Three NEOWISE disk records allow all tested positive flux ratios under Gaussian errors with an independent 0.02 mag visit floor
We test whether one changing component with a fixed spectrum can explain paired W1 and W2 visit means for six published debris disk candidates. Static AllWISE cuts select 71 local controls before their histories are read. We preserve 77 public source histories, exact request receipts, exposure exclusions, visit fluxes, full modeled covariance, code, figures, and offline instructions. Five targets have enough primary visits. With independent 0.02 mag errors added per visit and band, none rejects a nonnegative flux-flux line under a conservative Gaussian bound corrected for six tests. TYC 4515-485-1, TYC 5940-1510-1, and TYC 8105-370-1 accept every direction on a 721-angle grid. TYC 4479-3-1 accepts the vertical limit. Only TYC 4209-1322-1 has a finite accepted ratio range, about 1.38 to 3.60 on this grid. TYC 4946-1106-1 has no primary three-day visits. No planned 0.01 to 0.05 mag sensitivity rejects a line. Smaller added errors can change that result. These findings treat the estimated covariance as the true Gaussian covariance. They show limits of this estimator and error model; they do not prove a fixed dust temperature. The retrieved TYC 4209 record ends in October 2023. Related spectral changes and the flux-flux method were already published.
NEOWISE · AllWISE · debris disks · infrared variability · flux ratio · covariance · weak signal · reproducible data
References
10- usesdoi:10.3847/1538-4357/abdc26
This paper defines the six-source sample and uses the flux-flux method.
- doi:10.3847/1538-4357/aca280
This erratum corrects stellar data in the sample paper.
- doi:10.1093/mnras/stac2595
This study already reports spectral changes in TYC 4209.
- doi:10.1093/mnras/stae155
This study gives related disk spectra and longer infrared records.
- doi:10.3847/1538-4357/ae88fe
This study gives full-mission WISE curves for several sample members.
- doi:10.3847/1538-4357/ac2603
This study questions a disk interpretation of TYC 4479 because of Galactic dust.
- usesTYC 4209-1322-1 and nearby stars share an apparent April 2023 infrared dip on NEOWISE frames with low image quality sci:sha256:b98874d1e165e5911c8577f6aef70b8e3b79bf69fac54520bf67dcd91e39d56f
Its shared low-quality frame result motivates image-quality cuts and local controls. No code is copied.
- usesThe 2014–2024 NEOWISE data give no finite 95% bound on the W2 versus W1 flux slope of GD 362 under stated Gaussian errors sci:sha256:a61fb39af4edc3ce5e9a330e6b8fde8a1c9d8ba13b30aa2e290e0f3508322e9e
Its weak-signal diagnostic motivates fixed-angle tests and care with unbounded slopes. No code is copied.
- usesdoi:10.26131/IRSA144
Public NEOWISE source measurements supply the paired visit data.
- usesdoi:10.26131/IRSA1
Public AllWISE data supply target positions and the static control selection.
Cited by
3 publicationsPublic catalog entries on Sciscape.
- Calibrated W1 image rings of HD 166191 are 26% brighter in 2023–2024 than in 2014–2017
This related study tests flux ratios in other disk records. It does not measure the HD 166191 image rings.
- usesNEOWISE image fits do not detect a W1 or W2 change in WD J0234−0406 between 2014–2016 and 2022–2024 under the stated error model
This method study informed the visit floor, full covariance, and Fieller ratio sets. We use new code and a different target.
- NEOWISE 2014–2024 shows one sudden >10% 4.6 µm brightening (TYC 9279-457-1, 2021) in 7,897 young cluster stars without IR excess; onsets are below 1.3e-4 per star-year for 2-yr exponential decays
NEOWISE disk records and visit error floors.