Table A.2.
Quiescent epochs and magnitudes
| Source | Outburst | Quiescence | Quiescent | References |
|---|---|---|---|---|
| (Year) | (MJD) | Mags | for Mags | |
| V404 Cyg | 1989 | 48814-57190 | V = 18.42±0.02, R = 16.52±0.01 | (1) |
| 2015 | 57405- | V = 18.2±0.3 | (2) | |
| BW Cir | 1987 | ∼47200-50754 | R∼20.2, I∼19.2 | (3) |
| 1997 | ∼51135-57000 | R∼20-21, i’ = 19.7-20.8 | (3), (4) | |
| GX 339-4 a | 2014-5 | 57579-57990 | V≃20, R≃19, i≃18.7 | (5) |
| XTE J1550-564 | 2001 | 52020-52719 | V≃22 | (6) |
| 2003 | 52764- | V≃21.9 | (7) | |
| MAXI J1820+070 | 2018 | 60106- | g’ = 19.31±0.02, r’ = 18.58±0.01, i’ = 18.22±0.01 | (8) |
| N. Oph 77 | 1977 | 48719- | V = 21.5±0.1 | (9) |
| N. Mus 91 | 1991 | 48736- | V = 20.66±0.03, R = 19.75±0.27, I = 19.00±0.22 | (10) |
| MAXI J1305-704 | 2012 | 56771- | r’ = 21.69±0.17 | (11) |
| GS 2000+25 | 1988 | 47763- | R = 21.21±0.15 | (12) |
| A 0620-00 | 1975 | 43053- | V = 18.25, R = 17.00 | (13) |
| XTE J1650-500 b | 2001 | ∼52490- | V∼24, R∼22 | (14) |
| N. Vel 93 | 1993 | 49846- | R = 20.6±0.1 | (15) |
| N. Oph 93 | 2016 | 58208- | i’ = 21.39±0.15 | (16) |
| XTE J1859+226 | 1999 | 51781-59250 | V = 23.39±0.09, R = 22.48±0.07 | (17) |
| KY TrA c | 1990 | 48290- | V = 23.6±0.1, R = 22.3±0.1, I = 21.47±0.09 | (18) |
| GRO J0422+32 | 1992 | 49600- | R = 20.94±0.11 | (19) |
| XTE J1118+480 | 2000 | 52311-53375 | R = 18.93±0.01 | (20) |
| 2005 | 53447- | R∼19 | (21) | |
| Swift J1753.5-0127 | 2005 | 57907-60216 | V = 22.17±0.25, I’ = 21.00±0.14 | (22) |
| Swift J1357.2-0933 | 2011 | 56042-57845 | g’ = 22.26±0.38, r’ = 21.54±0.35, i’ = 21.21±0.36; I∼20-21 | (23), (24) |
| MAXI J1659-152 | 2010 | 56087- | r’ = 24.20±0.08, I = 23.3±0.1 | (25) |
References. (1) Casares et al. (1993); (2) Casares et al. (2022); (3) Casares et al. (2009); (4) Koljonen et al. (2016); (5) Russell et al. (2017); (6) Orosz et al. (2002); (7) Orosz et al. (2011); (8) Baglio et al. (2023); (9) Remillard et al. (1996); (10) King et al. (1996);(11) Mata Sánchez et al. (2021); (12) Callanan & Charles (1991); (13) Ciatti & Vittone (1977); (14) Garcia & Wilkes (2002); (15) Shahbaz et al. (1996); (16) Saikia et al. (2022); (17) Zurita et al. (2002b); (18) Zurita et al. (2015); (19) Garcia et al. (1996); (20) Zurita et al. (2002c); (21) Zurita et al. (2006); (22) Zhang et al. (2017); (23) Shahbaz et al. (2013); (24) Russell et al. (2018); (25) Corral-Santana et al. (2018).
Notes. (a) It shows outbursts every ∼2.5 years. The following outburst took place in 2017. (b) The quiescent R-band magnitude quoted by Garcia & Wilkes (2002) is consistent with our own PSF analysis of a DECaPS image taken on 29 April 2017, which yields r’ = 22.10±0.12, cThe optical counterpart of KY TrA was lost after the V> 21 upper limit reported by Murdin et al. (1977) during the decay of the 1974 discovery outburst. The quiescent counterpart was only recovered by Zurita et al. (2015) 17 years after a new mini-outburst was serendipitously discovered in 1990.
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