Table C.3
IRT fluxes from PEPSI spectra.
Star | M-K class | Teff (K) | log g (dex) | [Fe/H] (dex) | v sin i (km s−1) | (B–V)0 (mag) | ℱIRT–1 | ℱIRT–2 | ℱIRT–3 |
---|---|---|---|---|---|---|---|---|---|
(106 ergs cm−2 s−1) | |||||||||
Giants | |||||||||
32 Gem | A9 III | 7240 | 1.45 | −0.28 | 5.0 | 0.33 | 3.4905 | 2.3904 | 2.5544 |
HD 140283 | F3 IV | 5788 | 3.75 | −2.48 | 6.0 | 0.50 | 4.1208 | 3.0600 | 3.3142 |
η Boo | G0 IV | 6099 | 3.94 | +0.26 | 11 | 0.55 | 2.2494 | 1.5045 | 1.6306 |
ζ Her | G0 IV | 5759 | 3.69 | +0.02 | 3.1 | 0.61 | 2.0750 | 1.3677 | 1.4829 |
δ CrB | G3.5 III | 5362 | 3.29 | −0.12 | 5.2 | 0.77 | 1.6175 | 1.0950 | 1.1428 |
μ Her | G5 IV | 5633 | 4.02 | +0.31 | 2 | 0.70 | 1.7522 | 1.1614 | 1.2252 |
β Boo | G8 III | 5100 | 2.8 | −0.1 | 1 | 0.87 | 0.9447 | 0.5494 | 0.5970 |
ϵ Vir | G8 III | 5060 | 2.97 | +0.15 | 2 | 0.90 | 0.9813 | 0.5855 | 0.6312 |
HD 122563 | G8III | 4642 | 1.32 | −2.67 | 7.0 | 0.95 | 1.5216 | 0.9204 | 1.0394 |
β Gem | K0 IIIb | 4810 | 2.55 | +0.02 | 3 | 1.00 | 0.8799 | 0.5218 | 0.5588 |
HD 107328 | K0 IIIb | 4508 | 2.3 | −0.48 | 2 | 1.13 | 0.6167 | 0.3365 | 0.3511 |
α UMa | K0 III | 4660 | 2.46 | −0.20 | 6 | 1.10 | 0.6325 | 0.3613 | 0.3816 |
α Ari | K1 IIIb | 4498 | 2.4 | −0.25 | 4.2 | 1.14 | 0.6584 | 0.3721 | 0.3931 |
α Boo | K1.5 III | 4308 | 1.7 | −0.55 | 4.2 | 1.23 | 0.5253 | 0.2851 | 0.3013 |
7 Psc | K2 III | 4351 | 1.73 | −0.70 | 7.0 | 1.20 | 0.6126 | 0.3367 | 0.3560 |
μ Leo | K2 III | 4519 | 2.43 | +0.27 | 4.5 | 1.27 | 0.4468 | 0.2489 | 0.2597 |
γ Aql | K3 II | 4210 | 1.63 | −0.29 | 8 | 1.30 | 0.3083 | 0.1802 | 0.1855 |
β UMi | K4 III | 4030 | 1.83 | −0.29 | 8 | 1.43 | 0.3124 | 0.1678 | 0.1756 |
α Tau | K5 III | 3921 | 1.17 | −0.20 | 3.5 | 1.54 | 0.2607 | 0.1435 | 0.1488 |
μ UMa | M0 III | 3899 | 1.0 | 0.00 | 7.5 | 1.57 | 0.2370 | 0.1333 | 0.1367 |
γ Sge | M0 III | 3904 | 1.06 | −0.26 | 6 | 1.60 | 0.2124 | 0.1159 | 0.1216 |
α Cet | M1.5 III | 3738 | 0.66 | −0.24 | 7 | 1.70 | 0.1881 | 0.1095 | 0.1100 |
Dwarfs | |||||||||
α CMa | A1 V | 9850 | 4.3 | +0.40 | 16.7 | 0.00 | 9.9535 | 9.0056 | 8.3011 |
σ Boo | F4 V | 6756 | 4.28 | −0.36 | 7.3 | 0.34 | 4.2224 | 2.9811 | 3.1723 |
HD 49933 | F5 V-IV | 6628 | 4.19 | −0.39 | 5 | 0.36 | 4.0838 | 2.9441 | 3.0992 |
