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.
BHXB . | Instrument . | Date . | On source . | 1σ WCS . | Photometric . | Limiting . | Filter . | Average . |
---|---|---|---|---|---|---|---|---|
candidate . | . | observed . | time . | uncertaintya . | zero-pointb . | magnitudec . | . | seeing . |
. | . | . | (s) . | (mas) . | (mag) . | . | . | (arcsec) . |
Swift J1539.2−6227 | GROND | 2017 Sep 15 | 372 | 130 ± 20 | 25.61 ± 0.06 | <19.6 | g′ | 2.2 |
372 | 60 ± 20 | 26.34 ± 0.03 | <20.1 | r′ | 1.9 | |||
372 | 50 ± 15 | 25.41 ± 0.06 | <19.8 | i′ | 1.8 | |||
372 | 80 ± 15 | 25.18 ± 0.03 | <18.9 | z′ | 1.8 | |||
480 | 125 ± 15 | 24.32 ± 0.05 | <18.9 | J | 1.8 | |||
480 | 340 ± 15 | 23.85 ± 0.07 | <16.8 | H | 1.9 | |||
480 | 50 ± 15 | 24.57 ± 0.05 | <17.6 | Ks | 1.8 | |||
MAXI J1543−564 | HAWK-I | 2018 Apr 10 | 480 | 170 ± 15 | 27.56 ± 0.17 | <23.2 | H | 0.5 |
420 | 270 ± 15 | 27.31 ± 0.16 | <23.2 | Ks | 0.5 | |||
XTE J1650−500 | GROND | 2017 Sep 14 | 372 | 100 ± 20 | 25.61 ± 0.06 | <20.3 | g′ | 2.0 |
372 | 100 ± 20 | 26.34 ± 0.03 | <20.5 | r′ | 2.0 | |||
372 | 60 ± 15 | 25.41 ± 0.06 | <19.4 | i′ | 1.9 | |||
372 | 120 ± 15 | 25.18 ± 0.03 | <18.5 | z′ | 1.8 | |||
480 | 50 ± 15 | 24.32 ± 0.05 | <18.4 | J | 1.9 | |||
480 | 60 ± 15 | 23.85 ± 0.07 | <16.8 | H | 2.0 | |||
480 | 40 ± 15 | 24.57 ± 0.05 | <17.8 | Ks | 1.9 | |||
XTE J1726−476 | PANIC | 2006 Aug 3 | 900 | 100 ± 15 | 25.03 ± 0.24 | < 20.7 | J | 0.7 |
375 | 200 ± 15 | 25.38 ± 0.26 | <17.9 | Ks | 0.6 | |||
IGR J17451−3022 | LIRIS | 2015 Apr 9* | 360 | 110 ± 15 | 24.29 ± 0.09 | <17.5 | Ks | 0.7 |
2016 Mar 28 | 450 | 80 ± 15 | 24.41 ± 0.08 | <17.7 | Ks | 0.8 | ||
Swift J174510.8−262411 | LIRIS | 2017 Apr 13 | 1600 | 100 ± 15 | 24.80 ± 0.05 | <19.0 | Ks | 0.9 |
XTE J1752−223 | LIRIS | 2017 Apr 13 | 1600 | 40 ± 15 | 24.04 ± 0.07 | <19.6 | Ks | 1.0 |
MAXI J1807+132 | ACAM | 2017 Jul 11 | 1800 | 120 ± 20 | 25.88 ± 0.05 | <24.4 | i′ | 1.3 |
XTE J1818−245 | PANIC | 2005 Sep 12* | 450 | 80 ± 15 | 25.39 ± 0.01 | <19.3 | Ks | 0.5 |
2006 May 8 | 375 | 110 ± 15 | 25.62 ± 0.01 | <17.6 | Ks | 0.6 | ||
MAXI J1828−249 | MOSFIRE | 2017 Jun 15 | 419 | 160 ± 15 | 27.41 ± 0.08 | <21.9 | Ks | 1.1 |
MAXI J1836−194 | MOSFIRE | 2017 Jun 15 | 436 | 60 ± 15 | 27.51 ± 0.29 | <22.2 | Ks | 1.1 |
