Co XXV - VERSION 11.0

The CHIANTI database has the following primary ASCII files for this ion:

co_25.elvlc (energy levels)

contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

 

 Observed energies:
Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
NIST Atomic Spectra Database (ver. 5.0), [Online]. Available: http://physics.nist.gov/


Theoretical energies:
Liang, G. and Badnell, N.R., A&A 528, A69 (2011)
DOI: 10.1051/0004-6361/201016417

Produced for the CHIANTI database v.8 by G. Del Zanna  2014 Dec 17



 
 -1

contains wavelengths, gf and A values of the transitions. The wavelengths are based on the experimental energy levels and should be the best available. Wavelengths calculated from the theoretical energies are of an indeterminate accuracy and their values are presented as negative values of the calculated wavelength.

 

Observed energies:
Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
NIST Atomic Spectra Database (ver. 5.0), [Online]. Available: http://physics.nist.gov/

Theoretical energies, gf and A-values:
Liang, G. and Badnell, N.R., A&A 528, A69 (2011)
DOI: 10.1051/0004-6361/201016417


Note: only transitions with a branching ratio above 10^-5 
have been retained.

The autoionization rates have been calculated using AUTOSTRUCTURE v.24.24 and 
the same set of scaling parameters used by Liang and Badnell  

Produced for the CHIANTI database v.8 by Giulio Del Zanna 10 Mar 2015
 
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
%File processed with wgfa_tidy by pryoung on 31-May-2023

co_25.scups (electron collision data)

contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

 


Produced for the CHIANTI database v.8 by G. Del Zanna  2014 Dec 17

DOI: 10.1051/0004-6361/201016417                                  
Liang, G. and Badnell, N.R., A&A 528, A69 (2011)                  
 Data from

(proton collisional data) Not available in this VERSION.

The html table below contains the radiative data of the brightest lines sorted in wavelength

co_25_table.html (html table)