Table A.3.
The 16 objects presented in this work.
SDSS J | Teff (K) | log g(cgs) | Mass (M⊙) | Variability | Reference a |
---|---|---|---|---|---|
001245.60+143956.4 | 10893 ± 68 | 7.74 ± 0.07 | 0.482 ± 0.03 | Pulsations | Kleinman et al. (2013) |
![]() |
7.5 ± 0.4 | - | This work, χred2 = 1.6c | ||
002602.29-103751.9 | 9177 ± 30 | 7.26 ± 0.01 | 0.273 ± 0.004 | NOV | Caron et al. (2023) |
![]() |
7.9 ± 0.4 | - | This work, χred2 = 4.1 | ||
015958.50-180546.8 | ![]() |
6.4 ± 0.4 | - | NOV | This work, χred2 = 127b |
040600.99-542751.7 | ![]() |
7.0 ± 0.2 | - | NOV | This work, χred2 = 122b |
045116.83+010426.6 | ![]() |
4.9 ± 0.5 | - | Ellipsoidal | This work, χred2 = 245d |
083013.72-100356.0 | 7750 ± 190 | 5.2 ± 0.4 | - | NOV | This work, χred2 = 84d |
083417.21-652423.2 | ![]() |
5.4 ± 0.3 | - | Ellipsoidal | This work, χred2 = 354d |
090559.60+084324.9 | 10070.0 ± 38 | 8.18 ± 0.04 | 0.704 ± 0.03 | Pulsations | Kleinman et al. (2013) |
![]() |
8.2 ± 0.4 | - | This work, χred2 = 1.9c | ||
090901.01-454637.0 | ![]() |
7.3 ± 0.2 | - | NOV | This work, χred2 = 18 |
112521.26-023433.4 | 9615 ±149 | 8.08 ±0.2 | 0.644 ±0.1 | NOV | Kleinman et al. (2013) |
![]() |
8.5 ± 0.5 | - | This work, χred2 = 1.5c | ||
134619.11-135026.7 | 9102 ± 39 | 7.02 ± 0.009 | 0.216 ± 0.003 | NOV | Caron et al. (2023) |
![]() |
7.1 ± 0.2 | - | This work, χred2 = 136b | ||
151626.39-265836.9 | ![]() |
7.9 ± 0.4 | - | NOV | This work, χred2 = 1.7c |
161004.27+063330.6 | 9454±85 | 8.02 ±0.1 | 0.61 ±0.07 | NOV | Kleinman et al. (2013) |
8400 ± 840 | 8.5 ± 0.5 | - | This work, χred2 = 2.2c | ||
183245.52+141311.2 | 8860 ± 100 | 5.9 ± 0.1 | - | Reflection effect | This work, χred2 = 1359b |
183702.03-674141.1 | ![]() |
5.2 ± 0.4 | - | NOV | This work, χred2 = 148d |
212935.23+001332.3 | 8860 ± 30 | 7.16 ± 0.006 | 0.244 ± 0.002 | Pulsations | Caron et al. (2023) |
![]() |
6.8 ± 0.2 | - | This work, χred2 = 232b |
Notes: Column 1 provides the SDSS J identifier. The effective temperature, surface gravity, and stellar mass determinations are listed in columns 2, 3, and 4, respectively. Column 5 shows the type of variability seen in each object’s light curve. Column 6 contains the reference for the atmospheric parameters, along with the reduced χ2 for the parameters obtained in this work.
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