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Table 1

Observational and instrument details.

Observatory Telescope aperture Duration Detector (filter) Ref.
Modra 0.6 m Jun.–Jul. 2006 AP8p (clear) This work
(21 nights)
SMO 0.35 m May–Jun. 2006 SBIG ST-10XME (clear) This work
(12 nights)
WISE 0.4 m Jun. 2010 Teledyne HgCdTe (W1 and W2) Wright et al. (2010)
(1 night) DRS Si:As (W3 and W4) Mainzer et al. (2011)
KMTNet 1.6 m Jan.–Apr. 2016 18K mosaic CCD (R) Lee et al. (2017)
(CTIO, SAAO, and SSO) (51 nights) with four e2v 9K
TUG 1.0 m Jul.–Aug. 2017 SI 4K (R) This work
(4 nights)
LOAO 1.0 m Jun.–Sep. 2017 e2v 4K (R) This work
(4 nights)
BOAO 1.8 m Jun.–Sep. 2017 e2v 4K (R) This work
(6 nights)
OAdM 0.8 m Jun.–Aug. 2017 e2v 2K (R) This work
(7 nights)
La Sagra 0.45 m Jun. 2017 SBIG ST-10XME (R) This work
(3 nights)
McDonald 2.1 m Jul. 2017 SQUEAN (r) This work
(6 nights)
BlueEye 600 0.6 m Jul. 2017 G4-4000BI (R) This work
(2 nights)

Notes. SMO = Sugarloaf Mountain Observatory, WISE = Wide-field Infrared Survey Explorer, KMTNet = Korea Microlensing Telescope Network, CTIO = Cerro Tololo Inter-American Observatory, SAAO = South African Astronomical Observatory, SSO = Siding Spring Observatory, TUG = TÜBİTAK National Observatory, LOAO = Lemmonsan Optical Astronomy Observatory, BOAO = Bohyunsan Optical Astronomy Observatory, OAdM = Montsec Astronomical Observatory.

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