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TiO line lists calculated by Bertrand. <<TableOfContents>>
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'''Comment on "lambda doubling" (BP, 28 Jan 2009):''' = 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
<<BR>>
For files with lambda-doubled lines merged see below.

Number of lines:

||Isotope ||N,,merg,,||N,,orig,,||
||46 || 8193347 ||11140205 ||
||47 || 8194614 ||11141521 ||
||48 || 8195512 ||11142777 ||
||49 || 8196355 ||11143980 ||
||50 || 8197133 ||11144857 ||
||total ||40976961 ||55713340 ||

N,,orig,, ... original lists<<BR>>
N,,merg,, ... lambda-doubled lines merged

== Transitions in BP's line list ==

{{attachment:BP_transitions.png}}

== Lambda doubling ==

-- BertrandPlez 28 Jan 2009:
Line 8: Line 34:

-- UlrikeHeiter <<DateTime(2009-02-06T10:37:27+0200)>> - 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 alpha, beta, gamma, gammaprime transitions (systems)
with range:
||wavenumber(cm^-1^) ||wavelength(Å) ||
||20997.630 ||4762.4422 ||
||14729.730 ||6788.9907 ||

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

BP_transitions.png

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 alpha, beta, gamma, gammaprime transitions (systems) with range:

wavenumber(cm-1)

wavelength(Å)

20997.630

4762.4422

14729.730

6788.9907

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

ValdWiki: TiO (last edited 2012-05-04 17:16:40 by UlrikeHeiter)