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Table 1.

Best-fit spectroscopic parameters of observed sdA stars.

SDSS object name Plate-MJD-Fiber SDSS g (mag) Teff (K; solar z)a log g (cgs; solar z)a Teff (K; pure H)a log g (cgs; pure H)a
J123831.40−014654.3 0335-52000-0497 16.97 7932(17) 4.836(0.081) 7864 5.03
J131011.61−014233.0 0340-51990-0426 16.53 8237(10) 4.721(0.060) 8224 5.33
J221524.54−005018.2 0374-51791-0131 17.97 7763(90)b 4.529(0.038)b 7838 5.72
J090804.54−000208.8c 0470-51929-0076 15.13 8168(10) 5.039(0.036) 8130 5.33
J091416.42+004146.8 0472-51955-0499 17.39 8417(20) 5.883(0.081) 8440 5.71
J093003.42+054815.5 0992-52644-0435 18.13 8760(37) 6.240(0.105) 8656 5.52
J074939.74+194203.5 1582-52939-0406 18.04 7846(32) 5.958(0.094) 8042 6.71
J162953.16+220634.5 1658-53240-0584 18.20 8087(35) 5.833(0.122) 8057 5.08
J160410.81+062705.5 1729-53858-0213 15.10 7969(9) 5.473(0.039) 8097 5.71
J082900.96+084645.4 1758-53084-0449 17.81 8394(25) 5.995(0.100) 8195 5.16
J140119.77+351323.2 1838-53467-0506 17.64 8054(19) 4.996(0.094) 7908 5.21
J192253.84+783959.1 1857-53182-0494 14.32 7980(10) 5.328(0.032) 7904 5.24
J233258.96+490400.3 1888-53239-0477 16.26 8323(12) 6.210(0.036) 8283 5.77
J223831.92+125318.3 1892-53238-0249 15.54 7980(11) 4.816(0.056) 7999 5.03
J114224.61+374703.7 1997-53442-0225 15.09 8075(9) 5.211(0.037) 8082 5.16
J093356.45+191601.5 2361-53762-0308 18.54 8333(39) 6.088(0.127) 8126 3.75
J083054.47−035118.9 2807-54433-0499 15.15 8473(8) 4.444(0.042) 8460 5.03
J113143.46−074220.5 2861-54583-0078 15.93 7853(12) 4.635(0.064) 7637 4.61
J045309.80−041800.7 3123-54741-0483 16.99 7897(7) 4.693(0.042) 7665 4.59
J074013.22+481036.7 3668-55478-0370 16.68 7961(5) 3.932(0.021) 7748 5.34
J075644.33+502741.2 3679-55209-0229 16.56 7108(7) 4.045(0.027) 6875 5.34
J223716.61+052228.3 4291-55525-0872 19.46 8902(40) 6.695(0.017) 8856 6.66
J161831.69+385415.2 5189-56074-0177 19.67 9307(70) 7.153(0.096) 9149 6.70
J161831.69+385415.2d 5199-56067-0744 19.67 9354(54) 6.257(0.075) 9058 6.04

Notes.

(a)

We quote internal statistical uncertainties. The Teff and log g uncertainties for the pure-H models are similar to the solar z uncertainties. An analysis by Kepler et al. (2016) of the systematic uncertainties from multiple spectra indicated 5% in Teff and 0.05 dex in log g.

(b)

The fitting pipeline of Kepler et al. (2016) does not provide uncertainties for this fit because it does not agree with the cool Teff implied by the SDSS photometry for this star. We estimate the uncertainties by taking the difference between the parameters of the best fits to the tabulated Plate-MJD-Fiber and a second SDSS spectrum of this object, 3146-54773-0003.

(c)

Eclipsing binary with 7.68-h orbit (see text).

(d)

This is a second SDSS spectrum of the same object as above.

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