Table 3.
Reddening in the g band (Ag), which have been determined using Pan-STARRS1 data (Green et al. 2018a).
| Source | Porb | Ag | gq | Mg |
|---|---|---|---|---|
| (min) | (mag) | (mag) | (mag) | |
| V407 Vul | 9.5 | 4.9 | 20.16 | 4.0 ± 0.7 |
| ES Cet | 10.4 | 0.1 | 16.66 | 5.6 ± 0.4 |
| SDSS J1351-0643 | 15.7 | 0.1 | 18.66 | 8.0 ± 0.7 |
| AM CVn | 17.1 | 0.07 | 14.26 | 6.81 ± 0.03 |
| SDSS J1908+3940 | 18.1 | 0.53 | 16.16 | 5.5 ± 0.1 |
| HP Lib | 18.4 | 0.49 | 13.60 | 5.91 ± 0.03 |
| PTF1 J1919+4815 | 22.5 | 0.18 | 20.51 | 9.7 ± 0.8 |
| CX361 | 22.9 | 1.16 | 17.48 | 6.4 ± 0.3 |
| ASASSN-14cc | 22.5 | 0.12 | 19.0 | 8.9 ± 0.2 |
| KL Dra | 25.0 | 0.18 | 18.62 | 8.5 ± 0.3 |
| PTF1 J0719+4858 | 26.8 | 0.32 | 19.15 | 9.2 ± 0.7 |
| YZ LMi | 28.3 | 0.07 | 19.23 | 10.4 ± 1.0 |
| CP Eri | 28.4 | 0.35 | 20.07 | 9.8 ± 1.1 |
| SDSS J1043+5632 | 28.5 | 0.07 | 20.35 | 10.33 ± 1.0 |
| CRTS J0910-2008 | 30.2 | 0.32 | 19.39 | 9.9 ± 0.9 |
| CRTS J0105+1903 | 31.6 | 0.18 | 19.65 | 10.1 ± 0.9 |
| V406 Hya | 33.8 | 0.11 | 19.97 | 11.4 ± 1.5 |
| SDSS J1730+5545 | 35.2 | 0.14 | 20.05 | 10.1 ± 0.8 |
| NSV1440 | 36.3 | 0.21m | 18.53 | 10.7 ± 0.1 |
| V558 Vir | 36.6 | 0.14 | 19.99 | 10.7 ± 1.4 |
| SDSS J1240-0159 | 37.4 | 0.07 | 19.55 | 10.7 ± 1.1 |
| V744 And | 37.6 | 0.28 | 19.88 | 11.1 ± 0.8 |
| SDSS J1721+2733 | 38.1 | 0.07 | 20.43 | 10.4 ± 1.0 |
| ASASSN-14mv | 41 | 0.04 | 17.98 | 11.0 ± 0.1 |
| ASASSN-14ei | 43 | 0.21m | 15.54 | 8.94 ± 0.03 |
| SDSS J1525+3600 | 44.3 | 0.07 | 19.86 | 11.2 ± 0.3 |
| SDSS J0804+1616 | 44.5 | 0.18 | 18.60 | 8.8 ± 0.4 |
| SDSS J1411+4812 | 46.0 | 0.07 | 19.44 | 11.2 ± 0.3 |
| GP Com | 46.6 | 0.00 | 15.92 | 11.60 ± 0.01 |
| SDSS J0902+3819 | 48.3 | 0.11 | 20.39 | 12.0 ± 1.4 |
| Gaia14aae | 49.7 | 0.04 | 18.55 | 11.4 ± 0.1 |
| SDSS J1208+3550 | 53.0 | 0.07 | 18.82 | 12.2 ± 0.2 |
| SDSS J1642+1934 | 54.2 | 0.25 | 20.35 | 10.0 ± 1.0 |
| SDSS J1552+3201 | 56.3 | 0.14 | 20.40 | 12.0 ± 0.9 |
| SDSS J1137+4054 | 59.6 | 0.07 | 19.09 | 12.4 ± 0.1 |
| V396 Hya | 65.1 | 0.18 | 17.68 | 12.64 ± 0.03 |
| SDSS J1319+5915 | 65.6 | 0.04 | 19.12 | 12.6 ± 0.1 |
Notes. Those stars where the reddening has been estimated using the dust maps of (Schlafly & Finkbeiner 2011) have a superscript m to indicate it is the reddening to the edge of the Galaxy. The third column shows the quiescent g magnitude as determined from the survey magnitudes outlined in the appendix. In the final column we show the absolute magnitude, Mg. These data are also included in the online table.
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