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Table 4

Equivalent widths of water lines in mÅ as observed and the equivalent widths from synthetic spectra for the stars calculated for standard marcs models.

808.632 cm-1 814.675 cm-1 815.300 cm-1
HR Name Teff Wmod Wobs log (Wobs/λ) Wmod Wobs log (Wobs/λ) Wmod Wobs log (Wobs/λ)
[K] [mÅ] [mÅ] [mÅ] [mÅ] [mÅ] [mÅ]
HR8775 β Peg 3448 ± 42 506 – – 598 648 −5.28 511 – –
HR4910 δ Vir 3602 ± 44 324 612 −5.31 359 301 −5.61 301 873 −5.15
HR6056 δ Oph 3721 ± 47 211 444 −5.45 216 301 −5.61 135 858 −5.16
HR4069 μ UMa 3793 ± 47 143 459 −5.44 136 331 −5.57 135 752 −5.21
HR3705 α Lyn 3836 ± 47 114 321 −5.59 105 – – 94.8 617 −5.30
HR1457 α Tau 3871 ± 48 106 – – 101 – – 91.8 662 −5.27
HR3748 α Hya 4060 ± 60 23.9 – – 22.2 – – 18.1 141 −5.94
HR5340 α Boo 4226 ± 53 6.40 113 −6.04 4.52 150 −5.91 4.36 196 −5.79
HR5854 α Ser 4558 ± 56 – – – – 0.00 −∞ 0.00 0.00 0.00
HR2990 β Gem 4858 ± 60 – 0.00 −∞ – 0.00 −∞ 0.00 0.00 0.00
815.900 cm-1 816.450 cm-1 816.687 cm-1
HR8775 β Peg 3448 ± 42 713 826 −5.17 302 765 −5.20 703 1290 −4.98
HR4910 δ Vir 3602 ± 44 446 555 −5.34 150 495 −5.39 455 1012 −5.08
HR6056 δ Oph 3721 ± 47 285 466 −5.42 76.0 420 −5.46 312 884 −5.14
HR4069 μ UMa 3793 ± 47 186 421 −5.46 38.7 285 −5.63 221 930 −5.12
HR3705 α Lyn 3836 ± 47 147 481 −5.40 27.7 255 −5.68 186 705 −5.24
HR1457 α Tau 3871 ± 48 140 421 −5.46 26.4 255 −5.68 173 750 −5.21
HR3748 α Hya 4060 ± 60 32.2 165 −5.87 5.10 – – 43.5 225 −5.74
HR5340 α Boo 4226 ± 53 6.62 146 −5.92 – 67.1 −6.25 11.0 315 −5.59
HR5854 α Ser 4558 ± 56 – 0.00 −∞ – 0.00 −∞ – 0.00 −∞
HR2990 β Gem 4858 ± 60 – 0.00 −∞ – 0.00 −∞ – 0.00 −∞
817.157 cm -1 817.209 cm-1 818.425 cm-1
HR8775 β Peg 3448 ± 42 612 1228 −5.00 610 1138 −5.03 1025 1612 −4.88
HR4910 δ Vir 3602 ± 44 395 1063 −5.06 356 464 −5.42 694 1269 −4.98
HR6056 δ Oph 3721 ± 47 263 764 −5.20 207 374 −5.51 492 1120 −5.04
HR4069 μ UMa 3793 ± 47 184 884 −5.14 126 389 −5.50 365 985 −5.09
HR3705 α Lyn 3836 ± 47 150 659 −5.27 95.8 299 −5.61 311 1015 −5.08
HR1457 α Tau 3871 ± 48 141 524 −5.37 91.2 225 −5.74 289 836 −5.16
HR3748 α Hya 4060 ± 60 30.9 – – 19.4 – – 75.6 343 −5.55
HR5340 α Boo 4226 ± 53 8.39 240 −5.71 3.64 135 −5.96 20.6 0.00 −5.51
HR5854 α Ser 4558 ± 56 – 0.00 −∞ – 0.00 −∞ 2.65 0.00 −∞
HR2990 β Gem 4858 ± 60 – 0.00 −∞ – 0.00 −∞ – 0.00 −∞
819.046 cm -1 819.932 cm-1 820.583 cm-1
HR8775 β Peg 3448 ± 42 420 655 −5.27 505 1562 −4.89 833 – –
HR4910 δ Vir 3602 ± 44 256 537 −5.36 338 1071 −5.06 527 787 −5.19
HR6056 δ Oph 3721 ± 47 158 313 −5.59 236 684 −5.25 342 683 −5.25
HR4069 μ UMa 3793 ± 47 102 343 −5.55 170 684 −5.25 229 564 −5.33
HR3705 α Lyn 3836 ± 47 79.5 – – 141 640 −5.28 184 549 −5.35
HR1457 α Tau 3871 ± 48 75.6 209 −5.77 131 580 −5.32 173 – –
HR3748 α Hya 4060 ± 60 16.2 – – 31.5 – – 39.4 – –
HR5340 α Boo 4226 ± 53 4.37 118 −6.02 8.43 149 −5.91 10.7 178 −5.83
HR5854 α Ser 4558 ± 56 – – – – – – – – –
HR2990 β Gem 4858 ± 60 – 0.00 −∞ – 0.00 −∞ – 0.00 −∞

Notes. A measure of the lines’ observational line strength calculated as log Wobs/λ is also given. Wobs is the observed equivalent width and λ the wavelength.

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