J/A+A/533/A87       Sulphur ions iso-electronic sequence     (Liang+, 2011)

R-matrix electron-impact excitation data for astrophysically abundant sulphur ions. Liang G.Y., Badnell N.R., Zhao G., Zhong J.Y., Wang F.L. <Astron. Astrophys. 533, A87 (2011)> =2011A&A...533A..87L 2011A&A...533A..87L
ADC_Keywords: Atomic physics Keywords: plasmas - atomic processes - atomic data Abstract: We present our calculated data including energy levels, radiative decay rates and effective collision strengths for all the transitions among fine-structure levels of n=3 or 4 configurations, for four iso-nuclear ions, viz S8+, S9+, S10+ and S11+. Description: The effective collision strengths at 13 temperatures ranging from 2x102(q+1)2 to 2x106(q+1)2K, where q is the residual charge of ions, have been calculated using the ICFT R-matrix method. The data format adopts ADAS adf04 format, see the file at website http://www.adas.ac.uk/man/appxa-04.pdf Additionally, tables of level energies for S^10+ and S^11+, along with other predictions are available in this online material. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 50 4 List of files files/* . 4 Individual files table3.dat 60 92 *Level energies (Ryd) of S8+ table4.dat 60 84 *Level energies (Ryd) of S9+ table6.dat 74 204 *Level energies (Ryd) of S11+ table5.dat 66 254 *Level energies (Ryd) of S10+ -------------------------------------------------------------------------------- Note on table*.dat: from different calculations along with experimentally derived values from NIST v4. -------------------------------------------------------------------------------- See also: J/A+A/500/1263 : Na-like iso-electronic sequence. I. (Liang+, 2009) J/A+A/518/A64 : Na-like iso-electronic sequence. II. (Liang+, 2010) J/A+A/528/A69 : Li-like iso-electronic sequence. (Liang+, 2011) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- FileName Name of the file in subdirectory files (1) 15- 50 A36 --- Title Title of the table -------------------------------------------------------------------------------- Note (1): Each file deals with one ion, and includes the 204 fine-structure levels and 21809 transitions. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- ID Identification 5- 26 A22 --- Level Level specification 28- 36 F9.6 Ry ENIST ? NIST level energy (G1) 38- 44 F7.4 Ry EAS Present AUTOSTRUCTURE calculation level energy (G2) 46- 52 F7.4 Ry EBL03 ? Bhatia & Landi(2003ApJS..147..409B 2003ApJS..147..409B) level energy 54- 60 F7.4 Ry EMCHF ? MCHF collection level energy (G3) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- ID Identification 8- 22 A15 --- Level Level specification 26- 34 F9.6 Ry Enist ? NIST level energy (G1) 38- 44 F7.4 Ry EAS Present AUTOSTRUCTURE calculation level energy (G2) 49- 55 F7.4 Ry ELB03 ? Landi & Bhatia (2003ApJS..149..251L 2003ApJS..149..251L) level energy 60- 66 F7.4 Ry EMCHF ? MCHF collection level energy (G3) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- ID Identification number 8- 24 A17 --- Level Level specification 28- 36 F9.6 Ry ENIST ? NIST level energy (G1) 39- 47 F9.6 Ry EAS Present AUTOSTRUCTURE calculation level energy (G2) 51- 59 F9.6 Ry ECHIANTI ? CHIANTI v6 level energy 60 A1 --- n_ECHIANTI [x] x for data are found to be observed, after checking the original paper (Zhang et al., 1994, Cat. J/A+A/283/319)) 65- 73 F9.6 Ry ENSD07 ? Nataraj et al. (2007, J. Phys. B: At. Mol. Opt. Phys., 40, 3153) level energy prediction with relativistic coupled-cluster theory 74 A1 --- n_ENSD07 [y] y for data from the work of Merkelis et al. (1995, Scripta, 51, 233) by using many-body perturbation theory (MBPT) -------------------------------------------------------------------------------- Global notes: Note (G1): NIST, http://physics.nist.gov/PhysRefData/ASD/levels_form.html Note (G2): Autostructure, Badnell (1986, J. Phys. B: At. Mol. Opt. Phys., 19, 3827) Note (G3): MCHF, http://nlte.nist.gov/MCHF/ -------------------------------------------------------------------------------- Acknowledgements: Guiyun Liang, gyliang(at)bao.ac.cn Gang Zhao, gzhao(at)bao.ac.cn Nigel Badnell, badnell(at)phys.strath.ac.uk
(End) Guiyun Liang [Nat. Astron. Obs., CAS], Patricia Vannier [CDS] 04-Aug-2011
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