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The Korea Microlensing Telescope Network (KMTNet) Alert Algorithm and Alert System

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arxiv 1806.07545 v1 pith:KLEU4X7G submitted 2018-06-20 astro-ph.IM

classification astro-ph.IM
keywords algorithmhighalertdeltaeventskmtnetleastlight
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We describe a new microlensing-event alert algorithm that is tailored to the Korea Microlensing Telescope Network (KMTNet) multi-observatory system. The algorithm focuses on detecting "rising" events, i.e., events whose brightness is increasing as a function of time. The algorithm proceeds in three steps. It first identifies light curves with at least $N_{\rm high}$ points that are at least $3\sigma$ above the median and that had been taken since shortly before the previous search for new events. It then demands that there are at least $N_{\rm high}$ $\textit{consecutive}$ high points when considering any combination of light curves from one, two, or three observatories. Finally, it fits to a "rising microlensing model" consisting of a broken line, i.e., flat before some time $t_{\rm rise}$ and rising linearly afterward. If this fit is better than a flat line by $\Delta\chi^2>\Delta\chi^2_{\rm thresh}$, the light curve is sent for human review. Here, $(N_{\rm high},\Delta\chi^2_{\rm thresh})=(5,250)$ or $(10,400)$, depending on the field cadence. For 2018, KMTNet alerts will initially be restricted to a few northern bulge fields and may gradually extend to the full northern bulge. Further expansion of coverage is expected in 2019.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. KMT-2025-BLG-2093: Free-Floating Planet Candidate Near the Shore of the Einstein Desert

    astro-ph.EP 2026-06 unverdicted novelty 5.0 of 10

    KMT-2025-BLG-2093 is identified as the second isolated microlens in the Einstein Desert, a free-floating planet candidate with θ_E = 13.1 ± 2.8 μas.

  2. KMT-2025-BLG-1314 and KMT-2025-BLG-1392: two microlensing planetary/brown-dwarf candidates analyzed with differentiable code

    astro-ph.EP 2026-03 conditional novelty 5.0 of 10

    KMT-2025-BLG-1314 and KMT-2025-BLG-1392 are modeled as binary-lens microlensing events with planet/brown-dwarf candidates, and HMC with the differentiable microlux code is shown to handle bimodal posteriors better than emcee.

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