Table 2
Final sample of lowest-activity targets in the B–V range 0.53–0.73 from the RAVE survey.
| RAVE name | Teff (K) | log g (dex) | [Fe/H] (dex) | (B–V)0 (mag) | ℱIRT–1 | ℱIRT–2 | ℱIRT–3 | log RIRT (σTeff) | L (L⊙) | R (R⊙) | Other name |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (106 ergs cm−2 s−1) | |||||||||||
| J091344.0-185715 | 6078 | 4.07 | −0.06 | 0.53 | 2.3369 | 1.5231 | 1.5991 | −4.15 | 8.2 | 2.6 | TYC 6036-1085-1 |
| J210322.6-374731 | 6115 | 4.02 | +0.11 | 0.54 | 2.2724 | 1.5224 | 1.6340 | −4.16 | 5.5 | 2.1 | CPD-38 8173(a) |
| J210118.8-604737 | 6027 | 4.19 | −0.11 | 0.54 | 2.2114 | 1.5028 | 1.5405 | −4.15 | 4.1 | 1.9 | CPD-61 6520 |
| J200531.9-522958 | 6243 | 4.62 | +0.42 | 0.55 | 2.1681 | 1.3992 | 1.5136 | −4.23 | 2.6 | 1.4 | TYC 8404-7-1 (b) |
| J193243.7-551333 | 5971 | 4.17 | −0.15 | 0.55 | 2.1644 | 1.4197 | 1.5814 | −4.14 | 5.5 | 2.2 | TIC 320005130 |
| J014458.2-472433 | 5837 | 4.02 | −0.52 | 0.56 | 2.1365 | 1.4453 | 1.5049 | −4.11 | 3.3 | 1.8 | TYC 8040-22-1 |
| J024718.6-811225 | 5936 | 4.09 | −0.14 | 0.56 | 2.0863 | 1.3579 | 1.5066 | −4.15 | 6.7 | 2.5 | TYC 9374-1033-1 |
| J212620.6-031522 | 6010 | 4.05 | +0.08 | 0.56 | 2.1221 | 1.4442 | 1.5375 | −4.16 | 7.4 | 2.5 | TYC 5199-577-1 |
| J225620.6-473754 | 5680 | 4.09 | −0.68 | 0.59 | 1.9878 | 1.3423 | 1.3637 | −4.10 | 43 | 6.8 | CPD-48 10837 |
| J134102.1-214222 | 5816 | 4.15 | −0.20 | 0.59 | 1.9479 | 1.2159 | 1.4459 | −4.15 | 8.0 | 2.8 | CPD-21 5592(a,b) |
| J191213.1-760732 | 5786 | 4.72 | −0.11 | 0.62 | 1.9303 | 1.3100 | 1.2598 | −4.15 | 1.16 | 1.07 | TIC 352227373 |
| J055244.5-404031 | 5812 | 4.33 | +0.50 | 0.67 | 1.6271 | 1.0293 | 1.1135 | −4.23 | 2.3 | 1.5 | TYC 7602-148-1 (b) |
| J025410.6-383603 | 5509 | 4.18 | +0.10 | 0.72 | 1.6822 | 1.0943 | 1.0672 | −4.13 | 0.98 | 1.1 | TYC 7560-477-1 (b) |
Notes. (a)Double- or Multiple star. (b)Also in the sample of fake candidates in Table C.4. Teff, log g, and [Fe/H] are from RAVE DR6. (B–V)0 was converted from Teff. The next four columns are the resolution- and metallicity-corrected fluxes for each of the IRT lines and the combined radiative loss in logarithmic form, respectively. The luminosity, L, and radius, R, are from the DR3 parallax and the Simbad visual magnitude corrected for interstellar absorption according to Schlafly & Finkbeiner (2011). The distance to CPD-21°5592 was assumed to be 350 pc.
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