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J/MNRAS/330/75    Chemical abundances in UV-selected galaxies   (Contini+, 2002)

Chemical abundances in a UV-selected sample of galaxies. Contini T., Treyer M.A., Sullivan M., Ellis R.S. <Mon. Not. R. Astron. Soc. 330, 75 (2002)> =2002MNRAS.330...75C
ADC_Keywords: Photometry, ultraviolet ; Redshifts ; Spectroscopy ; Abundances Keywords: galaxies: abundances - galaxies: evolution - galaxies: starburst - ultraviolet: galaxies Abstract: We discuss the chemical properties of a sample of UV-selected intermediate-redshift (0≤z≤0.4) galaxies in the context of their physical nature and star-formation history. This work represents an extension of our previous studies of the rest-frame UV-luminosity function (Treyer et al., 1998, Cat. J/MNRAS/300/303) and the star-formation properties of the same sample (Sullivan et al., 2000, Cat. J/MNRAS/312/442). We revisit the optical spectra of these galaxies and perform further emission-line measurements restricting the analysis to those spectra with the full set of emission lines required to derive chemical abundances. Our final sample consists of 68 galaxies with heavy-element abundance ratios and both UV and CCD B-band photometry. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 105 68 The sample of UV-selected galaxies with measurements of chemical abundances, part 1 table2.dat 65 68 The sample of UV-selected galaxies with measurements of chemical abundances, part 2
See also: J/MNRAS/300/303 : UV-selected galaxy redshift survey. I. (Treyer+, 1998) J/MNRAS/312/442 : UV-selected galaxy redshift survey. II. (Sullivan+, 2000) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 --- [CTS2002] [1/68] Sequential number 4- 5 I2 h RAh Right ascension (1950) 7- 8 I2 min RAm Right ascension (1950) 10- 14 F5.2 s RAs Right ascension (1950) 16 A1 --- DE- Declination sign (1950) 17- 18 I2 deg DEd Declination (1950) 20- 21 I2 arcmin DEm Declination (1950) 23- 26 F4.1 arcsec DEs Declination (1950) 28 A1 --- OCs Number of optical counterparts in the POSS plates within 10" 30- 34 F5.2 --- [OIII]/[OII] Emission-line ratio [OIII]/[OII] 36- 39 F4.2 --- e_[OIII]/[OII] rms uncertainty on [OIII]/[OII] 41- 45 F5.2 --- [OIII]/Hbeta Emission-line ratio [OIII]/Hβ 47- 50 F4.2 --- e_[OIII]/Hbeta rms uncertainty on [OIII]/Hβ 52- 56 F5.2 --- [NII]/Halpha Emission-line ratio [NII]/Hα 58- 61 F4.2 --- e_[NII]/Halpha rms uncertainty on [NII]/Hα 63- 67 F5.2 --- [SII]/Halpha ? Emission-line ratio [SII]/Hα 69- 72 F4.2 --- e_[SII]/Halpha ? rms uncertainty on [SII]/Hα 74- 78 F5.2 --- [NII]/[OII] Emission-line ratio [NII]/[OII] 80- 83 F4.2 --- e_[NII]/[OII] rms uncertainty on [NII]/[OII] 85- 88 F4.2 --- log(R23) R23 = ([OII]3727+[OIII]4959,5007)/Hβ 90- 93 F4.2 --- e_log(R23) rms uncertainty on log(R23) 95 A1 --- Note [UL?] Flag (1) 97-100 F4.2 --- O/HL Oxygen abundance, 12+log(O/H), on the lower branch (2) 102-105 F4.2 --- O/HU Oxygen abundance, 12+log(O/H), on the upper branch (2)
Note (1): Flag indicating if the object lies on the lower (L) or in the upper (U) branch of the O/H versus R23 relationship, or falls in the turnaround region (?). Note (2): Oxygen abundances derived from the empirical calibrations (McGaugh, 1991ApJ...380..140M)
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 --- [CTS2002] [1/68] Sequential number 4- 5 I2 h RAh Right ascension (1950) 7- 8 I2 min RAm Right ascension (1950) 10- 14 F5.2 s RAs Right ascension (1950) 16 A1 --- DE- Declination sign (1950) 17- 18 I2 deg DEd Declination (1950) 20- 21 I2 arcmin DEm Declination (1950) 23- 26 F4.1 arcsec DEs Declination (1950) 28 A1 --- OCs Number of optical counterparts in the POSS plates within 10" 30- 34 F5.3 --- z Redshift 36- 39 F4.2 mag AV Extinction coefficient in V band 41- 44 F4.2 mag e_AV rms uncertainty on AV 46- 49 F4.2 --- 12+log(O/H) 12+log(O/H) abundance ratio 51- 54 F4.2 --- e_12+log(O/H) rms uncertainty on 12+log(O/H) 56- 60 F5.2 --- log(N/O) log(N/O) abundance ratio 62- 65 F4.2 --- e_log(N/O) rms uncertainty on log(N/O)
History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 28-Mar-2002
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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