Table 1
Spectroscopic atmospheric parameters for confirmed magnetic He-sdOs (upper), new magnetic stars (centre), and He-sdOs showing the 4630 Å feature (lower).
Star | Teff(K) | log ɡ (cm s−1) | log n(He)/n(H) | Bav (kG) | υrad (km s−1) | S/N | ||
---|---|---|---|---|---|---|---|---|
J0415+2528(*) | 46 580 ± 1500 | 5.98 ± 0.25 | −0.10 ± 0.15 | 305 ± 20 | −17 ± 10 | – | ||
J0809–2627(†) | 44900 ± 1000 | 5.93 ± 0.15 | 0.28 ± 0.10 | 353 ± 10 | 33 ± 2 | – | ||
J1303+2646(*) | 47 950 ± 1500 | 5.97 ± 0.30 | 0.25 ± 0.15 | 450 ± 20 | −37 ± 8 | – | ||
J1603+3412(*) | 46450 ± 1500 | 6.06 ± 0.20 | 0.07 ± 0.15 | 335 ± 15 | 6 ± 5 | – | ||
J1233–6749 | 47 680 ± 1000 | 5.60 ± 0.13 | 0.11 ± 0.05 | 222 ± 10 | 82 ± 15 | 110 | ||
J1256–5753 | 46980 ± 1000 | 5.75 ± 0.16 | 0.00 ± 0.05 | 216 ± 24 | 5 ± 12 | 110 | ||
J1444–6744 | 45 990 ± 1000 | 5.55 ± 0.15 | 0.17 ± 0.06 | 184±14 | 1 ± 10 | 90 | ||
EC20577–5504 | 46610 ± 1000 | 6.09 ± 0.12 | 0.19 ± 0.05 | ≤ 59 ± 3 | −42 ± 10 | 180 | ||
EC22332–6837 | 46990 ± 1000 | 5.93 ± 0.12 | 0.28 ± 0.06 | ≤ 82 ± 5 | −101±10 | 100 | ||
PG1625–034 | 46 570 ± 1100 | 5.67 ± 0.16 | 0.49 ± 0.09 | ≤128 ± 9 | −84± 11 | 40 | ||
J0714–2245 | 44400 ± 1000 | 5.61 ± 0.13 | −0.26 ± 0.05 | ≤107± 4 | 33 ± 10 | 70 | ||
J1346–4025 | 45 070 ± 1000 | 5.83 ± 0.12 | 0.13 ± 0.05 | ≤ 68 ± 4 | −17±10 | 130 | ||
J1946–4756 | 46730 ± 1100 | 5.84 ± 0.16 | 0.12 ± 0.08 | ≤129± 9 | −41 ± 11 | 40 |
Notes.(*) From Pelisoli et al. (2022).(†) From Dorsch et al. (2022). J0714–2245 ≡ Gaia DR3 2927944940172059648, J1346-4025 ≡ UCAC4 248-062759, and J1946–4756 ≡ GALEX J194618.8–475617. The last column lists the mean signal-to-noise ratio (S/N) of the RSS spectra. For J1233–6749, J1256–5753, and J1444–6744, the four available spectra were co-added to obtain average magnetic field strengths, while Teff, log ɡ, and log n(He)/n(H) were derived from the individual spectra. Estimated systematical uncertainties are stated for one sigma confidence.
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