Table 2.

Observing log of the BHXB candidates discussed in this paper. All of the sources are observed in quiescence. An (*) marks sources also observed in outburst.

BHXBInstrumentDateOn source1σ WCSPhotometricLimitingFilterAverage
candidateobservedtimeuncertaintyazero-pointbmagnitudecseeing
(s)(mas)(mag)(arcsec)
Swift J1539.2−6227GROND2017 Sep 15372130 ± 2025.61 ± 0.06<19.6g2.2
37260 ± 2026.34 ± 0.03<20.1r1.9
37250 ± 1525.41 ± 0.06<19.8i1.8
37280 ± 1525.18 ± 0.03<18.9z1.8
480125 ± 1524.32 ± 0.05<18.9J1.8
480340 ± 1523.85 ± 0.07<16.8H1.9
48050 ± 1524.57 ± 0.05<17.6Ks1.8
MAXI J1543−564HAWK-I2018 Apr 10480170 ± 1527.56 ± 0.17<23.2H0.5
420270 ± 1527.31 ± 0.16<23.2Ks0.5
XTE J1650−500GROND2017 Sep 14372100 ± 2025.61 ± 0.06<20.3g2.0
372100 ± 2026.34 ± 0.03<20.5r2.0
37260 ± 1525.41 ± 0.06<19.4i1.9
372120 ± 1525.18 ± 0.03<18.5z1.8
48050 ± 1524.32 ± 0.05<18.4J1.9
48060 ± 1523.85 ± 0.07<16.8H2.0
48040 ± 1524.57 ± 0.05<17.8Ks1.9
XTE J1726−476PANIC2006 Aug 3900100 ± 1525.03 ± 0.24< 20.7J0.7
375200 ± 1525.38 ± 0.26<17.9Ks0.6
IGR J17451−3022LIRIS2015 Apr 9*360110 ± 1524.29 ± 0.09<17.5Ks0.7
2016 Mar 2845080 ± 1524.41 ± 0.08<17.7Ks0.8
Swift J174510.8−262411LIRIS2017 Apr 131600100 ± 1524.80 ± 0.05<19.0Ks0.9
XTE J1752−223LIRIS2017 Apr 13160040 ± 1524.04 ± 0.07<19.6Ks1.0
MAXI J1807+132ACAM2017 Jul 111800120 ± 2025.88 ± 0.05<24.4i1.3
XTE J1818−245PANIC2005 Sep 12*45080 ± 1525.39 ± 0.01<19.3Ks0.5
2006 May 8375110 ± 1525.62 ± 0.01<17.6Ks0.6
MAXI J1828−249MOSFIRE2017 Jun 15419160 ± 1527.41 ± 0.08<21.9Ks1.1
MAXI J1836−194MOSFIRE2017 Jun 1543660 ± 1527.51 ± 0.29<22.2Ks1.1
XTE J1856+053MOSFIRE2017 Jun 1543650 ± 1528.69 ± 0.25<20.7Ks1.1
Swift J1910.2−0546ACAM2015 Jul 19600110 ± 1526.25 ± 0.01<22.4i1.1
600150 ± 1526.24 ± 0.01<22.5i1.2
600100 ± 1526.39 ± 0.12<23.6r1.3
LIRIS2017 Apr 1380020 ± 1524.68 ± 0.10<22.1Ks0.8
MAXI J1957+032MOSFIRE2017 Jun 1529180 ± 1527.63 ± 0.13<23.3Ks0.9
XTE J2012+381LIRIS2017 Apr 13200080 ± 1524.67 ± 0.22<21.5Ks0.8
BHXBInstrumentDateOn source1σ WCSPhotometricLimitingFilterAverage
candidateobservedtimeuncertaintyazero-pointbmagnitudecseeing
(s)(mas)(mag)(arcsec)
Swift J1539.2−6227GROND2017 Sep 15372130 ± 2025.61 ± 0.06<19.6g2.2
37260 ± 2026.34 ± 0.03<20.1r1.9
37250 ± 1525.41 ± 0.06<19.8i1.8
37280 ± 1525.18 ± 0.03<18.9z1.8
480125 ± 1524.32 ± 0.05<18.9J1.8
480340 ± 1523.85 ± 0.07<16.8H1.9
48050 ± 1524.57 ± 0.05<17.6Ks1.8
MAXI J1543−564HAWK-I2018 Apr 10480170 ± 1527.56 ± 0.17<23.2H0.5
420270 ± 1527.31 ± 0.16<23.2Ks0.5
XTE J1650−500GROND2017 Sep 14372100 ± 2025.61 ± 0.06<20.3g2.0
372100 ± 2026.34 ± 0.03<20.5r2.0
37260 ± 1525.41 ± 0.06<19.4i1.9
372120 ± 1525.18 ± 0.03<18.5z1.8
48050 ± 1524.32 ± 0.05<18.4J1.9
48060 ± 1523.85 ± 0.07<16.8H2.0
48040 ± 1524.57 ± 0.05<17.8Ks1.9
XTE J1726−476PANIC2006 Aug 3900100 ± 1525.03 ± 0.24< 20.7J0.7
375200 ± 1525.38 ± 0.26<17.9Ks0.6
IGR J17451−3022LIRIS2015 Apr 9*360110 ± 1524.29 ± 0.09<17.5Ks0.7
2016 Mar 2845080 ± 1524.41 ± 0.08<17.7Ks0.8
Swift J174510.8−262411LIRIS2017 Apr 131600100 ± 1524.80 ± 0.05<19.0Ks0.9
XTE J1752−223LIRIS2017 Apr 13160040 ± 1524.04 ± 0.07<19.6Ks1.0
MAXI J1807+132ACAM2017 Jul 111800120 ± 2025.88 ± 0.05<24.4i1.3
XTE J1818−245PANIC2005 Sep 12*45080 ± 1525.39 ± 0.01<19.3Ks0.5
2006 May 8375110 ± 1525.62 ± 0.01<17.6Ks0.6
MAXI J1828−249MOSFIRE2017 Jun 15419160 ± 1527.41 ± 0.08<21.9Ks1.1
MAXI J1836−194MOSFIRE2017 Jun 1543660 ± 1527.51 ± 0.29<22.2Ks1.1
XTE J1856+053MOSFIRE2017 Jun 1543650 ± 1528.69 ± 0.25<20.7Ks1.1
Swift J1910.2−0546ACAM2015 Jul 19600110 ± 1526.25 ± 0.01<22.4i1.1
600150 ± 1526.24 ± 0.01<22.5i1.2
600100 ± 1526.39 ± 0.12<23.6r1.3
LIRIS2017 Apr 1380020 ± 1524.68 ± 0.10<22.1Ks0.8
MAXI J1957+032MOSFIRE2017 Jun 1529180 ± 1527.63 ± 0.13<23.3Ks0.9
XTE J2012+381LIRIS2017 Apr 13200080 ± 1524.67 ± 0.22<21.5Ks0.8

