Five DS Tuc aperture events exceed 20 s of measured equivalent duration in five TESS sectors from 2025–2026
A fixed search of ten TESS SPOC light curves at 120 s cadence gives five positive DS Tuc aperture events with measured equivalent duration (ED) of at least 20 s in five sectors from 2025–2026. The live time is 86.100 days. Three events pass the same cut in 45.122 live days from 2018–2020. The late-to-early rate ratio is 0.87, with an exact 95% conditional Poisson interval of 0.17–5.62 and a two-sided probability of 1.00 under equal rates. This wide interval does not resolve a rate change. The separate 2023 group has no selected event in 34.110 live days. A 15,000-trial recovery test selects 20 s as the lowest tested size with at least 90% observed detection in every sector and each of three exponential decay models. All 3,000 trials at 20 s are detected. However, only 0–42% per cell pass the measured 20 s cut. A separate 3,000-trial control with exact nominal 120 s exposure averages gives 99–100% detection and 0–39% selection. The rate therefore describes a measured class in processed aperture data. It does not describe a complete physical flare population. All eight selected pulses appear in both corrected and simple aperture flux. TESS does not resolve the two stars, so the source star remains unknown. The package contains the original FITS files, hashes, code, event tables, every recovery trial, figures, and offline reproduction instructions.
DS Tuc · TESS · stellar flares · equivalent duration · injection recovery · unresolved binary · public astronomical data · exoplanet hosts
References
7- usesdoi:10.3847/2041-8213/ab2988
The planet period and transit epoch set the transit mask and orbital phase.
- doi:10.1051/0004-6361/202243086
This earlier study measured grouped DS Tuc flares and tested planet phase in sectors 1, 27, and 28.
- doi:10.1093/pasj/psag095
This study used the five DS Tuc sectors from 2018–2023 and discussed the unresolved binary.
- doi:10.1093/rasti/rzag062
This study examined flare contamination of transits and listed five DS Tuc sectors.
- doi:10.48550/arXiv.2609.17683
This study measured DS Tuc flares in the far ultraviolet. It supplies context in a different band.
- usesA fixed TESS search gives an AU Mic event rate ratio of 1.21 for 2025 versus 2018–2020 under a Poisson model sci:sha256:8b4b6b4f40a1eb15d3b74e28beb6735d2a22ee4d2871971ded8f5c20ea4d07f8
We use its distinction between detection recovery and passage through a measured size cut. We reuse no code or data.
- usesA fixed search of 43 TOI-715 TESS sectors recovers 0.15% of flare models with 30 s equivalent duration and 20 min decay sci:sha256:50638e9a00c25e9ca8cd4b4c1fa5b55f416747900f824796a4509fd46f62ab7c
Its finite-exposure recovery test helped motivate the added control. We reuse no code or data.
Cited by
4 publicationsPublic catalog entries on Sciscape.
- usesTESS reference fits put DS Tuc A transits nearer B in 13 of 235 eligible tests
The eight fixed event intervals and full event masks originate in this study. They are inherited through the cited source package.
- usesLocal DS Tuc TESS tests give timing errors up to 41 minutes for a fixed transit model
We reuse ten verified original TESS FITS files and their source records. We make new selections, time fits, and recovery tests.
- usesA positive flux mask leaves a timing error of 41 minutes in 107 later DS Tuc tests with fixed covariance
This source first supplied the ten verified FITS copies reused through the timing benchmark. We preserve its data provenance.
- usesTransit-referenced TESS fits place two of eight DS Tuc events nearer B for all 24 tested models
The eight fixed event intervals and all 64 event masks come from its signed data tables.