Table 3
Distance estimates of a subset of novae from our catalog.
| Name | Distance | Flux | Reference |
| [kpc] | [10-7 cm-2 s-1] | ||
|
|
|||
| V1309 Sco | 2.5 ± 0.4 | <1.0 | Özdönmez et al. (2016) |
| V1721 Aql | 7.5 ± 2.0 | <3.0 | Özdönmez et al. (2016) |
| V679 Car | 2.9 ± 0.7 | 1.9 ± 0.5 | MMRD, this work |
| V5583 Sgr | 10.5 ± 0.5 | <0.6 | Schwarz et al. (2011) |
| V2672 Oph | 3.12 ± 0.69 | <2.0 | Özdönmez et al. (2016) |
| KT Eri | 6.5 ± 0.5 | <0.3 | Ragan (2009) |
| V496 Sct | 3.2 ± 0.8 | <2.0 | Özdönmez et al. (2016) |
| V1722 Aql | >12 | <1.1 | Munari et al. (2010a) |
| U Sco | 12.0 ± 2.0 | <0.6 | Schaefer (2010a) |
| V2674 Oph | 1.65 ± 0.38 | <1.0 | Özdönmez et al. (2016) |
| V407 Cyg | 3.5 ± 0.3 | 6.6 ± 0.5 | Özdönmez et al. (2016) |
| V1723 Aql | 5.7 ± 0.4 | <2.3 | Weston et al. (2016b) |
| V5588 Sgr | >4 | <1.1 | Munari et al. (2015) |
| T Pyx | 4.8 ± 0.5 | <0.6 | Sokoloski et al. (2013) |
| V5589 Sgr | 3.9 ± 0.7 | <1.3 | Weston et al. (2016a) |
| V1324 Sco | 4.3 ± 0.9 | 5.0 ± 0.5 | Özdönmez et al. (2016) |
| V959 Mon | 2.3 ± 0.6 | 5.2 ± 0.5 | Özdönmez et al. (2016) |
| V809 Cep | >7 | <0.3 | Munari et al. (2014) |
| V339 Del | 4.54 ± 0.59 | 2.1 ± 0.2 | Schaefer et al. (2014) |
| V1830 Aql | >12 | <2.2 | Munari et al. (2014) |
| V1369 Cen | 2.5 ± 0.5 | 2.1 ± 0.3 | Shore (2014) |
| V745 Sco | 7.8 ± 1.8 | <0.5 | Schaefer (2010a) |
| V1535 Sco | 7.3 ± 1.7 | 1.0 ± 0.3 | MMRD, this work |
| V5668 Sgr | 2.0 ± 0.5 | 0.8 ± 0.1 | Banerjee et al. (2016) |
| V5583 Sgr | 10.5 ± 0.5 | <0.6 | Schwarz et al. (2011) |
Notes. A different distance for V1324 Sco of < 6.5 kpc was estimated by Finzell et al. (2015). Weston et al. (2016a) estimated a distance range of 3.2 to 4.6 kpc for V5589 Sgr; for simplicity, we have adopted a distance of 3.9 ± 0.7 kpc for this source. Linford et al. (2015) found a distance of V959 Mon between 0.9 and 2.2 kpc with a most likely distance of 1.4 ± 0.4 kpc using expansion parallax.
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