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Table 2

Spectroscopic results for the newly discovered variable sdBs presented in Table A.1 (asterisk-marked entries).

TIC Teff(K) Literature Teff log g(cm s−2) Literature log g log (nHe/nH) Distance (pc) Ref.
Pulsating sdBs
27782233 20 670 ± 100 21 420 ± 129 5.27 ± 0.02 5.26 ± 0.02 −2.24 ± 0.07 423-6+5$423_{-6}^{+5}$ This work, 1
28522887 20 620 ± 160 5.16 ± 0.05 −2.12 ± 0.12 773-12+17$773_{-12}^{+17}$ This work 1
207111243 29 410 ± 140 5.35 ± 0.02 −1.86 ± 0.04 3996+6$399_{-6}^{+6}$ This work
48085434 25 370 ± 110 5.33 ± 0.06 −2.62 ± 0.07 1358-37+43$1358_{-37}^{+43}$ This work
154432267 21 160 ± 260 5.35 ± 0.07 −3.38 ± 0.04 525-5+6$525_{-5}^{+6}$ This work
258021652 24 690 ± 440 5.14 ± 0.07 −2.94 ± 0.06 1215-58+62$1215_{-58}^{+62}$ This work
341157482 20 540 ± 160 5.10 ± 0.02 −1.63 ± 0.04 1076-33+45$1076_{-33}^{+45}$ This work
348825375 25 550 ± 980 5.27 ± 0.18 −2.89 ± 0.15 710-9+11$710_{-9}^{+11}$ This work
387884969 23 440 ± 840 5.30 ± 0.09 −2.92 ± 0.03 585-10+12$585_{-10}^{+12}$ This work
310930161 24 900 ± 980 5.09 ± 0.09 −2.73 ± 0.04 739-12+14$739_{-12}^{+14}$ This work
Low relative-likelihood pulsator/binary candidates
326559609 25 260 ± 110 5.38 ± 0.13 −1.57 ± 0.02 880-26+32$880_{-26}^{+32}$ This work
Stars whose atmospheric parameters were collected from literature. Pulsating sdBs
33770579 25 300 ± 500 5.55 ± 0.06 2760-270+252$2760_{-270}^{+252}$ 2
77477081 40 300 ± 80 6.08 ± 0.04 1507-73+73$1507_{-73}^{+73}$ 3
161358962 36 980 ± 90 5.59 ± 0.04 715-14+15$715_{-14}^{+15}$ 3
194807290 24 809 ± 298 5.27 ± 0.03 764-19+19$764_{-19}^{+19}$ 1
273084007 27 135 ± 204 5.26 ± 0.03 1035-34+39$1035_{-34}^{+39}$ 1
373731788 23 988 ±− 5.00 ±− 710-9+11$710_{-9}^{+11}$ 4*
Binary candidates
239930769 22 640 ± 550 5.71 ± 0.07 1247-68+80$1247_{-68}^{+80}$ 5
368827573 29 658 ± 509 5.53 ± 0.08 1205-42+47$1205_{-42}^{+47}$ 1
Low relative-likelihood pulsator/binary candidates
457094678 26 933 ± 355 5.27 ± 0.04 1077-38+42$1077_{-38}^{+42}$ 1
184607974 28 744 ± 303 5.47 ± 0.04 936-36+30$936_{-36}^{+30}$ 1

Notes. For 11 sdBs (top part of the table), the atmospheric parameters were derived from our own observations (see Table 1). When atmospheric parameters are also available in literature, they are shown in the columns marked ‘literature’ and referenced in the ‘Ref.’ column. If multiple parameters are available in literature for the same object, the most recently published values of Teff and log g are shown. Distances are given in the ‘Distance’ column. The bottom part of the table lists the remaining 10 objects from Table A.1, for which atmospheric parameters were found in literature. 1 – Luo et al. (2021); 2 – Moni Bidin et al. (2017); 3 – Jeffery et al. (2021); 4* – Kilkenny et al. (1988), errors are not listed in their catalogue; 5 – Lei et al. (2019).

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