2019ApJS..245....9S


Query : 2019ApJS..245....9S

2019ApJS..245....9S - Astrophys. J., Suppl. Ser., 245, 9-9 (2019/November-0)

Relativistic MR-MP energy levels for L-shell ions of iron.

SANTANA J.A., PENA-COTTO E.L., MORALES BUTLER E.J., BEIERSDORFER P. and BROWN G.V.

Abstract (from CDS):

A comprehensive set of level energies is provided for the valence and K-vacancy states of the ions Fe XVII, Fe XVIII, Fe XIX, Fe XX, Fe XXI, Fe XXII, Fe XXIII, and Fe XXIV. Level energies were calculated with the relativistic Multi-Reference Moller-Plesset Perturbation Theory method (MR-MP). The data set includes level energies coming from the configurations 1s22(s,p)q, 1s22(s,p)q–1nl, 1s12(s,p)q+1, 1s12(s,p)qnl, 2(s,p)q+2, and 2(s,p)q+1nl, where 1 <= q <= 8, n <= 5, and l <= 3. The results have been compared with data from the National Institute of Standards and Technology (NIST) online database and with previous calculations. In general, the deviation from the NIST-recommended values is below 0.6 and 1.0 eV for valence and K-vacancy level energies, respectively. However, we identify numerous outliers among the NIST-recommended values. The extensive data set presented here greatly augments the amount of available reference level energies in the NIST database for L-shell ions of Fe, and we expect our data set to ease line identification and confirm level designations.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): Atomic data benchmarking - Atomic spectroscopy - Atomic physics - Line positions - Spectroscopy

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ACO 426 ClG 03 19 47.6 +41 30 54           ~ 2508 1
2 * alf CMi SB* 07 39 18.11950 +05 13 29.9552 0.82 0.79 0.37 -0.05 -0.28 F5IV-V+DQZ 1925 0
3 V* GP Vel HXB 09 02 06.8608812864 -40 33 16.899168060 6.85 7.37 6.87 6.31 6.05 B0.5Ia 1588 0
4 NGC 3783 Sy1 11 39 01.7096819040 -37 44 19.009642992   12.46 13.43 11.33 12.1 ~ 1765 1
5 MCG-06-30-015 Sy1 13 35 53.7691256160 -34 17 44.160716796   13.89 13.61 8.9   ~ 1559 0
6 IRAS 13349+2438 Sy1 13 37 18.7199358192 +24 23 03.319883484     15.0     ~ 410 0
7 HD 153919 HXB 17 03 56.7725629224 -37 50 38.913331452 6.06 6.78 6.51 6.08 5.90 O6Iafcp 851 0
8 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0

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