J/ApJS/234/40    Be-like ions from BII to NeVII transition data    (Wang+, 2018)

Benchmarking atomic data for astrophysics: Be-like ions between B II and Ne VII. Wang K., Chen Z.B., Zhang C.Yu, Si R., Jonsson P., Hartman H., Gu M.F., Chen C.Y., Yan J. <Astrophys. J. Suppl. Ser., 234, 40 (2018)> =2018ApJS..234...40W 2018ApJS..234...40W
ADC_Keywords: Atomic physics Keywords: atomic data ; atomic processes Abstract: Large-scale self-consistent multiconfiguration Dirac-Hartree-Fock (MCDHF) and relativistic configuration interaction (RCI) calculations are reported for the n≤6 levels in Be-like ions from BII to NeVII. Effects from electron correlation are taken into account by means of large expansions in terms of a basis of configuration state functions, and a complete and accurate data set of excitation energies; lifetimes; wavelengths; electric dipole, magnetic dipole, electric quadrupole, and magnetic quadrupole line strengths; transition rates; and oscillator strengths for these levels is provided for each ion. Comparisons are made with available experimental and theoretical results. The uncertainty of excitation energies is assessed to be 0.01% on average, which makes it possible to find and rule out misidentifications and aid new line identifications involving high-lying levels in astrophysical spectra. The complete data set is also useful for modeling and diagnosing astrophysical plasmas. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 129 714 Excitation energies and lifetimes for all the levels of Be-like table5.dat 68 8405 Transition data for Be-like ions from BII to NeVII -------------------------------------------------------------------------------- See also: J/ApJS/91/461 : EUV spectrum of solar active region (Thomas+, 1994) J/A+AS/126/281 : Solar disk spectrum (660-1175A) (Curdt+ 1997) J/A+A/375/591 : SUMER Spectral Atlas of Solar Disk Features (Curdt+, 2001) J/ApJS/156/105 : Transitions in L-shell ions of Fe and Ni (Gu+, 2005) J/A+A/559/A100 : Boron isoelectronic sequence data (Jonsson+, 2013) J/A+A/564/A24 : Carbon isoelectronic sequence data (Ekman+, 2014) J/ApJS/215/26 : Energy levels & transition rates of C-like ions (Wang+, 2014) J/A+A/582/A61 : N-like ions atomic data (Radziute+, 2015) J/ApJS/218/16 : Energy levels & transition rates of Be-like ions (Wang+, 2015) J/ApJS/227/16 : Energy levels & transition rates for F-like ions (Si+, 2016) J/ApJS/226/14 : MBPT calc. for Ne-like ions (CrXV to KrXXVII) (Wang+, 2016) J/ApJS/223/3 : Energies & radiative transition (ArXII - ZnXXIV) (Wang+, 2016) J/ApJS/229/37 : Energy levels & transition rates of O-like ions (Wang+, 2017) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Z [5/10] Atomic number 4- 6 I3 --- Key [1/138] Key number 8- 36 A29 --- Level Configuration and LSJ level 38- 42 A5 --- Jpi J level parity π; o=odd or e=even 44- 50 I7 cm-1 Energy [0/1522569] Energy levels, MCDHF/RCI calculation 52- 60 E9.3 s Lifetime [0/589.5] Lifetimes, MCDHF/RCI calculation 62-129 A68 --- LS-comp Mixing coefficients of LSJ coupling scheme (1) -------------------------------------------------------------------------------- Note (1): The first number is the expansion coefficient for the leading LS-composition. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Z [5/10] Atomic number 4- 6 I3 --- j [3/138] Upper level 11- 13 I3 --- i [1/125] Lower level 15- 25 E11.5 0.1nm Wave [65.7/6195790] Wavelength; Angstroms 27- 28 A2 --- Type Transition type 30- 38 E9.3 --- Str [3.9e-08/3306] Line strength; Atomic units 40- 48 E9.3 --- gf [9.1e-12/17.6] Weighted oscillator strengths 50- 58 E9.3 s-1 A [5.6e-08/333200000000] Transition rates 60- 68 E9.3 --- BR [2.1e-09/1] Radiative branching ratio -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 27-Mar-2018
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