Contents
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 non-resolved lambda-doubled lines merged see below (under "Lambda doubling").
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 ... non-resolved 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 with same wavenumbers 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
In the calculated lists, parity is given by the syml and symu quantum numbers, which can be 1 or -1. In the merged lists, syml and symu are set to 0 for the merged lines.
lambda doubling in calculated lists in gamma prime system
- P1,Q1,R1: lambda doubling resolved for all lines
P2,Q2,R2: lambda doubling resolved for Jlow>~10
P3,Q3,R3: lambda doubling resolved for Jlow>=3
"resolved" here means: wavenumber difference >=0.001
wavenumber (wn) difference for calculated lambda-doubled lines in gamma prime system
- P1,P2,R1,R2 (all v-v):
for even Jlow: wn(syml=-1) > wn(syml=1),
for odd Jlow vice versa
- Q1,Q2: reverse of P
for even Jlow: wn(syml=1) > wn(syml=-1),
for odd Jlow vice versa
- PQR 3: reverse of PQR 1,2
- for the actual values for PQR 1 and 2 see the plots below (the values are the same for each of the three v-v combinations 0-0, 1-0, 0-1), and compare to the plots for observed lambda-doubled lines further down
- P1,P2,R1,R2 (all v-v):
Observed wavenumbers
A separate list with observed wavenumbers from Phillips (Bertrand Plez, priv. comm. 17 Sep 2008, 14 May 2009) and calculated other values from Plez (from the list with lambda-doubled lines merged), has been generated. Reference: Davis et al. 1986, ApJ 309, 449.
It contains lines in the alpha, beta, gamma, gamma prime 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)
The original list is at /h19/ulrike/Molecules/Data/TiO/TiO-Phillips-OBS.dat and has 35584 lines.
Content: "Obs", vupp, vlow, Jlow, "+", branch, ".0000E+00", wavenumber, ".000", system
There are five "double" lines with same quantum numbers and branch names but slightly different wavenumbers. The wavenumbers for these have been averaged for the converted list.
The converted list (ascii format, same format as calculated list) is at /h19/ulrike/Molecules/Data/TiO/TiO-Phillips-OBS-vald.asc and has 35920 lines.
The conversion code is at /h19/ulrike/Molecules/Data/TiO/tio_phillips_to_vald_ascii.f
The list has been sorted by wavelength after running the conversion code.
Differences between observed and calculated wavelengths, O-C: min=-5.4Å, max=1.7Å.
Explanation for different numbers of lines in original and converted list: P3,Q3,R3 lines in the gamma prime system (H, X-B) are "double", because of resolved lambda doubling in the calculated list (+958 lines). About 300 gamma prime PQR 1/2 lines have been discarded, where only one component (C or D) is in the observed list. 157 lines from other systems are not in the calculated list (all with Jlow<=4).
Observed lines in beta system
v-v |
branch |
Jlow,min |
Jlow,max |
Jlow missing |
|
|
|
|
|
0-0 |
P |
4 |
99 |
94 |
1-1 |
P |
2 |
100 |
66,88,91,92,93,95 |
2-2 |
P |
2 |
90 |
8,10,12,14,76,81,83 |
|
|
|
|
|
0-0 |
Q |
2 |
100 |
4 |
1-1 |
Q |
1 |
100 |
2,4,96 |
2-2 |
Q |
3 |
100 |
7,78,82,83,84,89,90,91 |
|
|
|
|
|
0-0 |
R |
2 |
100 |
|
1-1 |
R |
2 |
98 |
7 |
2-2 |
R |