XTE J1856+053 | MOSFIRE | 2017 Jun 15 | 436 | 50 ± 15 | 28.69 ± 0.25 | <20.7 | Ks | 1.1 |
Swift J1910.2−0546 | ACAM | 2015 Jul 19 | 600 | 110 ± 15 | 26.25 ± 0.01 | <22.4 | i′ | 1.1 |
600 | 150 ± 15 | 26.24 ± 0.01 | <22.5 | i′ | 1.2 | |||
600 | 100 ± 15 | 26.39 ± 0.12 | <23.6 | r′ | 1.3 | |||
LIRIS | 2017 Apr 13 | 800 | 20 ± 15 | 24.68 ± 0.10 | <22.1 | Ks | 0.8 | |
MAXI J1957+032 | MOSFIRE | 2017 Jun 15 | 291 | 80 ± 15 | 27.63 ± 0.13 | <23.3 | Ks | 0.9 |
XTE J2012+381 | LIRIS | 2017 Apr 13 | 2000 | 80 ± 15 | 24.67 ± 0.22 | <21.5 | Ks | 0.8 |
BHXB . | Instrument . | Date . | On source . | 1σ WCS . | Photometric . | Limiting . | Filter . | Average . |
---|---|---|---|---|---|---|---|---|
candidate . | . | observed . | time . | uncertaintya . | zero-pointb . | magnitudec . | . | seeing . |
. | . | . | (s) . | (mas) . | (mag) . | . | . | (arcsec) . |
Swift J1539.2−6227 | GROND | 2017 Sep 15 | 372 | 130 ± 20 | 25.61 ± 0.06 | <19.6 | g′ | 2.2 |
372 | 60 ± 20 | 26.34 ± 0.03 | <20.1 | r′ | 1.9 | |||
372 | 50 ± 15 | 25.41 ± 0.06 | <19.8 | i′ | 1.8 | |||
372 | 80 ± 15 | 25.18 ± 0.03 | <18.9 | z′ | 1.8 | |||
480 | 125 ± 15 | 24.32 ± 0.05 | <18.9 | J | 1.8 | |||
480 | 340 ± 15 | 23.85 ± 0.07 | <16.8 | H | 1.9 | |||
480 | 50 ± 15 | 24.57 ± 0.05 | <17.6 | Ks | 1.8 | |||
MAXI J1543−564 | HAWK-I | 2018 Apr 10 | 480 | 170 ± 15 | 27.56 ± 0.17 | <23.2 | H | 0.5 |
420 | 270 ± 15 | 27.31 ± 0.16 | <23.2 | Ks | 0.5 | |||
XTE J1650−500 | GROND | 2017 Sep 14 | 372 | 100 ± 20 | 25.61 ± 0.06 | <20.3 | g′ | 2.0 |
372 | 100 ± 20 | 26.34 ± 0.03 | <20.5 | r′ | 2.0 | |||
372 | 60 ± 15 | 25.41 ± 0.06 | <19.4 | i′ | 1.9 | |||
372 | 120 ± 15 | 25.18 ± 0.03 | <18.5 | z′ | 1.8 | |||
480 | 50 ± 15 | 24.32 ± 0.05 | <18.4 | J | 1.9 | |||
480 | 60 ± 15 | 23.85 ± 0.07 | <16.8 | H | 2.0 | |||
480 | 40 ± 15 | 24.57 ± 0.05 | <17.8 | Ks | 1.9 | |||
XTE J1726−476 | PANIC | 2006 Aug 3 | 900 | 100 ± 15 | 25.03 ± 0.24 | < 20.7 | J | 0.7 |
375 | 200 ± 15 | 25.38 ± 0.26 | <17.9 | Ks | 0.6 | |||
IGR J17451−3022 | LIRIS | 2015 Apr 9* | 360 | 110 ± 15 | 24.29 ± 0.09 | <17.5 | Ks | 0.7 |
2016 Mar 28 | 450 | 80 ± 15 | 24.41 ± 0.08 | <17.7 | Ks | 0.8 | ||
Swift J174510.8−262411 | LIRIS | 2017 Apr 13 | 1600 | 100 ± 15 | 24.80 ± 0.05 | <19.0 | Ks | 0.9 |
