J/A+A/543/A44    Atomic data for iron peak and light odd-Z ions (Palmeri+, 2012)

Atomic decay data for modeling K lines of iron peak and light odd-Z elements. Palmeri P., Quinet P., Mendoza C., Bautista M.A., Garcia J., Witthoeft M.C., Kallman T.R. <Astron. Astrophys. 543, A44 (2012)> =2012A&A...543A..44P 2012A&A...543A..44P
ADC_Keywords: Atomic physics Keywords: atomic data - atomic processes - line: formation - X-rays: general Abstract: Complete data sets of level energies, transition wavelengths, A-values, radiative and Auger widths and fluorescence yields for K-vacancy levels of the F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn isonuclear sequences have been computed by a Hartree-Fock method that includes relativistic corrections as implemented in Cowan's atomic structure computer suite. The atomic parameters for more than 3 million fine- structure K lines have been determined. Ions with electron number N>9 are treated for the first time, and detailed comparisons with available measurements and theoretical data for ions with N=<9 are carried out in order to estimate reliable accuracy ratings. Description: Computed level energies, wavelengths, radiative transition probabilities, absorption oscillator strengths, radiative and Auger widths, and K-shell fluorescence yields in ions belonging to the F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn isonuclear sequences are given in these two tables. In Table 9 levels are identified by the atomic number (Z), the electron number (N), the level index, the spin multiplicity, the total orbital angular momentum quantum number, the total angular momentum quantum number and the electronic configuration. For each level, the computed HFR energy and its radiative width are listed. For K-vacancy levels, the Auger width and the K-shell fluorescence yield are also given. In Table 10 transitions are identified with the atomic number, the electron number, the upper and lower level indices tabulating its computed wavelength, radiative transition probability, weighted oscillator strength, and cancellation factor. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table9.dat 79 51417 Valence and K-vacancy levels table10.dat 48 3398951 K-vacancy transitions -------------------------------------------------------------------------------- See also: J/A+A/410/359 : Radiative and Auger decay for Fe II-Fe IX (Palmeri+, 2003) J/A+A/414/377 : FeX-FeXVII fine-structure K-vacancy levels (Mendoza+, 2004) Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Z [9/30] Atomic number 4- 5 I2 --- N [2/29] Number of electrons 7- 10 I4 --- i [1/1943] Level index 12 I1 --- 2S+1 [1/8] Spin multiplicity 14 I1 --- L [0/7] Orbital angular momentum quantum number 16- 17 I2 --- 2J [0/17] 2*(Total angular momentum quantum number) 19- 41 A23 --- Conf Configuration assignment 43- 52 E10.5 keV E Level energy 54- 61 E8.3 s-1 Ar Radiative width 63- 70 E8.3 s-1 Aa Auger width 72- 79 E8.3 --- WK [0/1] Fluorescence yield -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Z [9/30] Atomic number 4- 5 I2 --- N [2/29] Number of electrons 7- 10 I4 --- k [1/1943] Upper level index 12- 15 I4 --- i [1/1943] Lower level index 17- 23 F7.4 0.1nm WL [1.25/19.7] Wavelength (in Å) 25- 32 E8.3 s-1 Ar Radiative transition probability 34- 41 E8.3 --- gf Weighted oscillator strength 43- 48 F6.3 --- CF [-1/1] Cancellation factor -------------------------------------------------------------------------------- Acknowledgements: Patrick Palmeri, patrick.palmeri(at)umons.ac.be
(End) Patrick Palmeri [UMONS], Patricia Vannier [CDS] 22-May-2012
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