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Show constraint information
J/A+A/547/A108/table6
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Iron line selection for the M6 stellar parameter determination (26 rows)
 
El

lambda
nm
Elow
eV
log(gf)

Source

Fe I843.957 4.549-0.587K07
Fe I847.174 4.956-1.037K07
Fe I852.667 4.913-0.760BWL
Fe I852.785 5.020-1.625K07
Fe I857.180 5.010-1.414K07
Fe I859.295 4.956-1.066K07
Fe I859.883 4.386-1.089BWL
Fe I860.105 5.112-1.577K07
Fe I861.394 4.988-1.247K07
Fe I863.241 4.103-2.341K07
Fe I869.945 4.955-0.380BWL
Fe I872.914 3.415-2.871K07
Fe I874.743 3.018-3.176K07
Fe I879.052 4.988-0.586BWL
Fe I879.807 4.985-1.895K07
Fe I881.451 5.067-1.793K07
Fe I881.689 4.988-2.203K07
Fe I883.402 4.218-2.558K07
Fe I884.674 5.010-0.777K07
Fe I889.140 5.334-1.108K07
Fe II611.332 3.221-4.230RU
Fe II614.774 3.889-2.827RU
Fe II641.692 3.892-2.877RU
Fe II643.26810.930-1.236RU
Fe II645.638 3.903-2.185RU
Fe II651.608 2.891-3.432RU
J/A+A/547/A108/table7
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Lines used in the A1 analysis to determine abundances for Star 1 (HR 1457) (32 rows)
 
Z

lambda
nm
log(gf)

Source

Elow
cm-1
abund

14568.448-1.650GARZ39955.053 6.95
14569.043-1.870GARZ39760.285 7.10
14570.110-2.050GARZ39760.285 7.08
14577.215-1.750GARZ40991.884 7.04
14579.307-2.060GARZ39760.285 7.15
20558.875 0.210NBS20371.000 4.83
20559.011-0.710NBS20335.360 5.23
20559.446-0.050NBS20349.260 4.81
20560.128-0.690NBS20371.000 5.13
20615.602-2.200NBS20335.360 5.88
20645.560-1.350NBS20349.260 5.48
20817.329-0.546K8839349.080 5.90
20820.375-0.848K8836575.119 5.90
20829.218-0.391K8839340.080 5.80
22546.047-2.880SK 386.874 4.55
22556.271-2.870MFW 7255.369 4.55
22802.484-1.140MFW15156.787 4.45
22806.825-1.280MFW15108.121 4.65
22841.229-1.483MFW18482.860 4.55
22867.527-1.669MFW 8602.340 4.50
22868.299-1.941MFW 8492.421 4.50
22869.233-2.295MFW 8436.618 4.70
22873.471-2.384MFW 8492.421 4.70
26552.554-1.330FMW34121.580 6.70
26552.890-2.020FMW36079.366 7.30
26552.916-2.730FMW29371.811 7.10
26553.275-2.150FMW28819.946 6.70
26554.394-1.140FMW34017.098 6.70
26555.798-1.280FMW36079.366 6.65
26556.021-1.190FMW35767.561 6.75
26829.351-2.126K8838678.032 6.90
26832.705-1.525FMW17726.981 6.70
J/A+A/547/A108/table8
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Fe lines used in the A1 analysis to determine abundances for Star 3 (artificial star) (5 rows)
 
lambda
nm
log(gf)

Source

Elow
cm-1
abund

1549.034-4.574O17726.987 7.85
1558.826 0.323K9451359.489 7.70
1561.115-3.822K9427523.001 7.65
1564.851-0.714K9443763.977 7.90
1565.283-0.476K9450377.905 7.80
J/A+A/547/A108/table9
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Lines used by the A2 participants (65 rows)
 
Ion

n_

lambda
nm
log(gf)

