VI/84               UVILLSS Catalogue          (Coluzzi 1996)

Identification List of Lines in Stellar Spectra in the Ultraviolet region (UVILLSS Catalogue) Coluzzi R. <Bull. Inf. CDS 48, 15 (1996)> =1996BICDS..48...15C 1996BICDS..48...15C
ADC_Keywords: Atomic physics ; Spectra, ultraviolet Description: This catalogue is an extension in the ultraviolet region (129 to 3903 Angstroems) of the ILLSS catalogue (Coluzzi, 1993; catalog VI/71) which lists lines in the optical region. The data are from "Ultraviolet Multiplet Table" (Moore 1950, 1952, 1962) and arranged in two files: the catalogue and the references. There are two versions of each file, one presented in the author's original format, and the second organised as a table. The reference files are arranged by element: for each spectrum the first line contains within parenthesis the Ionization Potential; the grade of analysis; the grade denoting the relative number of classified lines included as compared with the total number classified in the ultraviolet; the date of completion of the manuscript; the limit for three spectra H, He I, He II. The limit in cm-1 has been multiplied by the factor 0.00012345 to obtain the tabulated ionisation potential, which is expressed in electron-Volts. The analysis grades range from A to E, grade A indicating that the analysis is essentially complete ,and grade E that the structure has been recognised, but is limited to a single multiplet or transition. List A, List B, etc., denote the relative numbers of classified lines listed here as compared with the total number classified in the ultraviolet, A denoting that all classified lines in the ultraviolet are listed, and D that only a few of the leading ones are tabulated. The letters on the left, A, B, C, etc. preceding the reference, indicate the source used for the wavelength quoted in the Table. Those papers used only for analysis or intensity follow the ones used for wavelength, and are not preceded by the letters denoting the source. The letters "WL", "I", "T", indicating what was taken from each paper for the Table compilation , denote, respectively, wavelength, intensity, and terms, the last referring to the analysis of the spectrum. These informations are taken from Moore (1950). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file uvillss.dat 66 18431 The catalogue as a formatted table refs.dat 91 828 References as a formatted table uvillss.cat 67 18431 *The UVILLSS finding list uvillss.ref 137 1097 *The UVILLSS finding list -------------------------------------------------------------------------------- Note on uvillss.cat: this is the file as described in the publication: it contains multiplet number within parentheses (), intensities between square brackets [], and potential ionisation between angle brackets <>. Note on uvillss.ref: this is the file as described in the publication. -------------------------------------------------------------------------------- Byte-by-byte Description of file: uvillss.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 11 F9.4 0.1nm lambda [129/3903]+= Wavelength in Angstroems 13- 17 A5 --- Element Element name and spectrum 19- 20 I2 --- Z Atomic element number 22 I1 --- Ion [0/5] Electronic charge 24- 25 A2 --- n_lambda [a* ] '*' for blend, 'a' for air lambda 27- 36 A10 --- Multiplet Multiplet number 41 A1 --- RefL Reference of intensity (1) 43- 49 F7.1 --- Intens [0/99999]? Intensity with Moore notation (2) 50- 57 A8 --- n_Intens Notes about the Intensity (2) 59- 65 F7.3 eV IP ? Ionisation Potential 66 A1 --- u_IP [?] Uncertainty note on IP -------------------------------------------------------------------------------- Note (1): the Element, associated to the reference letter RefL, is the key to retrieve the reference in file refs.dat Note (2): the following notations are used: - A colon : indicates that the intensity is not the first or second choice (in place of the original parentheses) - The letters have the following meaning: 'bl' blended 'd' double 'g' ghost 'l' shaded to longer wave-length 'n' diffuse or hazy 'N' very diffuse or very hazy 'p' part of band 'r' narrow self-reversal 'R' wide self-reversal 's' shaded to shorter wave-length 'tr' trace 'w' wide(fine structure type),broad or complex 'W' very wide(fine structure type) or very broad -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Element Element name and spectrum (1) 7 A1 --- RefL Reference in element (1) 8- 91 A84 --- Text of reference -------------------------------------------------------------------------------- Note (1): the Element, associated to the reference letter RefL, is the key to retrieve the reference in file refs.dat -------------------------------------------------------------------------------- History: * 03-Apr-1996: First version * 28-Mar-1997: The Intens column which was stored as characters, have been transformed into a numeric intensity plus a remarks column at CDS (F. Ochsenbein). The very high value of 100000 for the line at 1178.650Angstroems was then changed to 99999. Courtesy: Regina Coluzzi References: Coluzzi, R.: 1993, Bull. Inf. CDS =1993BICDS..43....7C 1993BICDS..43....7C (catalog VI/71) Moore, C.E.: 1950, "AN ULTRAVIOLET MULTIPLET TABLE", Circular of the National Bureau of Standards 488, Section 1 Moore, C.E.: 1952, "AN ULTRAVIOLET MULTIPLET TABLE", Circular of the National Bureau of Standards 488, Section 2 Moore, C.E.: 1962, "AN ULTRAVIOLET MULTIPLET TABLE", Circular of the National Bureau of Standards 488, Sections 3,4,5
(End) Francois Ochsenbein [CDS] 27-Mar-1997
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