Table B.1
Stellar parameters and lithium content for our sample of 148 stars (first 5 lines only).
Name | EPIC | RA(2000) | Dec(2000) | V | J–K![]() |
Period | Amp. | WLi | rms | Teff | A[Li] | rms | Bin. |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(deg) | (deg) | (mag) | (mag) | (d) | (mag) | mÅ | mÅ | K | dex | dex | |||
PELS 123 | 211002011 | 53.30793 | 23.00647 | 11.98 | 0.591 | 7.575758 | 0.028 | 132 | 4 | 4945 | 1.95 | 0.084 | |
PELS 124 | 210990525 | 53.88203 | 22.82362 | 9.86 | 0.289 | 2.7953 | 0.005 | 98 | 10 | 6307 | 3.12 | 0.059 | |
PELS 189 | 211065162 | 54.12626 | 24.01222 | 12.26 | 0.567 | 7.575758 | 0.035 | 118 | 6 | 5011 | 1.95 | 0.083 | |
PELS 019 | 211095259 | 55.12802 | 24.4873 | 11.72 | 0.524 | 6.849315 | 0.022 | 49 | 5 | 5168 | 1.62 | 0.079 | |
DH 156 | 211039307 | 55.21359 | 23.59843 | 12.79 | 0.65 | 8.333334 | 0.085 | ≤15 | – | 4708 | 0.50 | 0.092 |
Notes. (a) The Pleiades were one of the regions covered by the 2MASS “6×” deeper integrations. The 2MASS measurements were harvested first from the main 2MASS catalog, and then from the deeper integration 6× catalog, allowing the 6× catalog to take precedence over the main 2MASS catalog. In most cases, this is advantageous, because the 6× data have higher signal-to-noise ratios; in a few cases (e.g., HII 335), the 6× data were significantly inferior to the original 2MASS catalog in that their J–Ks colors were inconsistent with their colors from other bands or their H-Ks colors. In such cases, we gave precedence to the 2MASS catalog. Only the first five lines of Table B.1 are presented here. The full table is available electronically at CDS Strasbourg.
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