VizieR Online Data Catalog: I-band LC of the microlensing event KMT-2016-BLG-1836 (Yang+, 2020)

The Korea Microlensing Telescope Network (KMTNet) continuously monitors a broad area at relatively high-cadence toward the Galactic bulge from three 1.6m telescopes equipped with 4°² field-of-view (FOV) cameras at the Cerro Tololo Inter-American Observatory (CTIO) in Chile (KMTC), the South African Astronomical Observatory (SAAO) in South Africa (KMTS), and the Siding Spring Observatory (SSO) in Australia (KMTA).

The super-Jovian planet KMT-2016-BLG-1836b was found by applying the KMTNet event-finding algorithm (Kim+ 2018AJ....155...76K) to the 2016 KMTNet survey data (Kim+ 2018, arXiv:1804.03352), and the apparently amplified flux of a KMTNet catalog star I=19.20+/-0.13 derived from the OGLE-III star catalog (Szymanski+ 2011, II/323) led to the detection of this microlensing event.

KMT-2016-BLG-1836 was located in two slightly offset fields, BLG02 and BLG42, with a nominal combined cadence of Γ~4/hr. The majority of observations were taken in the I band, with about 10% of the KMTC images and 5% of the KMTS images taken in the V band for the color measurement of microlens sources.

(1 data file).