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Galactic bulge reanalysis and compendium from OGLE: https://aasnova.org/2022/05/20/a-massive-reanalysis-of-microlensing-events/
MOA anomaly events http://iral2.ess.sci.osaka-u.ac.jp/~moa/anomaly/
ATLAS forced photometry server: https://fallingstar-data.com/forcedphot/
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event | link | RA | DEC | t_o, HJD-24500000 | baseline | notes | ATLAS |
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KMT-2022-BLG-0061 | https://kmtnet.kasi.re.kr/ulens/event/2022/view.php?event=KMT-2022-BLG-0061 | 17:38:26.66 | -28:15:44.17 | 9688.13539 | I=16.6 | parallax event? | |
KMT-2022-BLG-1018 | https://kmtnet.kasi.re.kr/ulens/event/2022/view.php?event=KMT-2022-BLG-1018 | 17:49:24.11 | -26:16:31.40 | 9742.62921 | I=19.9 | long event, going on now | |
MOA-2022-BLG-275 | https://www.massey.ac.nz/~iabond/moa/alert2022/display.php?id=gb9-R-3-150516 | 17:57:24.45 | -29:19:50.96 | 9728.10 | I=20.2 | finite source effect | |
MOA-2021-BLG-015 | https://www.massey.ac.nz/~iabond/moa/alert2021/display.php?id=gb3-R-10-38233 | 17:54:40.47 | -32:04:37.96 | 2459281.18 | I=16.5 | finite source effect | |
MOA-2020-BLG-033 | https://www.massey.ac.nz/~iabond/moa/alert2020/display.php?id=gb5-R-10-121819 | 17:55:47.08 | -28:38:17.72 | 2458909.10 | I=26 | very high amplification, A | |
MOA-2020-BLG-031 | https://www.massey.ac.nz/~iabond/moa/alert2020/display.php?id=gb10-R-4-47615 | 17:58:21.80 | -27:53:10.34 | 2458920.11 | I=16.3, amp=6 | ||
MOA-2019-BLG-141 | https://www.massey.ac.nz/~iabond/moa/alert2019/display.php?id=gb1-R-4-37369 | designated anomaly event- short binary event |
KMT-2022-BLG-0061, difference request
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ATLAS started operation mid-2015, so it's appropriate to compile a list of events from calendar 2015 to 2022. That spans both OGLE (until 2020) and MOA, not sure about KMT.
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1) construct aggregated event list that spans years when ATLAS observed Galactic plane. DONE- had to clean up changes in data format between years, for KMT alert files, and delete a few incomplete records. KMTevents.txt has around 15,000 candidate bulge events.
2) for each event, do a query on forced photometry difference photometry for duration spanning 10 event duration times on either side of event center.
3) construct database of event photometry.
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