J/A+A/486/697       Hydra I Cluster Catalogue (HCC)          (Misgeld+, 2008)

The early-type dwarf galaxy population of the Hydra I cluster. Misgeld I., Mieske S., Hilker M. <Astron. Astrophys., 486, 697-709 (2008)> =2008A&A...486..697M 2008A&A...486..697M
ADC_Keywords: Clusters, galaxy ; Galaxies, photometry ; Radial velocities Keywords: galaxies: clusters: individual: Hydra I - galaxies: dwarf - galaxies: fundamental parameters - galaxies: luminosity function - mass function Abstract: We analyse the properties of the early-type dwarf galaxy population in the Hydra I cluster. We investigate the galaxy luminosity function, the colour-magnitude relation, and the magnitude-surface brightness relation down to MV=-10mag. Deep VLT/FORS1 images in V and I bands were examined. We identify cluster members by radial velocity measurements and select other cluster galaxy candidates by their morphology. The candidates' total magnitudes and central surface brightnesses were derived from the analysis of their surface brightness profiles. Description: The obtained photometric parameters along with the available radial velocities for all early-type galaxies in our sample (111 objects) are presented in the Hydra I Cluster Catalogue (HCC). For each galaxy right ascension, declination, extinction corrected magnitude V and colour V-I, central surface brightness and scale length of an exponential fit to the surface brightness profile, effective surface brightness, effective radius and profile shape index n, as obtained from a Sersic fit, are given. The physical scale is 0.2kpc/arcsec at the assumed distance modulus of (m-M)=33.07mag. The radial velocities are taken from our study and from Christlein & Zabludoff (2003ApJ...591..764C 2003ApJ...591..764C). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea2.dat 109 111 Photometric parameters and radial velocities for 111 early-type galaxies in the Hydra I cluster, ordered by increasing magnitude -------------------------------------------------------------------------------- See also: J/ApJS/85/249 : Surface photometry of Hydra I galaxies. I. (Hamabe 1993) Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [HCC-] 5- 7 I03 --- HCC Hydra I Cluster Catalogue (HCC) number 9- 10 I2 h RAh Right ascension (J2000) 12- 13 I2 min RAm Right ascension (J2000) 15- 18 F4.1 s RAs Right ascension (J2000) 20 A1 --- DE- Declination sign 21- 22 I2 deg DEd Declination (J2000) 24- 25 I2 arcmin DEm Declination (J2000) 27- 30 F4.1 arcsec DEs Declination (J2000) 32- 36 F5.2 mag Vmag V magnitude 38- 41 F4.2 mag e_Vmag Error of Vmag 43- 46 F4.2 mag V-I V-I colour index 48- 51 F4.2 mag e_V-I Error of V-I 53- 57 F5.2 mag/arcsec2 mu0 ? Central surface brightness (1) 59- 62 F4.2 mag/arcsec2 e_mu0 ? Error of mu0 64- 67 F4.2 arcsec hr ? Scale length of exp. fit (1) 69- 72 F4.2 arcsec e_hr ? Error of hr 74- 78 F5.2 mag/arcsec2 mueff ? Effective surface brightness (2) 80- 83 F4.2 mag/arcsec2 e_mueff ? Error of mueff 85- 90 F6.2 arcsec reff ? Effective radius (2) 92- 95 F4.2 arcsec e_reff ? Error of reff 97-100 F4.2 --- n ? Sersic profile shape index (2) 102-105 I4 km/s HRV ? Heliocentric radial velocity 107-109 I3 km/s e_HRV ? Error of HRV -------------------------------------------------------------------------------- Note (1): For objects with V magnitude brighter than 16.1mag, parameters are not given, since the surface brightness profile is not well described by an exponential law. Note (2): Sersic index n: f(r)∝r1/n) For some galaxies the Sersic parameters are not given, since those objects show a two component surface brightness profile, not well fitted by a single Sersic law. -------------------------------------------------------------------------------- Acknowledgements: Ingo Misgeld, imisgeld(at)eso.org
(End) Ingo Misgeld [ESO, Germany], Patricia Vannier [CDS] 23-Jul-2008
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