J/A+AS/101/1 J/A+AS/101/1 Wavelengths and transition probabilities of the J O Ekberg Astron. Astrophys. Suppl. Ser. 101 1 1993 1993A&AS..101....1E atomic data Fe III transition probabilities wavelengths *** No Description Available ***

Comments Comments on line: see note number=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). --- gA gA-values s-1 Lambda(pre) Predicted wavelengths in vacuum (table1) in air (table2) (from energy levels): see note number=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 0.1nm Lambda(obs) Observed wavelengths 0.1nm Sigma Predicted wavenumbers cm-1 lower Designation of lower level in combination --- upper Designation of upper level in combination --- Designation Designations of level --- Energy Level energies cm-1 No. Number of combinations with the level --- Patricia Bauer CDS 1993Sep28 J_A+AS_101_1.xml