J/ApJ/661/801   Survey for ionization in neutral gas galaxies. III. (Oey+, 2007)

The survey for ionization in neutral gas galaxies. III. Diffuse, warm ionized medium and escape of ionizing radiation. Oey M.S., Meurer G.R., Yelda S., Furst E.J., Caballero-Nieves S.M., Hanish D.J., Levesque E.M., Thilker D.A., Walth G.L., Bland-Hawthorn J., Dopita M.A., Ferguson H.C., Heckman T.M., Doyle M.T., Drinkwater M.J., Freeman K.C., Kennicutt R.C.Jr, Kilborn V.A., Knezek P.M., Koribalski B., Meyer M., Putman M.E., Ryan-Weber E.V., Smith R.C., Staveley-Smith L., Webster R.L., Werk J., Zwaan M.A. <Astrophys. J., 661, 801-814 (2007)> =2007ApJ...661..801O 2007ApJ...661..801O
ADC_Keywords: Galaxy catalogs; H II regions Keywords: galaxies: evolution - galaxies: ISM - galaxies: starburst - H II regions - intergalactic medium - ISM: evolution Abstract: We use the first data release from the Survey for Ionization in Neutral-Gas Galaxies (SINGG) Hα survey of HI-selected galaxies to study the quantitative behavior of the diffuse, warm ionized medium (WIM) across the range of properties represented by these 109 galaxies. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 102 107 *SINGG SR1 Galaxy Parameters -------------------------------------------------------------------------------- Note on table1.dat: the multiple source J0514-61 was omitted owing to processing problems, so the sample has less galaxies than the full SR1 sample. -------------------------------------------------------------------------------- See also: VIII/73 : HI Parkes All Sky Survey Catalogue (HIPASS) (Meyer+, 2004) J/ApJS/165/307 : Ionization in neutral gas galaxies survey. I. (Meurer+, 2006) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- HIPASS HIPASS Identification (JHHMM-DDa or JHHMM-DD:SN) (1) 13- 25 A13 --- OptID Optical Identification 27 A1 --- n_OptID [bc] Individual notes on OptID (2) 29- 48 A20 --- HType Hubble type 50- 53 F4.1 Mpc Dist Distance (3) 55- 58 F4.1 deg Inc Inclination 60- 63 F4.2 pc/cm6/pc TG HIIphot terminal gradient 65 A1 --- l_logMHI Limit flag on logMHI 67- 71 F5.2 [solMass] logMHI Log of HI mass 73- 77 F5.2 [solLum] logLR Log of R band luminosity 79- 83 F5.2 [10-7W] logLHa Log of Hα luminosity 85- 89 F5.2 [10-7W/kpc2] logSuBr Log of Hα surface brightness (4) 91- 94 F4.2 --- fWIM Hα diffuse fraction 96 A1 --- l_logSFR Limit flag on logSFR 98-102 F5.2 [solMass/yr] logSFR Log of critical star formation rate -------------------------------------------------------------------------------- Note (1): Galaxies identified as HIPASS JHHMM+DDa or SINGG HIPASS JHHMM+DD SN in Simbad Note (2): Flags on OptID as follows: b = Galaxy identified in the Automatic Plate Measuring facility survey (Maddox et al. 1990MNRAS.243..692M 1990MNRAS.243..692M); full APM designation available via NED. c = Full designation is 2MASX J02243002-2444441 Note (3): Derived primarily from the HI radial velocities using the distance model of Mould et al. (2000ApJ...529..786M 2000ApJ...529..786M), with optical distances to the nearest sources taken from the Catalog of Neighboring Galaxies (Karachentsev et al., 2004, Cat. J/AJ/127/2031). Note (4): In units of erg/s/kpc2. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Meurer et al., Paper I 2006ApJS..165..307M 2006ApJS..165..307M, Cat. J/ApJS/165/307 Hanish et al., Paper II 2006ApJ...649..150H 2006ApJ...649..150H
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 04-Apr-2009
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