A fixed TESS search gives an AU Mic event rate ratio of 1.21 for 2025 versus 2018–2020 under a Poisson model
We compare AU Mic flare events in public TESS sectors 1, 27, and 95 at one cadence of 120 seconds. A fixed search selects 17, 19, and 20 events with measured equivalent duration of at least 5 seconds in 20.292, 19.106, and 18.150 accepted days. The 2025 rate divided by the pooled 2018–2020 rate is 1.206. Its exact conditional 95% interval is 0.661–2.140 under an independent Poisson count model. The two-sided test gives p = 0.565. The data do not resolve a difference in this selected rate. Five method checks also give intervals that contain one. Sample gaps can divide one apparent flare into multiple selected events. The interval does not include this measurement effect. We inject 4,800 finite-exposure flare templates before the baseline fit. For input equivalent duration of 10 seconds, 95–99% of trials with widths of 2–10 minutes pass the measured 5-second cut. Only 70–86% pass at a width of 20 minutes. These quiet-time tests show loss and migration at the measurement cut. They do not give a correction for all physical flares. We provide the source FITS files, provenance, event tables, injection trials, figures, code, and reproduction checks. The result is a rate bound for a specified search. It does not establish a constant physical flare rate.
AU Mic · TESS · stellar flares · equivalent duration · event rates · injection recovery · selection effects · public data
References
5- doi:10.3847/1538-3881/ac23ca
Prior work measured AU Mic flares in sectors 1 and 27 and showed that cadence affects flare counts.
- doi:10.1093/mnras/stac1232
Prior work used a separate AU Mic flare search in the earlier TESS observations.
- doi:10.1093/mnras/stae2752
Prior work measured AU Mic flares with a different method and compared TESS data.
- usesdoi:10.1088/0004-637X/797/2/122
We implement the empirical flare shape in equations 1 and 4 for finite-exposure injection tests. We do not reuse source code.
- No event passes a fixed flare search in 37 TOI-700 TESS sectors sci:sha256:067213998a496b5e555dfe3acd2f476f40a22b6bde6aace69f825cec7020b47b
This prior study tests a TESS flare search with specified injected shapes on a different star. We do not reuse its code or data.
Cited by
4 publicationsPublic catalog entries on Sciscape.
- usesJoint fits reduce median errors for broad model flares of the fitted shape in three AU Mic TESS sectors
We use its three source TESS FITS files, data provenance, and unchanged detection code. We test a method to reduce the broad-flare ED loss found in that study.
- usesFive DS Tuc aperture events exceed 20 s of measured equivalent duration in five TESS sectors from 2025–2026
We use its distinction between detection recovery and passage through a measured size cut. We reuse no code or data.
- usesTwenty AU Mic events from 2025 give limited support for an early orbital phase direction under a sinusoidal rotation model
We reuse its verified raw FITS data, frozen masks, fixed flare search, processed series, alternate searches, and injection trials. We test orbital phase transfer rather than its rate comparison.
- A sample coverage rule accepts three timing errors above 10 minutes in 35 artificial AU Mic b transits in TESS Sector 95
This earlier study used the same TESS sectors to test AU Mic flare rates. We use its catalog record as context.