2 |
92 |
5,26,42,62,64,70,74,75,84 |
Observed lines in gamma prime system
observed lines in gamma prime system, P1,Q1,R1 branches (C/D pairs for each v-v and Jlow), Jlow values:
vupp-vlow |
branch |
Jlow,min |
Jlow,max |
Jlow missing C+D |
Jlow missing C |
Jlow missing D |
|
|
|
|
|
|
|
0-0 |
P1 |
3 |
131 |
|
3,4,5,6,13,23 |
29,104,130,131 |
1-0 |
P1 |
2 |
107 |
98 |
21,77 |
15,63,103,107 |
0-1 |
P1 |
2 |
145 |
89,93,109,110,120,123 |
2,10,14,28,29,63,104, 126,131,135,138,139, 140,144,145 |
23,62,68,71,72,77,84,98, 99,111,125,129,130,136 |
|
|
|
|
|
|
|
0-0 |
Q1 |
1 |
141 |
2 |
1,12,119,138,139,140,141 |
4,7,118 |
1-0 |
Q1 |
1 |
120 |
|
1,104,105,112,114,118 |
|
0-1 |
Q1 |
2 |
144 |
94,138 |
11,104,107,114,125,127, 128,129,130,132,133,143,144 |
8,77,100,102,122,124 |
|
|
|
|
|
|
|
0-0 |
R1 |
1 |
122 |
96 |
5,6,19,64,87 |
1,2,76,83,84,90,94,100, 107,>=110 |
1-0 |
R1 |
1 |
135 |
126 |
28,43,78,82,95 |
116,119,121,128,131 |
0-1 |
R1 |
1 |
150 |
119,122,124,148 |
22,58,78,87,100,105,106, 108,111,114,115,130, 137,>=144 |
5,38,39,53,81,103,116, 117,121,125,128,141 (7 double) |
observed lines in gamma prime system, P1,Q1,R1 branches, wavenumber differences between C and D lines:
observed lines in gamma prime system, P2,Q2,R2 branches (C/D pairs for each v-v and Jlow), Jlow values:
vupp-vlow |
branch |
Jlow,min |
Jlow,max |
Jlow missing C+D |
Jlow missing C |
Jlow missing D |
||
|
|
|
|
|
|
|
|
|
0-0 |
P2 |
11 |
106 |
16 |
|
51, >=85 |
||
1-0 |
P2 |
3 |
88 |
|
3,4,6,15,34,35 |
5,16,82,88 |
||
0-1 |
P2 |
5 |
90 |
7,9,13,16 |
60,67,85 |
69,71,74,76, >=84 |
||
|
|
|
|
|
|
|
|
|
0-0 |
Q2 |
7 |
107 |
28 |
|
>=84 |
||
1-0 |
Q2 |
2 |
91 |
|
90 |
<=9, 35,74,91 |
||
0-1 |
Q2 |
4 |
85 |
8,19,75 |
78,82,84 |
72,76,79,80,82,83,84,85 |
||
|
|
|
|
|
|
|
|
|
0-0 |
R2 |
11 |
106 |
19,27,32 |
83,96,97 |
48,80, >=82 |
||
1-0 |
R2 |
4 |
90 |
|
18,36,81 |
4,5,6,8,22,25,37,41,50,61,75,89,90 |
||
0-1 |
R2 |
1 |
91 |
88 |
18,20,67,76 |
44,48,82,83, >=85 |
observed lines in gamma prime system, P2,Q2,R2 branches, wavenumber differences between C and D lines:
vupp-vlow |
branch |
Jlow,min |
Jlow,max |
wn(C)-wn(D) = delta |
|
|
|
|
|
0-0 |
P2 |
11 |
45 |
= 0 |
|
|
46 |
84 |
< 0 |
1-0 |
P2 |
7 |
12 |
|delta| < 0.07 |
|
|
13 |
42 |
> 0 |
|
|
43 |
51 |
|delta| < 0.07 |
|
|
52 |
87 |
< 0 |
0-1 |
P2 |
5 |
44 |
= 0 (39: -0.81) |
|
|
45 |
83 |
< 0 |
|
|
|
|
|
0-0 |
Q2 |
7 |
44 |
= 0 |
|
|
45 |
83 |
< 0 |
1-0 |
Q2 |
10 |
37 |
> 0 |
|
|
38 |
50 |
|delta| < 0.07 |
|
|
51 |
89 |
< 0 |
0-1 |
Q2 |
4 |
43 |
= 0 |
|
|
44 |
81 |
< 0 |
|
|
|
|
|
0-0 |
R2 |
11 |
45 |
= 0 (36: +0.19) |
|
|
46 |
81 |
< 0 |
1-0 |
R2 |
13 |
44 |
> 0 |
|
|
59 |
88 |
< 0 |
0-1 |
R2 |
1 |
42 |
= 0 |
|
|
43 |
84 |
< 0 |
observed lines in gamma prime system, P3,Q3,R3 branches:
vupp-vlow |
branch |
Jlow,min |
Jlow,max |
Jlow missing |
|
|
|
|
|
0-0 |
P3 |
4 |
121 |
10,14,19,31,68 |
1-0 |
P3 |
7 |
95 |
63,89,93 |
0-1 |
P3 |
4 |
103 |
7,19,20,52,79,82,93,97 |
|
|
|
|
|
0-0 |
Q3 |
11 |
130 |
|
1-0 |
Q3 |
4 |
109 |
5,10,14,17,19 |
0-1 |
Q3 |
6 |
112 |
10,25,54,87,94,102,104,110 |
|
|
|
|
|
0-0 |
R3 |
11 |
139 |
21,25,30,65,77,118,119,123,124,134,138 |
1-0 |
R3 |
5 |
124 |
99,100,103,119,122 |
0-1 |
R3 |
3 |
127 |
5,14,20,70,94,95,96,98,100,113,123 |