Size: 10745
Comment: corrections to gamma prime 2 table
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Size: 11958
Comment: Major restructuring
|
Deletions are marked like this. | Additions are marked like this. |
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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 non-resolved lambda-doubled lines merged see below (under "Lambda doubling"). Number of lines: |
== Summary of files == '''Calculated line lists''': {{{ /vald-archive/source-lists/Molecules/TiO/Plez/ }}} Original lists (Plez 2008): {{{ linelist??_all.dat.gz }}} Lists processed for non-resolved lambda doubling (Heiter 2009): {{{ linelist??_all_nodoubling.dat.gz }}} Merging code: {{{ tio_plez_rm_doubling.pro }}} '''Observed line lists''': {{{ /vald-archive/source-lists/Molecules/TiO/Phillips/ }}} Original list: {{{ TiO-Phillips-OBS.dat }}} Converted list (ascii format, same format as calculated lists): {{{ TiO-Phillips-OBS-vald.asc }}} Conversion code: {{{ tio_phillips_to_vald_ascii.f }}} == Calculated TiO data from B. Plez == TiO line lists calculated by Bertrand on 29 May 2008 with air wavelength, gf, energies for lower and upper levels, transition id and quantum numbers. '''Transitions:''' {{attachment:BP_transitions.png}} Vibrational quantum numbers from 0 to 15, rotational quantum numbers from 1 to 200. The original line lists have been processed to merge non-resolved lambda-doubled lines (with equal wave numbers) by Ulrike, 2009-02-06 (see below in section on lambda doubling). 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. The calculated lists where lambda doubling is resolved are gamma prime, delta, epsilon and E-B. '''Number of lines:''' |
Line 23: | Line 59: |
== Transitions in BP's line list == {{attachment:BP_transitions.png}} |
|
Line 35: | Line 67: |
-- UlrikeHeiter <<DateTime(2009-02-06T10:37:27+0200)>> - 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''' |
* lambda doubling in Plez 2008 calculated lists in '''gamma prime system''' |
Line 72: | Line 94: |
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 |
A line list with observed wavenumbers from Phillips has been provided by Bertrand Plez (priv. comm. 17 Sep 2008, 14 May 2009). Reference: Davis et al. 1986, ApJ 309, 449. It contains 35584 lines in the alpha, beta, gamma, gamma prime systems |
Line 83: | Line 105: |
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. There are 18 double lines with exactly the same parameters. The duplicates have been removed for these. The converted list (ascii format, same format as calculated list) is at /h19/ulrike/Molecules/Data/TiO/TiO-Phillips-OBS-vald.asc and has 35892 lines. The conversion code is at /h19/ulrike/Molecules/Data/TiO/tio_phillips_to_vald_ascii.f |
The list has been converted to an ascii format where the observed wave numbers have been converted to air wavelengths and all other line data needed for a VALD line list have been taken from the calculated list (isotope 48) by Plez (see above), by Ulrike, 2009-05-22. |
Line 96: | Line 109: |
Differences between observed and calculated wavelengths, O-C: min=-5.4Å, max=1.7Å. | Number of lines and wavelength ranges for converted list: || System || N |||| Air wavelength range [Å] || || A || 8761 || 4761 || 6277 || || B || 826 || 5597 || 5740 || || G || 21071 || 6294 || 8783 || || H || 5254 || 5847 || 6891 || || Total || 35912 |||| || |
Line 99: | Line 118: |
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). The 137 gamma prime P11/Q11/R11 lines have been discarded (not in calculated list). 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 J,,low,,<=4). 23 double entries were removed (see above). |
* 157 lines in systems other than gamma prime are not in the calculated list (all with J,,low,,<=4). * In the alpha and gamma systems, 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. There are 18 double lines with exactly the same parameters. The duplicates have been removed for these. * There are 137 gamma prime P11/Q11/R11 lines, which are not in calculated list and have been discarded. * 290 gamma prime PQR 1/2 lines have been discarded, where only one component (C or D) is in the observed list. * There is a double entry for gamma prime 0-1 J,,low,,=7 R1D. * For 20 lines in the gamma prime P1,Q1,P2,Q2,R2 lists, lambda doubling is not resolved in the calculated list. The observed wavenumber differences are very small for these lines (<=0.05 cm-1, >0 only for four lines), therefore they have been averaged. * The double line gamma prime 0-1 J,,low,,=1 R2 is not in the calculated list. * P3,Q3,R3 lines in the gamma prime system are "double", because of resolved lambda doubling in the calculated list (+958 lines). * Totals: -630 +958 |
