J/A+AS/101/1 Wavelengths and transition probabilities in FeIII (Ekberg 1993) ================================================================================ Wavelengths and transition probabilities of the 3d6-3d54p and 3d54s-3d54p transition arrays of Fe III EKBERG J. O. =1993A&AS..101....1E ================================================================================ ADC_Keywords: Atomic physics Keywords: atomic data - Fe III - wavelengths - transition probabilities File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 77 2717 Wavelength list 59.8-210.5 nm table2 77 560 Wavelength list 210.5-812.3 nm table3 33 107 Level list of 3d6 and 3d5 4s table4 34 208 Level list of 3d5 4p -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1 table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Comments Comments on line: see note (1) 11- 17 E7.2 s-1 gA gA-values 21- 28 F8.3 0.1nm Lambda(pre) Predicted wavelengths in vacuum (table1) in air (table2) (from energy levels): see note (2) 31- 38 F8.3 0.1nm Lambda(obs) Observed wavelengths 42- 50 F9.2 cm-1 Sigma Predicted wavenumbers 54- 64 A11 --- lower Designation of lower level in combination 67- 77 A11 --- upper Designation of upper level in combination -------------------------------------------------------------------------------- Note (1): The intensities are given first and are in table1: estimates of photographic blackening on a logarithmic scale in table2: marked E when from Edlen and Swings (1942) and G when from Glad (1956) A roman figure following the intensity indicates an affected (a) line and blended (b) line of that iron spectrum. An arabian figure gives the multiplet number from Moore (1952). Note (2): Predicted wavelengths are calculated from the adopted level energies in table 3 and table4. Observed are from: the present measurement in table1 Edlen and Swings (1942) and Glad (1956) in table2 Byte-by-byte Description of file: table3 table4 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Designation Designations of level 17- 25 F9.2 cm-1 Energy Level energies 31- 33 I3 --- No. Number of combinations with the level -------------------------------------------------------------------------------- References: Edlen B., Swings P., 1942, ApJ 95, 532 Glad S., 1956, Arkiv Fysik 10, 291 Moore C.E., 1952, "A Multiplet Table of Astrophysical Interest", NBS Circ. 488 ================================================================================ (End) Patricia Bauer [CDS] 28-Sep-1993