| Size: 1663 Comment: added number of lines | Size: 3347 Comment: corrected obs wave range | 
| Deletions are marked like this. | Additions are marked like this. | 
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| <<TableOfContents>> | |
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| <<BR>> | |
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| N,,merg,, ... original lists<<BR>> N,,orig,, ... lambda-doubled lines merged | N,,orig,, ... original lists<<BR>> N,,merg,, ... lambda-doubled lines merged | 
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| == Observed wavenumbers == A separate list with observed wavenumbers from Phillips (Bertrand Plez, priv. comm. 17 Sep 2008) and calculated other values from Plez (from the list with lambda-doubled lines merged), will be generated. Reference: Davis et al. 1986, ApJ 309, 449. The original list is at /h19/ulrike/Molecules/Data/TiO/TiO-Phillips-OBS.dat It contains about 35000 lines in the alpha, beta, gamma, gammaprime systems with range: ||wavenumber(cm^-1^) ||wavelength(Å) || ||20997.64 ||4762.440 || ||11383.24 ||8784.845 || Isotope: ^48^Ti (see Davis et al. 1986, IV.a p. 452) Content: "Obs", vupp, vlow, Jlow, "+", branch, ".0000E+00", wavenumber, ".000", system There are a few "double" lines with same quantum numbers and branch names (but different wavenumbers). The wavenumbers for these will be averaged. '''beta system:''' ||v-v || branch || J,,low,, range || J,,low,, missing || || || || || || ||0-0 || P || 4<=Jlow<= 99 || 94 || ||1-1 || P || 2<=Jlow<=100 || 66,88,91,92,93,95 || ||2-2 || P || 2<=Jlow<= 90 || 8,10,12,14,76,81,83 || || || || || || ||0-0 || Q || 2<=Jlow<=100 || 4 || ||1-1 || Q || 1<=Jlow<=100 || 2,4,96 || ||2-2 || Q || 3<=Jlow<=100 || 7,78,82,83,84,89,90,91 || || || || || || ||0-0 || R || 2<=Jlow<=100 || || ||1-1 || R || 2<=Jlow<= 98 || 7 || ||2-2 || R || 2<=Jlow<= 92 || 5,26,42,62,64,70,74,75,84|| | 
TiO data
TiO line lists calculated by Bertrand on 29 May 2008. The files are in Uppsala at /h5/plez/TiOVALD/linelist/linelist??_all.dat.gz 
 For files with lambda-doubled lines merged see below. 
Number of lines:
| Isotope | Nmerg | Norig | 
| 46 | 8193347 | 11140205 | 
| 47 | 8194614 | 11141521 | 
| 48 | 8195512 | 11142777 | 
| 49 | 8196355 | 11143980 | 
| 50 | 8197133 | 11144857 | 
| total | 40976961 | 55713340 | 
Norig ... original lists
 Nmerg ... lambda-doubled lines merged 
Transitions in BP's line list
 
 
Lambda doubling
-- BertrandPlez 28 Jan 2009:
Some transitions are affected by Lambda-doubling. In that case there are 2 sublevels that give rise to transitions, and if the separation is large enough, they appear in the list as 2 lines with the same parameters except for the parity of the upper and lower level, and a slightly different wavenumber. The degeneracy of these sublevels is 2*J+1. When the Lambda-doubling is too small there are 2 lines with exactly the same data (except the parities). One way to compact the list is to merge these lines and double the gf-value 2*(2*J+1)*f.
For some transitions Lambda-doubling does not exist (if Lambda=0, i.e if one of the states is a sigma state).
-- UlrikeHeiter 2009-02-06 08:37:27 - Lambda-doubled lines have been merged according to BP's comment above.
The new files are in Uppsala at /h19/ulrike/Molecules/Data/TiO/linelist??_all_nodoubling.dat.gz
The merging code is at /h19/ulrike/Molecules/Data/TiO/tio_plez_rm_doubling.pro
Observed wavenumbers
A separate list with observed wavenumbers from Phillips (Bertrand Plez, priv. comm. 17 Sep 2008) and calculated other values from Plez (from the list with lambda-doubled lines merged), will be generated. Reference: Davis et al. 1986, ApJ 309, 449.
The original list is at /h19/ulrike/Molecules/Data/TiO/TiO-Phillips-OBS.dat
It contains about 35000 lines in the alpha, beta, gamma, gammaprime systems with range:
| wavenumber(cm-1) | wavelength(Å) | 
| 20997.64 | 4762.440 | 
| 11383.24 | 8784.845 | 
Isotope: 48Ti (see Davis et al. 1986, IV.a p. 452)
Content: "Obs", vupp, vlow, Jlow, "+", branch, ".0000E+00", wavenumber, ".000", system
There are a few "double" lines with same quantum numbers and branch names (but different wavenumbers). The wavenumbers for these will be averaged.
beta system:
| v-v | branch | Jlow range | Jlow missing | 
| 
 | 
 | 
 | 
 | 
| 0-0 | P | 4<=Jlow<= 99 | 94 | 
| 1-1 | P | 2<=Jlow<=100 | 66,88,91,92,93,95 | 
| 2-2 | P | 2<=Jlow<= 90 | 8,10,12,14,76,81,83 | 
| 
 | 
 | 
 | 
 | 
| 0-0 | Q | 2<=Jlow<=100 | 4 | 
| 1-1 | Q | 1<=Jlow<=100 | 2,4,96 | 
| 2-2 | Q | 3<=Jlow<=100 | 7,78,82,83,84,89,90,91 | 
| 
 | 
 | 
 | 
 | 
| 0-0 | R | 2<=Jlow<=100 | 
 | 
| 1-1 | R | 2<=Jlow<= 98 | 7 | 
| 2-2 | R | 2<=Jlow<= 92 | 5,26,42,62,64,70,74,75,84 |