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Table A.2

List of lines observed in the CRIRES spectrum of HD 154708.

λ(obs) Rc(obs) Element λ(lab) log    gf χlow χup Sourcea Notes
[Å] [Å] [cm-1] [cm-1]

10747.4 0.94 component
10749.39 0.80 Si i 10749.378  −0.272 39760.285 49060.601 NIST4
10751.4 0.93 component
10769.7 0.98 ?
10771.0 0.975 ?
10809.8 0.92 component
10811.1 0.84 Mg i 10811.053  + 0.024 47957.045 57204.305 NIST4
Mg i 10811.076  −0.137 47957.027 57204.267 NIST4
Mg i 10811.097  −1.038 47957.045 57204.267 NIST4
Mg i 10811.122  −1.036 47957.027 57204.228 NIST4
Mg i 10811.158  −0.305 47957.058 57204.228 NIST4
10812.3 0.91 component
10814.4 0.99 ?
10825.2 0.92 component
10827.1 0.75 Si i 10827.089  + 0.239 39955.053 49188.617 NIST4
10829.2 0.93 component
10834.3 0.96 component blend telluric
10836.1 0.925 Dy ii 10835.94  −0.77 16177.40 25343.42 VALD
10837.8 0.965 component
10839.0 0.98 Ca i 10838.97  + 0.238 39340.080 48563.522 K07Ca
10842.5 0.92 component
10844.12 0.83 Si i 10843.858  + 0.220 47284.061 56503.346 NIST4
10845.7 0.92 component
10848.6 0.98 ?
10867.3 0.94: guessed component blend
10868.65 0.82 Si i 10868.790  −0.010 49933.775 59131.912 MB99 blend telluric
10870.35 0.90 guessed component
10868.0 0.88 guessed component blend
10869.55 0.78 Si i 10869.536  + 0.286 40991.884 50189.389 NIST4
10870.8 0.90 component
10882.02 0.94 ?
10883.5 0.90 ?
10884.85 0.92 ?
10885.45 0.90 Si i 1088.5333  −0.100 49850.83 59034.988 MB99
10914.3 0.85 component
10915.15 0.81 Sr ii 10914.887  −0.638 14555.900 23715.190 WA
10916.1 0.88 component
10936.7 0.74 component ?
10938.0 0.70 H i 10938.086  + 0.002 9742.304 109250.343 NIST4
10939.6 0.74 component ?
10950.8 0.96 ?
10951.95 0.94 Mg ii 10951.778 ?  −0.219 71491.063 80619.500 NIST4
10953.2 0.935 Mg i 10953.320 ?  −0.863 47841.119 56968.271 NIST4
10954.6 0.94 ?
10954.85 0.92 ?
10956.2 0.91 ?
10958.0 0.96 ?
10979.2 0.84 Si i 10979.308  −0.562 39955.053 49060.601 NIST4 blend telluric
10980.6 0.98 ?
10981.85 0.90 Si i 10982.058  −0.270 49933.775 59037.043 MB99
10983.6 0.90 ?
10985.4 0.96 ?
11015.7 0.95 Cr i 11015.679  −0.42 27820.198 36895.681 K10Cr1
11016.2 0.87 component
11017.9 0.83 Si i 11017.966  + 0.310 50054.800 59128.400 MB99
11019.3 0.91 component
15528.0-15530. 0.97 ? broad
15532.3 0.965 ?
15533.55 0.960 ?
15536.7 0.97 ? broad
15542.15 0.98 Fe i 15542.079  −0.336 45509.149 51941.537 K07
15556.0 0.96 component ?
H i 15556.467  −1.166 101823.904 109250.343 NIST4 continuum
Si i 15557.779  −0.540 48102.323 54528.220 NIST4 not observed !
15559.8 0.955 component ?
15621.70 0.96 Fe i 15621.654  + 0.586 44677.003 51076.625 K07
15631.90 0.96 Fe i 15631.948  + 0.122 43163.323 49558.731 K07
15648.55 0.985 Fe i 15648.510  −0.596 43763.977 50152.616 K07
15653.00 0.99 Fe i 15652.874  −0.170 50377.905 56764.763 K07
15661.95 0.98 Fe i 15662.016  + 0.382 47005.503 53388.633 K07
15665.25 0.985 Fe i 15665.243  −0.338 48221.321 54603.136 K07
15715.80 0.97 Ce iii 15715.837  −3.080 0.000 8361.000 BIE blend telluric
15727.40 0.99 C i 15727.376  −0.682 77679.831 84036.327 NIST4
15740.00 0.98 ? on telluric wing
15746.0-15748.0 0.915 component? broad
Mg i 15748.886  −0.338 47844.414 54192.335 NIST4 not observed
Mg i 14748.998  + 0.140 47844.414 54192.294 NIST4 not observed
15749.4 0.90 component
15750.3 0.91 component
15762.90 0.94 ?
15764.45 0.89 component
15766.0 ? Mg i 15765.645  −1.514 47851.162 54192.335 NIST4 blend telluric
? Mg i 15765.747  −0.337 47851.162 54192.294 NIST4
? Mg i 15765.842  + 0.411 47851.162 54192.256 NIST4
15767.1 0.90 component
15769.35 0.92 Fe i 15769.423  + 0.700 44677.003 51016.657 K07
15770.50 0.93 Fe i 15770.619  + 0.448 50807.994 57147.167 K07 blend telluric
15822.70 0.98 Fe i 15822.817  + 0.181 45509.149 51827.410 K07
15827.30 0.98 Si i 15827.213  −0.690 57198.027 63514.533 MB99
15830.0 0.96 component ?
15832.7 0.945 component ?
Si i 15833.602  −0.450 50189.389 56503.346 MB99 not observed !
15834.4 0.955 component ?
15836.4 0.945 component ?
15844.70 0.92 component
15847.70 0.73 Ce iii 15847.550  −1.030 1528.320 7836.720 BIE
15850.80 0.88 component

Notes. The adopted parameters are Teff = 6800 K, log    g = 4.11 (Nesvacil et al. 2008). The radial velocity shift between the observed wavelength positions of the spectral lines and their laboratory wavelengths is 15 km s-1.

(a)

BIE: Biémont (2011, priv. comm.),

MB99: Meléndez & Barbuy (1999), NIST4: http://www.nist.gov/pml/data/asd.cfm, K07: http://kurucz.cfa.harvard.edu/atoms/2600/gf2600.pos, K07Si: http://kurucz.cfa.harvard.edu/atoms/1400/gf1400.pos, VALD: http://vald.astro.univie.ac.at/~vald/php/vald.php, WA: Warner (1968).

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