Source

EW1
0.1pm
EW2
0.1pm
26.00*490.514-2.050FMW 73.63 30.33
26.01  492.393-1.320FMW    
26.00  492.477-2.220FMW107.96183.82
24.00  493.634-0.340MFW110.10 82.99
26.00*496.258-1.290FMW 52.20  
28.00  501.094-0.870FMW    
26.00  504.422-2.150FMW169.70181.76
26.00  504.982-1.420FMW    
26.00*505.465-2.140FMW 25.21 25.79
22.00*506.406-0.270MFW 2.45 2.50
26.00*508.334-2.958FMW 1.16 11.24
26.00  509.078-0.400FMW   4.39
28.00*509.441-1.080FMW 23.30 22.79
26.00*512.735-3.307FMW 72.89 74.44
26.00*514.174-2.150FMW 73.17 91.99
26.00*514.373-3.790FMW 27.32 28.61
22.00*514.547-0.574MFW    
26.00*515.191-3.322FMW 83.65104.74
26.00*515.906-0.820FMW 74.80 80.40
26.00  518.006-1.260FMW    
26.00*518.791-1.260FMW 56.57 37.12
26.00  519.495-2.090FMW 73.31113.68
26.00*519.547 0.018K94 85.83 21.61
22.01  521.154-1.356K88    
22.00*521.970-2.292MFW174.09173.95
26.00  522.985-0.241K94   26.94
26.01  523.463-2.050FMW    
26.00  524.250-0.840FMW114.71172.90
26.01*525.693-4.250K88 57.75  
26.00  526.331-0.970FMW129.66135.07
24.00*528.718-0.907MFW 61.55 19.62
24.00  529.670-1.400MFW214.13203.87
27.00*535.205 0.060FMW 62.30 50.28
26.00  536.162-1.430FMW269.68225.63
26.00*537.371-0.860FMW 82.82 97.37
26.00  537.958-1.480FMW102.03113.47
26.00  538.634-1.770FMW    
26.00*538.948-0.410FMW 20.50 85.97
28.00  539.233-1.320FMW   4.94
26.00  612.025-5.950FMW112.24113.17
26.00*615.938-1.970FMW 26.72 40.58
26.00  622.674-2.220FMW 23.82 6.31
26.01*636.946-4.253K88    
26.00*639.254-4.030FMW 64.58 67.31
21.01  660.460-1.480MFW142.65127.39
26.00*672.536-2.300FMW 61.93 8.42
26.00*848.198-1.647K94 39.32 30.20
14.00*850.222-1.260KP 14.75 1.58
26.00  851.510-2.073O152.76132.81
26.00  858.225-2.133O146.53141.05
Result truncated to 50 rows
J/A+A/547/A108/table10
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Lines analysed by the A5 team (60 rows)
 
El

lambda
nm
Elow
eV
log(gf)

EW
0.1pm
Source

Fe I491.0325 4.191-0.459143.3K88
Fe I491.6662 3.929-2.960 26.8FMW
Fe I491.8020 4.231-1.360 68.9FMW
Fe I492.7417 3.573-1.990 78.1FMW
Fe I494.5636 4.209-1.510 82.5FMW
Fe I495.2639 4.209-1.665 73.6K88
Fe I501.0300 2.559-4.577 11.0K88
Fe I505.8496 3.641-2.830 45.1FMW
Fe I513.7395 4.177-0.400116.9FMW
Fe I523.6205 4.186-1.720 51.3FMW
Fe I526.2608 4.320-2.280 30.4FMW
Fe I530.0412 4.593-1.750 19.1FMW
Fe I531.5065 4.371-1.550 70.2FMW
Fe I532.2041 2.279-3.030156.2FMW
Fe I532.6799 4.415-2.100 31.5FMW
Fe I536.4858 4.445 0.230136.7FMW
Fe I538.5579 3.694-2.970 32.9FMW
Fe I538.6959 3.642-2.624 84.9K88
Fe I615.1617 2.176-3.299152.8FMW
Fe I616.5361 4.143-1.550 82.5FMW
Fe I621.3429 2.223-2.660160.5FMW
Fe I625.3829 4.733-1.660 54.6FMW
Fe I627.1276 3.332-2.950 65.7FMW
Fe I630.1498 3.653-0.745143.1K88
Fe I630.2494 3.687-1.203112.1K88
Fe I630.7856 3.642-3.535 33.6K88
Fe I631.5809 4.076-1.710 72.3FMW
Fe I632.2690 2.588-2.426151.1FMW
Fe I633.6823 3.687-1.050145.7FMW
Fe I640.8016 3.687-1.048161.0K88
Fe I641.1647 3.653-0.820148.9FMW
Fe I648.1869 2.279-2.984151.1FMW
Fe I651.8365 2.830-2.750131.2FMW
Fe I660.9110 2.559-2.692158.4FMW
Fe I660.9676 0.990-4.936153.7K88
Fe I663.3746 4.559-0.780 81.4FMW
Fe I664.6932 2.609-3.990 81.6FMW
Fe I664.8079 1.011-5.275118.3FMW
Fe I666.3437 2.424-2.479161.5FMW
Fe I666.7417 2.453-4.400 56.7FMW
Fe I670.3568 2.759-3.160100.2FMW
Fe I670.5101 4.607-1.496 63.1K88
Fe I671.0316 1.484-4.880125.8FMW
Fe I672.5353 4.103-2.300 30.8FMW
Fe I673.3151 4.638-1.580 57.4FMW
Fe I673.9520 1.557-4.950 97.0FMW
Fe I843.9563 4.549-0.698132.7K88
Fe I847.1739 4.956-0.863 67.7K88
Fe I848.1982 4.187-1.631 60.1K88
Fe I852.6667 4.913-0.513 86.4K88
Result truncated to 50 rows
J/A+A/547/A108/table11
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Measured CO 3-0 lines in Star 4 (artificial star) from the T analysis (14 rows)
 