α CMi | F5 V-IV | 6582 | 3.98 | −0.02 | 5.4 | 0.42 | 3.1220 | 2.0978 | 2.2249 |
θ UMa | F7 V | 6217 | 3.83 | −0.17 | 8.8 | 0.48 | 2.8152 | 1.8675 | 2.0413 |
HD 84937 | F8 V | 6356 | 4.1 | −2.0 | 5 | 0.38 | 4.9229 | 3.5873 | 3.9031 |
β Vir | F9 V | 6093 | 4.08 | +0.13 | 3.4 | 0.52 | 2.4794 | 1.6909 | 1.8066 |
HD 22879 | F9 V | 5868 | 4.45 | −0.80 | 3.0 | 0.52 | 2.9752 | 2.1878 | 2.3040 |
HD 159222 | G1 V | 5856 | 4.39 | +0.16 | 2 | 0.61 | 2.2225 | 1.5620 | 1.6471 |
16 Cyg A | G1.5 V | 5849 | 4.28 | +0.08 | 5 | 0.61 | 2.2240 | 1.5606 | 1.6462 |
HD 101364 | G2 V | 5771 | 4.34 | −0.01 | 1 | 0.62 | 2.2710 | 1.6254 | 1.6832 |
HD 82943 | G2 V | 5918 | 4.34 | +0.23 | 1.4 | 0.59 | 2.2340 | 1.5333 | 1.6082 |
18 Sco | G2 V | 5824 | 4.42 | +0.03 | 2.1 | 0.61 | 2.3081 | 1.6577 | 1.7123 |
Sun (11/2016) | G2 V | 5771 | 4.44 | 0.00 | 2 | 0.63 | 2.3047 | 1.6363 | 1.6862 |
51 Peg | G2.5 V | 5758 | 4.32 | +0.18 | 2.0 | 0.62 | 2.1585 | 1.5179 | 1.5758 |
16 Cyg B | G3 V | 5807 | 4.35 | +0.07 | 2.3 | 0.62 | 2.2205 | 1.5726 | 1.6386 |
70 Vir | G4 V-IV | 5473 | 3.94 | −0.06 | 1 | 0.73 | 1.8243 | 1.2563 | 1.3129 |
μ Cas | G5 V | 5358 | 4.49 | −0.83 | 4.1 | 0.66 | 2.3501 | 1.7607 | 1.8201 |
HD 103095 | G8 V | 5235 | 4.72 | −1.33 | 3.1 | 0.68 | 2.2667 | 1.7027 | 1.7640 |
τ Cet | G8.5 V | 5463 | 4.52 | −0.51 | 3 | 0.70 | 2.0853 | 1.5612 | 1.6198 |
ϵ Eri | K2 V | 5130 | 4.63 | −0.08 | 4 | 0.86 | 1.8753 | 1.5881 | 1.5170 |
HD 192263 | K2 V | 4975 | 4.61 | +0.04 | 3.3 | 0.94 | 1.5477 | 1.2374 | 1.2102 |
HD 128311 | K3 V | 4967 | 4.67 | +0.16 | 3.2 | 0.94 | 1.6079 | 1.3509 | 1.2797 |
HD 82106 | K3 V | 4861 | 4.59 | −0.02 | 3.0 | 0.99 | 1.4735 | 1.2390 | 1.1824 |
61 Cyg A | K5 V | 4398 | 4.63 | −0.13 | 1 | 1.23 | 0.9089 | 0.6748 | 0.6819 |
61 Cyg B | K7 V | 4174 | 4.68 | −0.21 | 3 | 1.38 | 0.7832 | 0.5904 | 0.5982 |
Notes. The first column gives the name for the target, listing first the giants and then the dwarfs, followed by the spectral class on the second column. Columns 3–6 list the stellar parameters effective temperature, surface gravity, metallicity, and v sin i value, respectively. The seventh column has the (B–V)0 colour. The flux values for each of the IRT lines are given in columns 8–10.
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