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J/AJ/105/427        IRAS fluxes of UCM galaxies             (Rego+ 1993)

IRAS observations of H-alpha selected emission-line galaxies. Rego M., Cordero-Gracia M., Zamorano J., Gallego J. <Astron. J. 105, 427 (1993)> =1993AJ....105..427R
ADC_Keywords: Galaxy catalogs ; Infrared sources Abstract: We present the results of IRAS observations of the UCM (Universidad Complutense de Madrid) sample of emission-line galaxies, which have been selected from wide-dispersion Hα objective-prism plates. These data are intended to provide a convenient summary of the relevant far-infrared (FIR) properties of these galaxies. Color-color diagrams, as interpreted by theoretical models, suggest that emission from UCM galaxies is mainly due to dust heated directly by photons emitted in active star-forming regions. Statistical analysis of some samples, including the IRAS minisurvey and blue selected objective-prism samples, have been performed. Comparisons, based on FIR luminosity distributions, with the IRAS minisurvey make evident the lower metallicity of the UCM galaxies which cannot be considered as a parent population of IRAS-detected galaxies. The FIR luminosity distributions of different samples have been compared using nonparametric methods and the best correlation has been found for the UCM and Wasilewski samples. Finally, a more detailed analysis of a UCM subsample has been performed from a three component model in order to get information concerning the fractional contribution of disk, star formation activity, and nonthermal mechanisms operating in the UCM galaxies. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 83 248 UCM galaxy sample table2.dat 35 58 Contributions of the three components to the UCM (Universidad Complutense de Madrid) observed fluxes.
See also: J/ApJS/95/387 : Universidad Complutense de Madrid list 1 (Zamorano+ 1994) J/ApJS/105/343 : Universidad Complutense de Madrid list 2 (Zamorano+ 1996) J/ApJS/122/415 : UCM list 3 (Alonso+, 1999) J/A+AS/118/7 : Photometry + morphology of UCM galaxies (Vitores+, 1996) J/A+AS/120/323 : Long-slit spectroscopy of UCM galaxies (Gallego+ 1996) J/A+AS/141/409 : Photometry of UCM galaxies. I. (Perez-Gonzalez+, 2000) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 A3 --- --- [UCM] 4- 12 A9 --- UCM UCM designation (HHMM+DDMM, 1950 position) 14 A1 --- l_F12um Limit flag on F12um 15- 18 F4.2 Jy F12um IRAS Flux density at 12µm 20 A1 --- l_F25um Limit flag on F25um 21- 24 F4.2 Jy F25um IRAS Flux density at 25µm 26 A1 --- l_F60um Limit flag on F60um 27- 31 F5.2 Jy F60um IRAS Flux density at 60µm 33 A1 --- l_F100um Limit flag on F100um 34- 38 F5.2 Jy F100um IRAS Flux density at 100µm 40- 44 F5.2 mag mpg ? Photographic magnitude 46- 52 F7.5 --- z ? Redshift 54- 83 A30 --- Names Other names (1)
Note (1): abbreviations used are: CG = Pesch et al., 1991ApJS...76.1043P HOLM = Holmberg, 1937AnLun...6....1H KARA = Karachentsev, 1972, Cat. VII/77 KAZ = Kazarian & Kazarian, 1980Afz....16...17K KUG = KISO (Takase & Hiyauchi-Isobe, 1991, See Cat. VII/179) M = Vorontsov-Velyaminov & Krasnogorskaja, 1962, Cat. VII/62 MK = Markarian & Lipovetskii, 1971-79, See Cat. VII/172 N = NGC, Dreyer, 1888, See Cat. VII/118 PG = Palomar Green (Green et al., 1986, Cat. II/207) REIZ = Reiz, 1941AnLun...9....1R U = UGC Nilson, 1973, Cat. VII/26 UM = University of Michigan Survey (MacAlpine & Williams, 1981, Cat. VII/171) WAS = Wasilewski, 1983ApJ...272...68W ZWG = Zwicky & Herzog, 1963, Cat. VII/4
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 A3 --- --- [UCM] 4- 12 A9 --- UCM UCM designation (HHMM+DDMM, 1950 position) 14- 17 F4.2 % d Contribution fraction of normal disk (d) component 19- 22 F4.2 % b Contribution fraction of starburst (b) component 24- 27 F4.2 % s Contribution fraction of Seyfert (s) component 29- 32 F4.2 % sigma Computed error
History: Prepared via OCR at CDS, and proof-read by Heinz Andernach (Guanajuato Univ.)
(End) James Marcout, Patricia Bauer [CDS] 20-Oct-1998
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

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