No tested tail fit reaches a 500 ppm loss in covered Beta Pictoris archive flux from TESS sectors 87, 95, and 98
We searched public TESS light curves of Beta Pictoris for deep, isolated dimming events. We tested nine dust-tail shapes in sectors 87, 95, and 98. We kept samples with no quality flags, removed 50 high-frequency sinusoids per long data block, and made 30-minute bins. The three sectors contain 81.87 days of accepted two-minute samples. The eligible onset measure is 45.75 to 63.04 days, depending on shape. No eligible fit reaches a loss of 500 parts per million (ppm) in either simple aperture flux or corrected flux. The known sector 6 event is recovered near BTJD 1486.35 at about 2069 ppm in corrected flux. For 1000 ppm signals added before our pulsation removal, recovery is 808/810 (99.8%) in simple aperture flux and 810/810 (100.0%) in corrected flux. These tests use the released archive flux. Official notes list an aperture warning for the target in sector 95. The tests do not measure losses in image extraction or archive correction. Deep points near data gaps remain outside some search windows. The result is a measured null for this search rule. It does not establish a limit on all comets or a change in their rate. The package has source files, hashes, code, search tables, recovery tests, and figures.
Beta Pictoris · TESS · exocomets · light curves · null result · injection recovery · public data
References
8- usesdoi:10.17909/T9-NMC8-F686
We use the public TESS two-minute light-curve products from MAST.
- usesdoi:10.1051/0004-6361/201935552
The known deep event in sector 6 is the positive control.
- doi:10.1051/0004-6361/202142111
- usesdoi:10.1038/s41598-022-09021-2
We use its analytic dust-tail family and its comparison-star choice. Our mode removal and search rule differ.
- doi:10.1093/mnras/staf1298
- doi:10.48550/arXiv.2602.02701
- doi:10.1007/s11214-026-01300-y
- supportsA fixed shape fit gives 2714 ppm in QLP raw flux and -65 ppm in QLP spline flux for the Sector 15 dip of TIC 229790952 sci:sha256:61a96a012f90abcc1b3739dfaf5d8001362daf37d3926a224563f109008aabbe
Its test of a different star shows why flux products and nearby data must be checked. We wrote new code for Beta Pictoris.
Cited by
4 publicationsPublic catalog entries on Sciscape.
- TESS fits show a 75.5% fall in the Beta Pictoris F8/F11 amplitude ratio from 2020–2021 to 2025–2026
The source study obtained four original files from this earlier package. We retain that source record.
- A fit with two fixed F8 frequencies through 2024 misses Beta Pictoris sector 98 by 689 ppm
This publication is the earlier source for four files in the preserved data chain.
- usesA fixed 500 ppm search finds 4 early dimming clusters and none later in nine TESS light curves of Beta Pictoris
We reuse the detector, source files, and four sets of mode frequencies. We reproduce the shared flux arrays. We extend the early sample and test common coverage and recovery.
- usesThe 8.51-hour cycle in TESS sector 66 pixels of HD 172555 is strongest near CD-64 1208
Method guidance for coverage, opposite-sign, and conditional-injection controls. New code and a different target are used; no code or data from that package enter this calculation.