XTE J1752−223 | LIRIS | 2017 Apr 13 | 1600 | 40 ± 15 | 24.04 ± 0.07 | <19.6 | Ks | 1.0 |
MAXI J1807+132 | ACAM | 2017 Jul 11 | 1800 | 120 ± 20 | 25.88 ± 0.05 | <24.4 | i′ | 1.3 |
XTE J1818−245 | PANIC | 2005 Sep 12* | 450 | 80 ± 15 | 25.39 ± 0.01 | <19.3 | Ks | 0.5 |
2006 May 8 | 375 | 110 ± 15 | 25.62 ± 0.01 | <17.6 | Ks | 0.6 | ||
MAXI J1828−249 | MOSFIRE | 2017 Jun 15 | 419 | 160 ± 15 | 27.41 ± 0.08 | <21.9 | Ks | 1.1 |
MAXI J1836−194 | MOSFIRE | 2017 Jun 15 | 436 | 60 ± 15 | 27.51 ± 0.29 | <22.2 | Ks | 1.1 |
XTE J1856+053 | MOSFIRE | 2017 Jun 15 | 436 | 50 ± 15 | 28.69 ± 0.25 | <20.7 | Ks | 1.1 |
Swift J1910.2−0546 | ACAM | 2015 Jul 19 | 600 | 110 ± 15 | 26.25 ± 0.01 | <22.4 | i′ | 1.1 |
600 | 150 ± 15 | 26.24 ± 0.01 | <22.5 | i′ | 1.2 | |||
600 | 100 ± 15 | 26.39 ± 0.12 | <23.6 | r′ | 1.3 | |||
LIRIS | 2017 Apr 13 | 800 | 20 ± 15 | 24.68 ± 0.10 | <22.1 | Ks | 0.8 | |
MAXI J1957+032 | MOSFIRE | 2017 Jun 15 | 291 | 80 ± 15 | 27.63 ± 0.13 | <23.3 | Ks | 0.9 |
XTE J2012+381 | LIRIS | 2017 Apr 13 | 2000 | 80 ± 15 | 24.67 ± 0.22 | <21.5 | Ks | 0.8 |
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.
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.
BHXB . | Instrument . | Date . | On source . | 1σ WCS . | Photometric . | Limiting . | Filter . | Average . |
---|---|---|---|---|---|---|---|---|
candidate . | . | observed . | time . | uncertaintya . | zero-pointb . | magnitudec . | . | seeing . |
. | . | . | (s) . | (mas) . | (mag) . | . | . | (arcsec) . |
Swift J1539.2−6227 | GROND | 2017 Sep 15 | 372 | 130 ± 20 | 25.61 ± 0.06 | <19.6 | g′ | 2.2 |
372 | 60 ± 20 | 26.34 ± 0.03 | <20.1 | r′ | 1.9 | |||
372 | 50 ± 15 | 25.41 ± 0.06 | <19.8 | i′ | 1.8 | |||
372 | 80 ± 15 | 25.18 ± 0.03 | <18.9 | z′ | 1.8 | |||
480 | 125 ± 15 | 24.32 ± 0.05 | <18.9 | J | 1.8 | |||
480 | 340 ± 15 | 23.85 ± 0.07 | <16.8 | H | 1.9 | |||
480 | 50 ± 15 | 24.57 ± 0.05 | <17.6 | Ks | 1.8 | |||
MAXI J1543−564 | HAWK-I | 2018 Apr 10 | 480 | 170 ± 15 | 27.56 ± 0.17 | <23.2 | H | 0.5 |
420 | 270 ± 15 | 27.31 ± 0.16 | <23.2 | Ks | 0.5 | |||
XTE J1650−500 | GROND | 2017 Sep 14 | 372 | 100 ± 20 | 25.61 ± 0.06 | <20.3 | g′ | 2.0 |
372 | 100 ± 20 | 26.34 ± 0.03 | <20.5 | r′ | 2.0 | |||
372 | 60 ± 15 | 25.41 ± 0.06 | <19.4 | i′ | 1.9 | |||
