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J/A+A/415/993       FeII, ZNI and SI abundances on halo stars   (Nissen+, 2004)

Sulphur and zinc abundances in Galactic stars and damped Ly-alpha systems. Nissen P.E., Chen Y.Q., Asplund M., Pettini M. <Astron. Astrophys. 415, 993 (2004)> =2004A&A...415..993N
ADC_Keywords: Equivalent widths ; Stars, F-type ; Stars, G-type ; Stars, halo Keywords: stars: abundances - stars: atmospheres - galaxy: evolution - galaxies: high-redshift - quasars: absorption lines Description: The table gives equivalent widths (in mÅ) for 19 FeII lines, two ZnI lines, and four SI lines, as measured in high resolution VLT/UVES spectra of 34 metal-poor, main sequence and subgiant, halo stars. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 70 34 Star positions and magnitudes (from Simbad) tablea1.dat 187 25 Equivalent widths
See also: II/180 : uvby-beta photometry of metal-poor stars (Schuster+ 1989) J/A+A/390/235 : OI & FeII equivalent widths in metal-poor stars (Nissen+ 2002) J/A+AS/117/317 : uvby-beta photometry of metal-poor stars VIII (Schuster+ 1996) J/A+A/326/751 : Chemical composition of halo and disk stars (Nissen+, 1997) J/A+AS/141/491 : Chemical composition of halo and disk stars (Nissen+, 2000) Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Name Object name 15- 16 I2 h RAh Right ascension (J2000.0) 18- 19 I2 min RAm Right ascension (J2000.0) 21- 24 F4.1 s RAs Right ascension (J2000.0) 26 A1 --- DE- Declination sign (J2000.0) 27- 28 I2 deg DEd Declination (J2000.0) 30- 31 I2 arcmin DEm Declination (J2000.0) 33- 34 I2 arcsec DEs Declination (J2000.0) 38- 42 F5.2 mag Bmag ? B magnitude 44- 48 F5.2 mag Vmag ? V magnitude 50- 70 A21 --- SpType MK Spectral type
Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Element Chemical element and ionization stage 7- 13 F7.2 0.1nm Lambda Wavelength of spectral line 15- 18 F4.1 0.1pm EW1 ? Equivalent widths for BD-13 3442 20- 23 F4.1 0.1pm EW2 ? Equivalent widths for CD-30 18140 25- 28 F4.1 0.1pm EW3 ? Equivalent widths for CD-35 14849 30- 33 F4.1 0.1pm EW4 ? Equivalent widths for CD-42 14278 35- 38 F4.1 0.1pm EW5 ? Equivalent widths for HD 103723 40- 43 F4.1 0.1pm EW6 ? Equivalent widths for HD 105004 45- 48 F4.1 0.1pm EW7 ? Equivalent widths for HD 106038 50- 53 F4.1 0.1pm EW8 ? Equivalent widths for HD 108177 55- 58 F4.1 0.1pm EW9 ? Equivalent widths for HD 110621 60- 64 F5.1 0.1pm EW10 ? Equivalent widths for HD 121004 66- 69 F4.1 0.1pm EW11 ? Equivalent widths for HD 140283 71- 74 F4.1 0.1pm EW12 ? Equivalent widths for HD 146296 76- 80 F5.1 0.1pm EW13 ? Equivalent widths for HD 148816 82- 85 F4.1 0.1pm EW14 ? Equivalent widths for HD 160617 87- 90 F4.1 0.1pm EW15 ? Equivalent widths for HD 179626 92- 95 F4.1 0.1pm EW16 ? Equivalent widths for HD 181743 97-100 F4.1 0.1pm EW17 ? Equivalent widths for HD 188031 102-105 F4.1 0.1pm EW18 ? Equivalent widths for HD 193901 107-110 F4.1 0.1pm EW19 ? Equivalent widths for HD 194598 112-115 F4.1 0.1pm EW20 ? Equivalent widths for HD 215801 117-120 F4.1 0.1pm EW21 ? Equivalent widths for LP 815-043 122-125 F4.1 0.1pm EW22 ? Equivalent widths for G 011-044 127-130 F4.1 0.1pm EW23 ? Equivalent widths for G 013-009 132-136 F5.1 0.1pm EW24 ? Equivalent widths for G 016-013 138-141 F4.1 0.1pm EW25 ? Equivalent widths for G 018-039 143-146 F4.1 0.1pm EW26 ? Equivalent widths for G 020-008 148-151 F4.1 0.1pm EW27 ? Equivalent widths for G 024-003 153-156 F4.1 0.1pm EW28 ? Equivalent widths for G 029-023 158-161 F4.1 0.1pm EW29 ? Equivalent widths for G 053-041 163-166 F4.1 0.1pm EW30 ? Equivalent widths for G 064-012 168-171 F4.1 0.1pm EW31 ? Equivalent widths for G 064-037 173-176 F4.1 0.1pm EW32 ? Equivalent widths for G 066-030 178-181 F4.1 0.1pm EW33 ? Equivalent widths for G 126-062 183-186 F4.1 0.1pm EW34 ? Equivalent widths for G 186-026
Acknowledgements: Poul Erik Nissen
(End) Patricia Bauer [CDS] 09-Dec-2003
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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