Note. *Observation in outburst. aUncertainty with respect to the reference catalog. The first value is a statistical uncertainty, given by the starlink gaia tool, while the second value is a systematic uncertainty, and corresponds to the astrometric accuracy of the reference catalog (20 mas for UCAC4 and 15 mas for 2MASS). bPhotometric zero-point derived from the data with respect to the 2MASS catalogue, or VVV when possible, (for all the NIR sources), and the Pan-STARRS 1 catalogue (for the optical sources). cLimiting magnitude close to the position of the BHXB.

Table 2.

Observing log of the BHXB candidates discussed in this paper. All of the sources are observed in quiescence. An (*) marks sources also observed in outburst.

BHXBInstrumentDateOn source1σ WCSPhotometricLimitingFilterAverage
candidateobservedtimeuncertaintyazero-pointbmagnitudecseeing
(s)(mas)(mag)(arcsec)
Swift J1539.2−6227GROND2017 Sep 15372130 ± 2025.61 ± 0.06<19.6g2.2
37260 ± 2026.34 ± 0.03<20.1r1.9
37250 ± 1525.41 ± 0.06<19.8i1.8
37280 ± 1525.18 ± 0.03<18.9z1.8
480125 ± 1524.32 ± 0.05<18.9J1.8
480340 ± 1523.85 ± 0.07<16.8H1.9
48050 ± 1524.57 ± 0.05<17.6Ks1.8
MAXI J1543−564HAWK-I2018 Apr 10480170 ± 1527.56 ± 0.17<23.2H0.5
420270 ± 1527.31 ± 0.16<23.2Ks0.5
XTE J1650−500GROND2017 Sep 14372100 ± 2025.61 ± 0.06<20.3g2.0
372100 ± 2026.34 ± 0.03<20.5r2.0
37260 ± 1525.41 ± 0.06<19.4i1.9
372120 ± 1525.18 ± 0.03<18.5z1.8
48050 ± 1524.32 ± 0.05<18.4J1.9
48060 ± 1523.85 ± 0.07<16.8H2.0
48040 ± 1524.57 ± 0.05<17.8Ks1.9
XTE J1726−476PANIC2006 Aug 3900100 ± 1525.03 ± 0.24< 20.7J0.7
375200 ± 1525.38 ± 0.26<17.9Ks0.6
IGR J17451−3022LIRIS2015 Apr 9*360110 ± 1524.29 ± 0.09<17.5Ks0.7
2016 Mar 2845080 ± 1524.41 ± 0.08<17.7Ks0.8
Swift J174510.8−262411LIRIS2017 Apr 131600100 ± 1524.80 ± 0.05<19.0Ks0.9
XTE J1752−223LIRIS2017 Apr 13160040 ± 1524.04 ± 0.07<19.6Ks1.0
MAXI J1807+132ACAM2017 Jul 111800120 ± 2025.88 ± 0.05<24.4i1.3
XTE J1818−245PANIC2005 Sep 12*45080 ± 1525.39 ± 0.01<19.3Ks0.5
2006 May 8375110 ± 1525.62 ± 0.01<17.6Ks0.6
MAXI J1828−249MOSFIRE2017 Jun 15419160 ± 1527.41 ± 0.08<21.9Ks1.1
MAXI J1836−194MOSFIRE2017 Jun 1543660 ± 1527.51 ± 0.29<22.2Ks1.1
XTE J1856+053MOSFIRE2017 Jun 1543650 ± 1528.69 ± 0.25<20.7Ks1.1
Swift J1910.2−0546ACAM2015 Jul 19600110 ± 1526.25 ± 0.01<22.4i1.1
600150 ± 1526.24 ± 0.01<22.5i1.2
600100 ± 1526.39 ± 0.12<23.6r1.3
LIRIS2017 Apr 1380020 ± 1524.68 ± 0.10<22.1Ks0.8
MAXI J1957+032MOSFIRE2017 Jun 1529180 ± 1527.63 ± 0.13<23.3Ks0.9