lambda
nm
log(gf)

Elow
cm-1
logW/nu

Ident

1560.082-7.797 886.903-4.69612C16O 3-0 R 21
1560.447-7.823 806.383-4.63212C16O 3-0 R 20
1560.839-7.850 729.678-4.69112C16O 3-0 R 19
1561.257-7.877 656.789-4.67912C16O 3-0 R 18
1561.533-7.2495055.604-4.73212C16O 3-0 R 51
1561.702-7.907 587.721-4.62112C16O 3-0 R 17
1562.002-7.2345252.117-4.78412C16O 3-0 R 52
1562.499-7.2205452.275-4.74412C16O 3-0 R 53
1563.748-8.038 349.698-4.64512C16O 3-0 R 13
1564.157-7.1796074.532-4.79112C16O 3-0 R 56
1564.326-8.076 299.766-4.69512C16O 3-0 R 12
1564.930-8.116 253.667-4.70712C16O 3-0 R 11
1565.561-8.159 211.404-4.72912C16O 3-0 R 10
1566.763-7.1256954.739-4.90212C16O 3-0 R 60
J/A+A/547/A108/star1
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Observed optical spectrum for Albedaran (HR 1457)
spectrum
(plot) (114979 rows)
 
lambda
0.1nm
Flux

4900.003 8.131e-01
4900.034 8.241e-01
4900.064 8.455e-01
4900.095 8.490e-01
4900.126 8.328e-01
4900.157 8.123e-01
4900.187 7.807e-01
4900.218 7.474e-01
4900.249 6.992e-01
4900.280 6.376e-01
4900.310 5.430e-01
4900.341 4.404e-01
4900.372 3.495e-01
4900.403 3.237e-01
4900.434 3.523e-01
4900.464 4.385e-01
4900.495 5.547e-01
4900.526 6.421e-01
4900.557 6.740e-01
4900.587 6.697e-01
4900.618 6.862e-01
4900.649 6.817e-01
4900.680 6.295e-01
4900.710 4.911e-01
4900.741 3.267e-01
4900.772 2.100e-01
4900.803 1.660e-01
4900.833 1.900e-01
4900.864 2.461e-01
4900.895 2.956e-01
4900.926 3.177e-01
4900.956 2.936e-01
4900.987 2.562e-01
4901.018 2.784e-01
4901.048 3.838e-01
4901.079 5.254e-01
4901.110 6.310e-01
4901.140 6.687e-01
4901.172 6.911e-01
4901.202 7.208e-01
4901.233 7.626e-01
4901.264 7.832e-01
4901.295 7.732e-01
4901.325 7.387e-01
4901.356 6.844e-01
4901.387 6.340e-01
4901.417 5.798e-01
4901.448 4.945e-01
4901.479 4.194e-01
4901.509 4.322e-01
Result truncated to 50 rows
J/A+A/547/A108/star2
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Observed optical spectrum for Menkar (HR 911)
spectrum
(plot) (114973 rows)
 