372 | 120 ± 15 | 25.18 ± 0.03 | <18.5 | z′ | 1.8 | |||
480 | 50 ± 15 | 24.32 ± 0.05 | <18.4 | J | 1.9 | |||
480 | 60 ± 15 | 23.85 ± 0.07 | <16.8 | H | 2.0 | |||
480 | 40 ± 15 | 24.57 ± 0.05 | <17.8 | Ks | 1.9 | |||
XTE J1726−476 | PANIC | 2006 Aug 3 | 900 | 100 ± 15 | 25.03 ± 0.24 | < 20.7 | J | 0.7 |
375 | 200 ± 15 | 25.38 ± 0.26 | <17.9 | Ks | 0.6 | |||
IGR J17451−3022 | LIRIS | 2015 Apr 9* | 360 | 110 ± 15 | 24.29 ± 0.09 | <17.5 | Ks | 0.7 |
2016 Mar 28 | 450 | 80 ± 15 | 24.41 ± 0.08 | <17.7 | Ks | 0.8 | ||
Swift J174510.8−262411 | LIRIS | 2017 Apr 13 | 1600 | 100 ± 15 | 24.80 ± 0.05 | <19.0 | Ks | 0.9 |
XTE J1752−223 | LIRIS | 2017 Apr 13 | 1600 | 40 ± 15 | 24.04 ± 0.07 | <19.6 | Ks | 1.0 |
MAXI J1807+132 | ACAM | 2017 Jul 11 | 1800 | 120 ± 20 | 25.88 ± 0.05 | <24.4 | i′ | 1.3 |
XTE J1818−245 | PANIC | 2005 Sep 12* | 450 | 80 ± 15 | 25.39 ± 0.01 | <19.3 | Ks | 0.5 |
2006 May 8 | 375 | 110 ± 15 | 25.62 ± 0.01 | <17.6 | Ks | 0.6 | ||
MAXI J1828−249 | MOSFIRE | 2017 Jun 15 | 419 | 160 ± 15 | 27.41 ± 0.08 | <21.9 | Ks | 1.1 |
MAXI J1836−194 | MOSFIRE | 2017 Jun 15 | 436 | 60 ± 15 | 27.51 ± 0.29 | <22.2 | Ks | 1.1 |
XTE J1856+053 | MOSFIRE | 2017 Jun 15 | 436 | 50 ± 15 | 28.69 ± 0.25 | <20.7 | Ks | 1.1 |
Swift J1910.2−0546 | ACAM | 2015 Jul 19 | 600 | 110 ± 15 | 26.25 ± 0.01 | <22.4 | i′ | 1.1 |
600 | 150 ± 15 | 26.24 ± 0.01 | <22.5 | i′ | 1.2 | |||
600 | 100 ± 15 | 26.39 ± 0.12 | <23.6 | r′ | 1.3 | |||
LIRIS | 2017 Apr 13 | 800 | 20 ± 15 | 24.68 ± 0.10 | <22.1 | Ks | 0.8 | |
MAXI J1957+032 | MOSFIRE | 2017 Jun 15 | 291 | 80 ± 15 | 27.63 ± 0.13 | <23.3 | Ks | 0.9 |
XTE J2012+381 | LIRIS | 2017 Apr 13 | 2000 | 80 ± 15 | 24.67 ± 0.22 | <21.5 | Ks | 0.8 |
BHXB . | Instrument . | Date . | On source . | 1σ WCS . | Photometric . | Limiting . | Filter . | Average . |
---|---|---|---|---|---|---|---|---|
candidate . | . | observed . | time . | uncertaintya . | zero-pointb . | magnitudec . | . | seeing . |
. | . | . | (s) . | (mas) . | (mag) . | . | . | (arcsec) . |
Swift J1539.2−6227 | GROND | 2017 Sep 15 | 372 | 130 ± 20 | 25.61 ± 0.06 | <19.6 | g′ | 2.2 |
372 | 60 ± 20 | 26.34 ± 0.03 | <20.1 | r′ | 1.9 | |||
372 | 50 ± 15 | 25.41 ± 0.06 | <19.8 | i′ | 1.8 | |||
372 | 80 ± 15 | 25.18 ± 0.03 | <18.9 | z′ | 1.8 | |||
480 | 125 ± 15 | 24.32 ± 0.05 | <18.9 | J | 1.8 | |||