XTE J2012+381LIRIS2017 Apr 13200080 ± 1524.67 ± 0.22<21.5Ks0.8
BHXBInstrumentDateOn source1σ WCSPhotometricLimitingFilterAverage
candidateobservedtimeuncertaintyazero-pointbmagnitudecseeing
(s)(mas)(mag)(arcsec)
Swift J1539.2−6227GROND2017 Sep 15372130 ± 2025.61 ± 0.06<19.6g2.2
37260 ± 2026.34 ± 0.03<20.1r1.9
37250 ± 1525.41 ± 0.06<19.8i1.8
37280 ± 1525.18 ± 0.03<18.9z1.8
480125 ± 1524.32 ± 0.05<18.9J1.8
480340 ± 1523.85 ± 0.07<16.8H1.9
48050 ± 1524.57 ± 0.05<17.6Ks1.8
MAXI J1543−564HAWK-I2018 Apr 10480170 ± 1527.56 ± 0.17<23.2H0.5
420270 ± 1527.31 ± 0.16<23.2Ks0.5
XTE J1650−500GROND2017 Sep 14372100 ± 2025.61 ± 0.06<20.3g2.0
372100 ± 2026.34 ± 0.03<20.5r2.0
37260 ± 1525.41 ± 0.06<19.4i1.9
372120 ± 1525.18 ± 0.03<18.5z1.8
48050 ± 1524.32 ± 0.05<18.4J1.9
48060 ± 1523.85 ± 0.07<16.8H2.0
48040 ± 1524.57 ± 0.05<17.8Ks1.9
XTE J1726−476PANIC2006 Aug 3900100 ± 1525.03 ± 0.24< 20.7J0.7
375200 ± 1525.38 ± 0.26<17.9Ks0.6
IGR J17451−3022LIRIS2015 Apr 9*360110 ± 1524.29 ± 0.09<17.5Ks0.7
2016 Mar 2845080 ± 1524.41 ± 0.08<17.7Ks0.8
Swift J174510.8−262411LIRIS2017 Apr 131600100 ± 1524.80 ± 0.05<19.0Ks0.9
XTE J1752−223LIRIS2017 Apr 13160040 ± 1524.04 ± 0.07<19.6Ks1.0
MAXI J1807+132ACAM2017 Jul 111800120 ± 2025.88 ± 0.05<24.4i1.3
XTE J1818−245PANIC2005 Sep 12*45080 ± 1525.39 ± 0.01<19.3Ks0.5
2006 May 8375110 ± 1525.62 ± 0.01<17.6Ks0.6
MAXI J1828−249MOSFIRE2017 Jun 15419160 ± 1527.41 ± 0.08<21.9Ks1.1
MAXI J1836−194MOSFIRE2017 Jun 1543660 ± 1527.51 ± 0.29<22.2Ks1.1
XTE J1856+053MOSFIRE2017 Jun 1543650 ± 1528.69 ± 0.25<20.7Ks1.1
Swift J1910.2−0546ACAM2015 Jul 19600110 ± 1526.25 ± 0.01<22.4i1.1
600150 ± 1526.24 ± 0.01<22.5i1.2
600100 ± 1526.39 ± 0.12<23.6r1.3
LIRIS2017 Apr 1380020 ± 1524.68 ± 0.10<22.1Ks0.8
MAXI J1957+032MOSFIRE2017 Jun 1529180 ± 1527.63 ± 0.13<23.3Ks0.9
XTE J2012+381LIRIS2017 Apr 13200080 ± 1524.67 ± 0.22<21.5Ks0.8

Note. *Observation in outburst. aUncertainty with respect to the reference catalog. The first value is a statistical uncertainty, given by the starlink gaia tool, while the second value is a systematic uncertainty, and corresponds to the astrometric accuracy of the reference catalog (20 mas for UCAC4 and 15 mas for 2MASS). bPhotometric zero-point derived from the data with respect to the 2MASS catalogue, or VVV when possible, (for all the NIR sources), and the Pan-STARRS 1 catalogue (for the optical sources). cLimiting magnitude close to the position of the BHXB.

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