region surrounding the nearby NGC 5846 group of galaxies, using the Canada-France-Hawaii and Keck I telescopes to study the population of dwarf galaxies as faint as MR=-10. Candidates are identified on the basis of quantitative surface brightness and qualitative morphological criteria. Spectroscopic follow up and a spatial correlation analysis provide the basis for affirming group memberships. Altogether, 324 candidates are identified, and 83 have spectroscopic membership confirmation. Description: Observations of the NGC 5846 Group were made with the CFHT 12K CCD camera in queue mode during 11 nights between 2002 March 16 and June 10. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 98 324 Photometric and spectroscopic data -------------------------------------------------------------------------------- See also: J/ApJ/607/202 : Redshift survey of nearby galaxy groups (Mahdavi+, 2004) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- [MTT2005] Galaxy Identification 11 I1 --- Memb Original membership probability (1) 13- 14 I2 h RAh Hour of Right Ascension (J2000) 16- 17 I2 min RAm Minute of Right Ascension (J2000) 19- 22 F4.1 s RAs Second of Right Ascension (J2000) 24 A1 --- DE- Sign of the Declination (J2000) 25- 26 I2 deg DEd Degree of Declination (J2000) 28- 29 I2 arcmin DEm Arcminute of Declination (J2000) 31- 32 I2 arcsec DEs Arcsecond of Declination (J2000) 34- 37 A4 --- MType Morphological type (2) 39- 43 F5.2 mag Rcmag Cousins R band isophotal magnitude to a 25.2mag/arcsec2 45- 49 F5.2 mag R300mag R band magnitude within 300pc (2.3") 51- 56 F6.2 mag RcMAG Absolute isophotal R band magnitude 58- 61 F4.2 mag AR Reddening in the R band 63- 66 F4.1 arcsec Reff Half-light radius 68- 72 F5.2 mag/arcsec2 SuBrR R band surface brightness 74- 77 I4 km/s cz ? Heliocentric velocity 79- 98 A20 --- Notes Other galaxy identifications (3) -------------------------------------------------------------------------------- Note (1): Assigned to the galaxy purely from photometry and morphology. 0 = non-SDSS spectroscopic redshift; 1 = probable member; 2 = possible member; 3 = conceivable member; 4 = likely not a member; 5 = Excluded from original sample by the TT02 surface brightness criteria. Note (2): Morphological type, defined as follows: dI = dwarf irregular; dE = dwarf elliptical; N = nucleated dwarf; E = elliptical; S = spiral; VLSB = very low surface brightness galaxy. Note (3): ZM indicates data from Zabludoff & Mulchaey (1998, Cat. J/ApJ/496/39). All redshifts are from the NASA Extragalactic Database, unless the date of a Keck observation is indicated, in which case they are new. Galaxies marked with "sat" were saturated in our imaging; for these galaxies, all values were derived from SDSS public data, with appropriate conversions from the SDSS r to Cousins R photometric bands. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 20-Dec-2005
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