atomic data summary paper (trac #230)

reported by: @CloudyLex

Title:
Atomic decay data for modeling K lines of iron peak and light odd-Z elements Authors:
Palmeri, P.; Quinet, P.; Mendoza, C.; Bautista, M. A.; García, J.; Witthoeft, M. C.; Kallman, T. R. Affiliation:
AA(Astrophysique et Spectroscopie (ASPECT), Université de Mons - UMONS, 20 place du Parc, 7000, Mons, Belgium patrick.palmeri@umons.ac.be), AB(Astrophysique et Spectroscopie (ASPECT), Université de Mons - UMONS, 20 place du Parc, 7000, Mons, Belgium; IPNAS, Université de Liège, Campus du Sart Tilman, Bât. B15, 4000, Liège, Belgium pascal.quinet@umons.ac.be), AC(Centro de Física, Instituto Venezolano de Investigaciones Científicas (IVIC), PO Box 20632, Caracas, 1020A, Venezuela claudio@ivic.gob.ve), AD(Department of Physics, Western Michigan University, Kalamazoo, MI, 49008, USA manuel.bautista@wmich.edu), AE(Department of Astronomy, University of Maryland, College Park, MD, 20742, USA javier@astro.umd.edu; NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA), AF(NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA michael.c.witthoeft@nasa.gov), AG(NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA timothy.r.kallman@nasa.gov) Publication:
Astronomy & Astrophysics, Volume 543, id.A44 (A&A Homepage) Publication Date:
07/2012 Origin: EDP Sciences Astronomy Keywords: atomic data, atomic processes, line: formation, X-rays: general DOI:
10.1051/0004-6361/201219438 Bibliographic Code: 2012A&A...543A..44P 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.

Full Tables 9 and 10 are available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/543/A44

Migrated from https://www.nublado.org/ticket/230

{
    "status": "new",
    "changetime": "2019-02-04T13:07:06Z",
    "_ts": "1549285626580696",
    "description": "Title:\t\n\tAtomic decay data for modeling K lines of iron peak and light odd-Z elements\nAuthors:\t\n\tPalmeri, P.; Quinet, P.; Mendoza, C.; Bautista, M. A.; Garc\u00eda, J.; Witthoeft, M. C.; Kallman, T. R.\nAffiliation:\t\n\tAA(Astrophysique et Spectroscopie (ASPECT), Universit\u00e9 de Mons - UMONS, 20 place du Parc, 7000, Mons, Belgium patrick.palmeri@umons.ac.be), AB(Astrophysique et Spectroscopie (ASPECT), Universit\u00e9 de Mons - UMONS, 20 place du Parc, 7000, Mons, Belgium; IPNAS, Universit\u00e9 de Li\u00e8ge, Campus du Sart Tilman, B\u00e2t. B15, 4000, Li\u00e8ge, Belgium pascal.quinet@umons.ac.be), AC(Centro de F\u00edsica, Instituto Venezolano de Investigaciones Cient\u00edficas (IVIC), PO Box 20632, Caracas, 1020A, Venezuela claudio@ivic.gob.ve), AD(Department of Physics, Western Michigan University, Kalamazoo, MI, 49008, USA manuel.bautista@wmich.edu), AE(Department of Astronomy, University of Maryland, College Park, MD, 20742, USA javier@astro.umd.edu; NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA), AF(NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA michael.c.witthoeft@nasa.gov), AG(NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA timothy.r.kallman@nasa.gov)\nPublication:\t\n\tAstronomy & Astrophysics, Volume 543, id.A44 (A&A Homepage)\nPublication Date:\t\n\t07/2012\nOrigin:\t\n\tEDP Sciences\nAstronomy Keywords:\t\n\tatomic data, atomic processes, line: formation, X-rays: general\nDOI:\t\n\t10.1051/0004-6361/201219438\nBibliographic Code:\t\n\t2012A&A...543A..44P\nAbstract\nComplete 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.\n\nFull Tables 9 and 10 are available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/543/A44 ",
    "reporter": "gary",
    "cc": "",
    "resolution": "",
    "time": "2012-07-04T12:12:47Z",
    "component": "atomic/molecular data base",
    "summary": "atomic data summary paper",
    "priority": "good to do",
    "keywords": "",
    "version": "trunk",
    "milestone": "no milestone",
    "owner": "nobody",
    "type": "enhancement"
}

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atomic data summary paper (trac #230) #232