THE SPECTRUM AND TERM ANALYSIS OF CO III MEASURED USING FOURIER TRANSFORM AND GRATING SPECTROSCOPY

被引:7
作者
Smillie, D. G. [1 ]
Pickering, J. C. [1 ]
Nave, G. [2 ]
Smith, P. L. [3 ]
机构
[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England
[2] NIST, Gaithersburg, MD 20899 USA
[3] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
关键词
atomic data; line: identification; line: profiles; methods: laboratory: atomic; DOUBLY IONIZED ATOMS; IRON-GROUP ELEMENTS; VACUUM-ULTRAVIOLET; ENERGY-LEVELS; CONFIGURATIONS; WAVELENGTHS; 3RD; UV; SPECTROMETER; MULTIPLET;
D O I
10.3847/0067-0049/223/1/12
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The spectrum of Co III has been recorded in the region 1562-2564 angstrom (64,000 cm(-1)-39,000 cm(-1)) by Fourier transform (FT) spectroscopy, and in the region 1317-2500 angstrom (164,000 cm(-1)-40,000 cm(-1)) using a 10.7 m grating spectrograph with phosphor image plate detectors. The spectrum was excited in a cobalt-neon Penning discharge lamp. We classified 514 Co III lines measured using FT spectroscopy, the strongest having wavenumber uncertainties approaching 0.004 cm(-1) (approximately 0.2 m angstrom at 2000 angstrom, or 1 part in 10(7)), and 240 lines measured with grating spectroscopy with uncertainties between 5 and 10 m angstrom. The wavelength calibration of 790 lines of Raassen & Orti Ortin and 87 lines from Shenstone has been revised and combined with our measurements to optimize the values of all but one of the 288 previously reported energy levels. Order of magnitude reductions in uncertainty for almost two-thirds of the 3d(6)4s and almost half of the 3d(6)4p revised energy levels are obtained. Ritz wavelengths have been calculated for an additional 100 forbidden lines. Eigenvector percentage compositions for the energy levels and predicted oscillator strengths have been calculated using the Cowan code.
引用
收藏
页数:11
相关论文
共 50 条
[1]   Advanced Spectral Library (ASTRAL): Cool stars edition [J].
Ayres, T. R. .
ASTRONOMISCHE NACHRICHTEN, 2013, 334 (1-2) :105-108
[2]  
Cowan R. D., 1981, THEORY ATOMIC STRUCT
[4]  
Davis S.P., 2001, FOURIER TRANSFORM SP
[5]   The NIST FT700 Vacuum Ultraviolet Fourier Transform Spectrometer: applications in ultraviolet spectrometry and radiometry [J].
Griesmann, U ;
Kling, R ;
Burnett, JH ;
Bratasz, L .
ULTRAVIOLET ATMOSPHERIC AND SPACE REMOTE SENSING: METHODS AND INSTRUMENTATION II, 1999, 3818 :180-188
[6]   CALCULATIONS OF TRANSITION-PROBABILITIES FOR FORBIDDEN LINES IN THE 3D7 GROUND CONFIGURATIONS OF CO-III AND NI-IV [J].
HANSEN, JE ;
RAASSEN, AJJ ;
UYLINGS, PHM .
ASTROPHYSICAL JOURNAL, 1984, 277 (01) :435-443
[7]   A STUDY OF FITTED AND CALCULATED PARAMETER VALUES IN III, IV, V AND VI SPECTRA OF THE IRON GROUP ELEMENTS [J].
HANSEN, JE ;
RAASSEN, AJJ .
PHYSICA B & C, 1981, 111 (01) :76-101
[8]   RADIOMETRIC CHARACTERIZATION OF A PENNING DISCHARGE IN THE VACUUM-ULTRAVIOLET [J].
HEISE, C ;
HOLLANDT, J ;
KLING, R ;
KOCK, M ;
KUHNE, M .
APPLIED OPTICS, 1994, 33 (22) :5111-5117
[9]   New developments in the radiance calibration of deuterium lamps in the UV and VUV spectral range at the PTB [J].
Hollandt, J ;
Becker, U ;
Paustian, W ;
Richter, M ;
Ulm, G .
METROLOGIA, 2000, 37 (05) :563-566
[10]  
Iglesias L., 1979, Optica Pura y Aplicada, V12, P63