J/A+AS/128/361     Vacuum ultraviolet emission band systems of N2 (Roncin+ 1998)

Table of vacuum ultraviolet emission band systems of molecular nitrogen from 82.6 to 124.2 nm Roncin J.-Y., Launay F. <Astron. Astrophys. Suppl. Ser. 128, 361 (1998)> =1998A&AS..128..361R 1998A&AS..128..361R (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics ; Spectra, ultraviolet Keywords: molecular data - planets and satellites: general Abstract: Observed wavenumbers of the emission lines belonging to 10 vacuum ultraviolet band systems of molecular nitrogen are classified into 283 bands, 220 of them reported for the first time Description: The first column gives the rotational quantum number J of the electronic ground state. The corresponding R and P branch lines of the {SIGMA}-{SIGMA} transitions are listed in the second and third columns and the R, Q, and P branch lines of the {PI}-{SIGMA} transitions are listed in the second, third, and fourth columns. An asterisk is used to identify blended lines that have been assigned more than once, or to indicate, in the case of a missing line, that a feature has been observed within 1.2 and 2 cm-1 from the missing transition. For many missing lines we have written, in the same column, the name of the molecular absorption lines preventing the emission from being seen. Some missing lines could not be measured because they are overlapped by a strong atomic line which is identified in this column. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file rplines.dat 81 5968 Wavenumbers of R and P lines of the N2 band rqplines.dat 82 1356 Wavenumbers of R, Q and P lines of the N2 band -------------------------------------------------------------------------------- Byte-by-byte Description of file: rplines.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Band Band (1) 11- 12 I2 ---- J Rotational quantum number of the electronic ground state 14- 22 F9.2 cm-1 R ? R branch lines of the {SIGMA}-{SIGMA} transitions (2) 23 A1 --- BlendR [*] Blended line (3) 25- 43 A19 --- n_R Note for missing line (4) 45- 53 F9.2 cm-1 P ? P branch lines of the {SIGMA}-{SIGMA} transitions (2) 54 A1 --- BlendP [*] Blended line (3) 56- 81 A26 --- n_P Note for missing line (4) -------------------------------------------------------------------------------- Note (1): b'(i-j): b' 1{SIGMA}u+ -X 1{SIGMA}g+ band system of N2 c'4(i-j): c'4 1{SIGMA}u+ -X 1{SIGMA}g+ band system of N2 c'6(i-j): c'6 1{SIGMA}u+ -X 1{SIGMA}g+ band system of N2 3dp(0-1): 3dp 1{SIGMA}u+ -X 1{SIGMA}g+ band system of N2 Note (2): Some missing lines could not be measured because they are overlapped by a strong atomic line which is identified in this column. Note (3): An asterisk is used to identify blended lines that have been assigned more than once, or to indicate, in the case of a missing line, that a feature has been observed within 1.2 and 2cm-1 from the missing transition Note (4): Name of the molecular absorption lines preventing the emission from being seen -------------------------------------------------------------------------------- Byte-by-byte Description of file: rqplines.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Band Band (1) 11- 12 I2 ---- J Rotational quantum number of the electronic ground state 14- 22 F9.2 cm-1 R ? R branch lines of the {PI}-{SIGMA} transitions (2) 23 A1 --- BlendR [*] Blended line (3) 25- 33 A9 --- n_R Note for missing line (4) 34- 42 F9.2 cm-1 Q ? Q branch lines of the {PI}-{SIGMA} transitions (2) 43 A1 --- BlendQ [*] Blended line (3) 45- 59 A15 --- n_Q Note for missing line (4) 61- 69 F9.2 cm-1 P ? P branch lines of the {PI}-{SIGMA} transitions (2) 70 A1 --- BlendP [*] Blended line (3) 72- 82 A11 --- n_P Note for missing line (4) -------------------------------------------------------------------------------- Note (1): b(i-j): b 1{PI}u -X 1{SIGMA}g+ band system of N2 c3(i-j): c3 1{PI}u -X 1{SIGMA}g+ band system of N2 c4(0-j): c4 1{PI}u -X 1{SIGMA}g+ band system of N2 o3(i-j): o3 1{PI}u -X 1{SIGMA}g+ band system of N2 a(i-j): a 1{PI}g -X 1{SIGMA}g+ band system (L.B.H.) of N2 Note (2): Some missing lines could not be measured because they are overlapped by a strong atomic line which is identified in this column. Note (3): An asterisk is used to identify blended lines that have been assigned more than once, or to indicate, in the case of a missing line, that a feature has been observed within 1.2 and 2cm-1 from the missing transition Note (4): Name of the molecular absorption lines preventing the emission from being seen -------------------------------------------------------------------------------- Acknowledgements: Jean-Yves Roncin
(End) Patricia Bauer [CDS] 10-Nov-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