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J/A+AS/103/293   Lines unaffected by polarization          (Vela Villahoz+ 1994)

Spectral lines unaffected by instrumental polarization. II. Selected lines of astrophysical interest. VELA VILLAHOZ E., SANCHEZ ALMEIDA J., WITTMANN A.D. <Astron. Astrophys. Suppl. Ser. 103, 293 (1994)> =1994A&AS..103..293V
ADC_Keywords: Polarization; Atomic physics Keywords: magnetic field measurements - Zeeman effect - instrumental polarization File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 61 86 Lines with no linear polarization table2 75 420 Lines with negligible linear polarization
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
2- 5 A4 --- S Species 10- 16 F7.1 0.1nm lambda [2000/11300]+ Wavelength (Angstroems) 21- 35 A15 --- Trans Transition 40- 44 F5.3 --- geff Effective Lande factor 50- 55 F6.1 0.1pm W ]0/663]? Equivalent width (milli-Angstroems) 60 I1 --- Blend [0/3]? Blends
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
2- 5 A4 --- S Species 10- 16 F7.1 0.1nm lambda [2000/7301]+= Wavelength (Angstroems) 21- 35 A15 --- Trans Transition 40- 44 F5.3 --- geff Effective Lande factor 50- 53 F4.2 % R Ratio linear to circular polarization 60- 65 F6.1 0.1pm W ]0/1685]? Equivalent width (milli-Angstroems) 70 I1 ---- Blend [0/3]? Blends

(End) Francois Ochsenbein [CDS] 20-Sep-1993
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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