480 | 340 ± 15 | 23.85 ± 0.07 | <16.8 | H | 1.9 | |||
480 | 50 ± 15 | 24.57 ± 0.05 | <17.6 | Ks | 1.8 | |||
MAXI J1543−564 | HAWK-I | 2018 Apr 10 | 480 | 170 ± 15 | 27.56 ± 0.17 | <23.2 | H | 0.5 |
420 | 270 ± 15 | 27.31 ± 0.16 | <23.2 | Ks | 0.5 | |||
XTE J1650−500 | GROND | 2017 Sep 14 | 372 | 100 ± 20 | 25.61 ± 0.06 | <20.3 | g′ | 2.0 |
372 | 100 ± 20 | 26.34 ± 0.03 | <20.5 | r′ | 2.0 | |||
372 | 60 ± 15 | 25.41 ± 0.06 | <19.4 | i′ | 1.9 | |||
372 | 120 ± 15 | 25.18 ± 0.03 | <18.5 | z′ | 1.8 | |||
480 | 50 ± 15 | 24.32 ± 0.05 | <18.4 | J | 1.9 | |||
480 | 60 ± 15 | 23.85 ± 0.07 | <16.8 | H | 2.0 | |||
480 | 40 ± 15 | 24.57 ± 0.05 | <17.8 | Ks | 1.9 | |||
XTE J1726−476 | PANIC | 2006 Aug 3 | 900 | 100 ± 15 | 25.03 ± 0.24 | < 20.7 | J | 0.7 |
375 | 200 ± 15 | 25.38 ± 0.26 | <17.9 | Ks | 0.6 | |||
IGR J17451−3022 | LIRIS | 2015 Apr 9* | 360 | 110 ± 15 | 24.29 ± 0.09 | <17.5 | Ks | 0.7 |
2016 Mar 28 | 450 | 80 ± 15 | 24.41 ± 0.08 | <17.7 | Ks | 0.8 | ||
Swift J174510.8−262411 | LIRIS | 2017 Apr 13 | 1600 | 100 ± 15 | 24.80 ± 0.05 | <19.0 | Ks | 0.9 |
XTE J1752−223 | LIRIS | 2017 Apr 13 | 1600 | 40 ± 15 | 24.04 ± 0.07 | <19.6 | Ks | 1.0 |
MAXI J1807+132 | ACAM | 2017 Jul 11 | 1800 | 120 ± 20 | 25.88 ± 0.05 | <24.4 | i′ | 1.3 |
XTE J1818−245 | PANIC | 2005 Sep 12* | 450 | 80 ± 15 | 25.39 ± 0.01 | <19.3 | Ks | 0.5 |
2006 May 8 | 375 | 110 ± 15 | 25.62 ± 0.01 | <17.6 | Ks | 0.6 | ||
MAXI J1828−249 | MOSFIRE | 2017 Jun 15 | 419 | 160 ± 15 | 27.41 ± 0.08 | <21.9 | Ks | 1.1 |
MAXI J1836−194 | MOSFIRE | 2017 Jun 15 | 436 | 60 ± 15 | 27.51 ± 0.29 | <22.2 | Ks | 1.1 |
XTE J1856+053 | MOSFIRE | 2017 Jun 15 | 436 | 50 ± 15 | 28.69 ± 0.25 | <20.7 | Ks | 1.1 |
Swift J1910.2−0546 | ACAM | 2015 Jul 19 | 600 | 110 ± 15 | 26.25 ± 0.01 | <22.4 | i′ | 1.1 |
600 | 150 ± 15 | 26.24 ± 0.01 | <22.5 | i′ | 1.2 | |||
600 | 100 ± 15 | 26.39 ± 0.12 | <23.6 | r′ | 1.3 | |||
LIRIS | 2017 Apr 13 | 800 | 20 ± 15 | 24.68 ± 0.10 | <22.1 | Ks | 0.8 | |
MAXI J1957+032 | MOSFIRE | 2017 Jun 15 | 291 | 80 ± 15 | 27.63 ± 0.13 | <23.3 | Ks | 0.9 |
XTE J2012+381 | LIRIS | 2017 Apr 13 | 2000 | 80 ± 15 | 24.67 ± 0.22 | <21.5 | Ks | 0.8 |
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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