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J/A+A/317/416       Superclustering in the field of Q1037-2704 (Lespine+ 1997)

Physical conditions in metal line systems toward Q1037-2704: Evidence for superclustering at z ∼ 2. Lespine Y., Petitjean P. <Astron. Astrophys. 317, 416 (1997)> =1997A&A...317..416L (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; Line Profiles Keywords: intergalactic medium - quasars: absorption lines; Q1037-2704 - large-scale structure of the universe - galaxies: formation Description: The table gives the characteristics of the absorption lines observed in the spectrum of Q1037-2704 from 3733 A to 5050 A. Objects: ----------------------------------------- RA (2000) DE Designation(s) ----------------------------------------- 10 39 21.8 -27 19 15.8 QSO 1037-2704 ----------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 72 162 Absorption lines table1.tex 144 275 LaTeX version of table1
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
2- 3 I2 --- No Numbering of the line as indicated in Fig. 1 of the paper 5- 11 F7.2 0.1nm Lambda Vacuum heliocentric wavelength 12 A1 --- u_Lambda Uncertainty flag on LambdaHelio 14- 18 F5.2 0.1nm Wobs Observed wavelength 19 A1 --- u_Wobs Uncertainty flag on Wobs 20- 23 F4.2 0.1nm e_Wobs 1 sigma error in the continuum (1) 25- 42 A18 --- Ident Identification 44- 49 F6.4 --- Zabs ? Mean redshift of the line 51 I1 --- nFit ? Number of components used to fit the line 53- 57 F5.2 [cm-2] log(N) ? Logarithm of the column density 58 A1 --- n_log(N) Note on log(N) (2) 61- 64 F4.1 km/s b ? Doppler parameter 65 A1 --- u_b Uncertainty flag on b 66- 72 F7.5 --- z ? Redshift of the component (upper limit)
Note (1): sigmaWobs = σ x FWHM where σ is the noise rms in the adjacent continuum Note (2): Uncertain determination: typical error is 0.5 instead of 0.15 for other lines
Acknowledgements: Patrick Petitjean
(End) Patricia Bauer [CDS] 18-Jun-1996
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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