We complete the analysis of all 2018 prime-field microlensing planets identified by the Korea Microlensing Telescope Network (KMTNet) Anomaly Finder. Among the ten previously unpublished events with clear planetary solutions, eight are either unambiguously planetary or are very likely to be planetary in nature: OGLE-2018-BLG-1126, KMT-2018-BLG-2004, OGLE-2018-BLG-1647, OGLE-2018-BLG-1367, OGLE-2018-BLG-1544, OGLE-2018-BLG-0932, OGLE-2018-BLG-1212, and KMT-2018-BLG-2718. Combined with the four previously published new Anomaly Finder events and 12 previously published (or in preparation) planets that were discovered by eye, this makes a total of 24 2018 prime-field planets discovered or recovered by Anomaly Finder. Together with a paper in preparation on 2018 subprime planets, this work lays the basis for the first statistical analysis of the planet mass-ratio function based on planets identified in KMTNet data. By systematically applying the heuristic analysis to each event, we identified the small modification in their formalism that is needed to unify the so-called close-wide and inner-outer degeneracies.
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Can We Build Useful Models of Future Risk from Natural Hazards?
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Model output from experiments described in Cooper et al 2022.</p> Includes WW3 output of ice concentration and significant wave height (hourly) for 2018-01-01 through 2018-12-31.</p> Includes WW3 1-D wave spectra (hourly) for 2018-07.</p> Includes CICE output of representative radius (daily) for 2018-01-01 through 2018-12-31.</p> Note: uncompressed file size is 2x the tar.gz file size.</p>more » « less
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Model output from experiments described in Cooper et al 2022.</p> Includes WW3 output of ice concentration and significant wave height (hourly) for 2018-01-01 through 2018-12-31.</p> Includes WW3 1-D wave spectra (hourly) for 2018-07.</p> Includes CICE output of representative radius (daily) for 2018-01-01 through 2018-12-31.</p> Note: uncompressed file size is 2x the tar.gz file size.</p>more » « less
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Model output from experiments described in Cooper et al 2022.</p> Includes WW3 output of ice concentration and significant wave height (hourly) for 2018-01-01 through 2018-12-31.</p> Includes WW3 1-D wave spectra (hourly) for 2018-07.</p> Includes CICE output of representative radius (daily) for 2018-01-01 through 2018-12-31.</p> Note: uncompressed file size is 2x the tar.gz file size.</p>more » « less
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Model output from experiments described in Cooper et al 2022.</p> Includes WW3 output of ice concentration and significant wave height (hourly) for 2018-01-01 through 2018-12-31.</p> Includes WW3 1-D wave spectra (hourly) for 2018-07.</p> Includes CICE output of representative radius (daily) for 2018-01-01 through 2018-12-31.</p> Note: uncompressed file size is 2x the tar.gz file size.</p>more » « less
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