lambda
0.1nm
Flux

4900.026 6.555e-01
4900.057 6.034e-01
4900.089 5.575e-01
4900.119 5.045e-01
4900.150 4.391e-01
4900.180 4.203e-01
4900.211 4.601e-01
4900.242 5.510e-01
4900.273 6.323e-01
4900.303 6.620e-01
4900.334 6.374e-01
4900.365 5.912e-01
4900.396 5.837e-01
4900.426 6.067e-01
4900.457 6.212e-01
4900.488 5.854e-01
4900.518 5.182e-01
4900.549 4.851e-01
4900.580 5.379e-01
4900.611 6.517e-01
4900.641 7.938e-01
4900.672 8.737e-01
4900.703 9.017e-01
4900.734 8.957e-01
4900.764 8.748e-01
4900.795 8.697e-01
4900.826 8.462e-01
4900.856 7.971e-01
4900.887 7.426e-01
4900.918 7.006e-01
4900.948 6.912e-01
4900.979 7.137e-01
4901.010 7.483e-01
4901.041 7.737e-01
4901.071 7.628e-01
4901.102 7.513e-01
4901.133 7.586e-01
4901.163 7.882e-01
4901.194 8.159e-01
4901.225 8.342e-01
4901.255 8.272e-01
4901.286 8.112e-01
4901.317 7.772e-01
4901.348 7.269e-01
4901.378 6.482e-01
4901.409 5.734e-01
4901.440 5.576e-01
4901.470 5.619e-01
4901.501 5.712e-01
4901.532 5.359e-01
Result truncated to 50 rows
J/A+A/547/A108/star3
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Simulated observed H-band spectrum for Star 3 (T=4257K, logg=1.47, M=1.165M, [Fe/H]=-0.4)
spectrum
(plot) (2101 rows)
 
lambda
0.1nm
Flux

15456.007 0.924594
15456.110 0.895154
15456.213 0.886720
15456.316 0.916134
15456.419 0.926298
15456.522 0.941416
15456.625 0.949626
15456.728 0.968006
15456.831 0.991316
15456.934 0.992409
15457.037 0.991612
15457.141 0.987177
15457.244 0.987038
15457.347 0.991190
15457.450 0.992743
15457.553 0.995338
15457.656 1.009889
15457.759 1.000419
15457.862 1.011121
15457.965 1.006275
15458.068 0.995413
15458.171 1.005134
15458.274 0.997911
15458.377 0.985913
15458.480 0.994238
15458.583 0.978214
15458.686 0.990292
15458.789 0.998648
15458.892 1.012441
15458.995 1.003786
15459.099 0.999372
15459.202 0.996339
15459.305 0.990124
15459.408 0.993637
15459.511 0.977036
15459.614 0.955701
15459.717 0.912506
15459.820 0.898243
15459.923 0.882264
15460.026 0.897393
15460.129 0.928884
15460.232 0.963829
15460.335 0.989343
15460.438 0.996324
15460.541 0.990799
15460.645 1.000442
15460.748 1.001578
15460.851 0.988763
15460.954 0.981132
15461.057 0.980400
Result truncated to 50 rows
J/A+A/547/A108/star4
Post annotation
Comparative modelling of cool giants spectra (Lebzelter+, 2012)
Simulated observed H-band spectrum for Star 4 (T=3280K, logg=0.06, M=1.509M, [Fe/H]=+0.1)
spectrum
(plot) (2101 rows)
 
lambda
0.1nm
Flux

15456.007 0.809149
15456.110 0.769156
15456.213 0.742427
15456.316 0.754086
15456.419 0.759952
15456.522 0.749855
15456.625 0.785922
15456.728 0.855046
15456.831 0.919516
15456.934 0.958356
15457.037 0.961642
15457.141 0.983463
15457.244 0.943445
15457.347 0.940400
15457.450 0.931669
15457.553 0.946127
15457.656 0.967389
15457.759 0.970436
15457.862 0.969926
15457.965 0.983620
15458.068 0.995217
15458.171 0.978290
15458.274 0.968000
15458.377 0.933016
15458.480 0.939195
15458.583 0.921649
15458.686 0.968219
15458.789 0.984235
15458.892 0.979517
15458.995 0.979196
15459.099 0.989973
15459.202 0.993004
15459.305 0.980650
15459.408 0.965244
15459.511 0.900023
15459.614 0.809580
15459.717 0.703405
15459.820 0.653914
15459.923 0.663434
15460.026 0.680766
15460.129 0.739339
15460.232 0.847715
15460.335 0.926647
15460.438 0.968113
15460.541 0.988601
15460.645 0.990145
15460.748 0.984631
15460.851 0.961183
15460.954 0.920071
15461.057 0.898088
Result truncated to 50 rows
elapse time 1

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