Line 207: | Line 232: |
== Comparison of observed and calculated wavelengths == Differences between observed and calculated wavelengths, O-C: min=-5.4Å, max=1.7Å. |
Contents
TiO data
Summary of files
Calculated line lists:
/vald-archive/source-lists/Molecules/TiO/Plez/
Original lists (Plez 2008): linelist??_all.dat.gz
Lists processed for non-resolved lambda doubling (Heiter 2009): linelist??_all_nodoubling.dat.gz
Merging code: tio_plez_rm_doubling.pro
Observed line lists:
/vald-archive/source-lists/Molecules/TiO/Phillips/
Original list: TiO-Phillips-OBS.dat
Converted list (ascii format, same format as calculated lists): TiO-Phillips-OBS-vald.asc
Conversion code: tio_phillips_to_vald_ascii.f
Calculated TiO data from B. Plez
TiO line lists calculated by Bertrand on 29 May 2008 with air wavelength, gf, energies for lower and upper levels, transition id and quantum numbers.
Transitions:
Vibrational quantum numbers from 0 to 15, rotational quantum numbers from 1 to 200.
The original line lists have been processed to merge non-resolved lambda-doubled lines (with equal wave numbers) by Ulrike, 2009-02-06 (see below in section on lambda doubling).
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.
The calculated lists where lambda doubling is resolved are gamma prime, delta, epsilon and E-B.
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
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).
lambda doubling in Plez 2008 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 line list with observed wavenumbers from Phillips has been provided by Bertrand Plez (priv. comm. 17 Sep 2008, 14 May 2009). Reference: Davis et al. 1986, ApJ 309, 449.
It contains 35584 lines in the alpha, beta, gamma, gamma prime systems with range:
wavenumber(cm-1) |
wavelength(Å) |
|
|
vacuum |
air |
20997.64 |
4762.440 |
4761.109 |
11383.24 |
8784.845 |
8782.433 |
Isotope: 48Ti (see Davis et al. 1986, IV.a p. 452)
The list has been converted to an ascii format where the observed wave numbers have been converted to air wavelengths and all other line data needed for a VALD line list have been taken from the calculated list (isotope 48) by Plez (see above), by Ulrike, 2009-05-22.
The list has been sorted by wavelength after running the conversion code.
Number of lines and wavelength ranges for converted list:
System |
N |
Air wavelength range [Å] |
|
A |
8761 |
4761 |
6277 |
B |
826 |
5597 |
5740 |
G |
21071 |
6294 |
8783 |
H |
5254 |
5847 |
6891 |
Total |
35912 |
|
Explanation for different numbers of lines in original and converted list:
157 lines in systems other than gamma prime are not in the calculated list (all with Jlow<=4).
- In the alpha and gamma systems, 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. There are 18 double lines with exactly the same parameters. The duplicates have been removed for these.
- There are 137 gamma prime P11/Q11/R11 lines, which are not in calculated list and have been discarded.
- 290 gamma prime PQR 1/2 lines have been discarded, where only one component (C or D) is in the observed list.
There is a double entry for gamma prime 0-1 Jlow=7 R1D.
For 20 lines in the gamma prime P1,Q1,P2,Q2,R2 lists, lambda doubling is not resolved in the calculated list. The observed wavenumber differences are very small for these lines (<=0.05 cm-1, >0 only for four lines), therefore they have been averaged.
The double line gamma prime 0-1 Jlow=1 R2 is not in the calculated list.
- P3,Q3,R3 lines in the gamma prime system are "double", because of resolved lambda doubling in the calculated list (+958 lines).
- Totals: -630 +958
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 |
7,9,13,16,85 |
60,67 |
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 |
8,19,75,82,84 |
78 |
72,76,79,80,83,85 |
||
|
|
|
|
|
|
|
|
|
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 |
Comparison of observed and calculated wavelengths
Differences between observed and calculated wavelengths, O-C: min=-5.4Å, max=1.7Å.