J/ApJS/202/15              UV spectrum of CrII              (Sansonetti+, 2012)

Comprehensive observations of the ultraviolet spectrum and improved energy levels for singly ionized chromium (Cr II). Sansonetti C.J., Nave G., Reader J., Kerber F. <Astrophys. J. Suppl. Ser., 202, 15 (2012)> =2012ApJS..202...15S 2012ApJS..202...15S
ADC_Keywords: Atomic physics ; Line Profiles ; Spectra, ultraviolet Keywords: atomic data - line: identification - methods: laboratory - techniques: spectroscopic - ultraviolet: general Abstract: We report new observations of the spectrum of singly ionized chromium (CrII) in the region 1142-3954Å. The spectra were recorded with the National Institute of Standards and Technology 10.7m normal-incidence vacuum spectrograph and FT700 vacuum ultraviolet Fourier transform spectrometer. More than 3600 lines are classified as transitions among 283 even and 368 odd levels. The new spectral data are used to re-optimize the energy levels, reducing their uncertainties by a typical factor of 20. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 59 651 Optimized energy levels of Cr II table2.dat 137 3600 Classified lines of Cr II -------------------------------------------------------------------------------- See also: J/ApJS/196/24 : Electron-impact excitation of CrII (Wasson+, 2011) J/A+A/511/A68 : Transitions of CrII (Gurell+, 2010) J/A+A/524/A35 : Effective collision strengths of CrII (Wasson+, 2010) J/ApJ/700/720 : The 236.6-5400.0nm spectrum of CrI (Wallace+, 2009) J/ApJ/667/1267 : CrI transition probabilities (Sobeck+, 2007) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 21 A21 --- Conf Configuration 24- 28 A5 --- Term Term 31- 32 I2 --- 2J [1/17] J value 33- 34 A2 --- --- [/2] 37- 47 F11.4 cm-1 E Energy level value 50- 55 F6.4 cm-1 e_E Uncertainty in Energy 58- 59 I2 --- Nl Number of lines observed for level -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Int Intensity 7- 9 A3 --- Comm Codes describing line character (1) 11- 20 F10.5 0.1nm lambda Wavelength λ in Angstroms (2) 23- 29 F7.5 0.1nm e_lambda Uncertainty in lambda 33- 42 F10.4 cm-1 sigma Wavenumber σ 45- 50 F6.4 cm-1 e_sigma Uncertainty in sigma 55- 68 A14 --- Conf.0 Even level configuration 70- 73 A4 --- Term.0 Even level term 76- 77 I2 --- 2J0 [1/17] Even level J value 78- 79 A2 --- --- [/2] 81 A1 --- --- [-] Dash to visually offset even/odd sides 83-103 A21 --- Conf.1 Odd level configuration 105-109 A5 --- Term.1 Odd level term 112-113 I2 --- 2J1 [1/17] Odd J value 114-115 A2 --- --- [/2] 119-128 F10.5 0.1nm lam.c Calculated wavelength (2) 131-137 F7.5 0.1nm e_lam.c Uncertainty in CWave -------------------------------------------------------------------------------- Note (1): Code as follows: a = Asymmetric c = Complex h = blend on high side l = blend on low side p = perturbed by close line w = wide x = extrapolated wavelength # = omitted from level optimization * = multiply classified Note (2): Vacuum wavelength for λ<2000Å; standard air wavelength for λ>2000Å -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 18-Oct-2012
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