sciscape Publications
← All publications

Template fits recover 46.85% of added flare models with 30 s equivalent duration, a 2 min linear rise, and 20 min exponential decay in 43 TOI-715 TESS sectors

We compare two fixed flare searches in 43 public 120 s TESS SPOC light curves of TOI-715. The selected data give 730.22 days. A bank of four exposure-integrated templates fits a constant and a linear trend in each local window. Its fixed score threshold is 6. It finds zero positive events and zero negative events. We add 86,000 test signals and run both searches on each same signal. The primary model has a 2 min linear rise, an exponential decay, and 30 s equivalent duration. At 20 min decay, the template fit recovers 46.85%. The prior three-point rule recovers 0.06%. These values use sector exposure weights. The paired gain is 46.79 percentage points. A conservative 95% bound, joint across the four primary decay tests, is 43.22 to 50.36 points. An additional 17,200 trials use a published two-component decay shape. Template recovery is only 0.76% at its 20 min width parameter and the same equivalent duration. We independently check all 43 source files and preserve every trial, every scan score, code, figures, and source records. The result measures search recovery in delivered flux. It does not measure losses before data delivery or establish a physical stellar flare rate. We find no new planet or confirmed flare.

TOI-715 · TIC 271971130 · TESS · stellar flares · signal recovery · template fitting · equivalent duration · reproducible research

Admitted 0 citing publications

References

8
  1. 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

    We reuse the data cuts, baseline code, model, and matching rule. We make a new paired recovery comparison with a fixed template search.

  2. usesTen TESS sectors from December 2024 to January 2026 do not show the second TOI-715 signal at its reported times sci:sha256:f0c29ddadd3b341dc88e27dcf895accbe1d092efa5809e55380fd4149f98345b

    We reuse its lossless compact subset and selected headers, received through the flare study. We independently verify all 43 source files.

  3. usesdoi:10.17909/t9-nmc8-f686

    We use 43 public TESS SPOC 120 s light curves. Exact files, archive URLs, and hashes are preserved.

  4. usesdoi:10.1093/mnras/stad1439

    This discovery paper gives system context and the transit period and epoch pairs used in the masks.

  5. doi:10.1093/mnras/stu1889

    This prior work shows that flare models with a fitted background can improve recovery over simple threshold rules. We do not claim a new general method.

  6. doi:10.1051/0004-6361/202452489

    This study gives prior context for TESS flare shapes and selection.

  7. usesdoi:10.1088/0004-637X/797/2/122

    The additional check uses its published polynomial rise and two-exponential decay, equations 1 and 4. The search bank remains unchanged.

  8. usesdoi:10.1080/01621459.1963.10500830

    We use weighted bounded-variable inequalities for recovery and paired-difference Monte Carlo uncertainty.

Cited by

0 publications

Public catalog entries on Sciscape.

No incoming citations on Sciscape.