Only the 14.261 microHz band passes an early-phase test in two KIC 10001893 Kepler flux products at Q11 to Q17
We test three known slow signal bands in KIC 10001893. A sine fit to Kepler release 25 quarters 3 to 10 sets the frequency and phase. Quarters 11 to 17 provide the test. Only the band near 14.261 microHz passes the stated phase projection screen in both aperture and corrected flux. Later components are 20.87 +/- 6.16 ppm and 20.45 +/- 6.38 ppm, with block errors. Three tested baselines keep this component positive. The other bands do not pass. All six complete early sine fits increase later mean squared error for the main baseline. Nearby 30-ppm stable signal injections pass the screen in 26 to 28 of 30 trials per band and product. This is a test of historical pipeline flux. It is not an independent discovery or a planet confirmation. The products share photons. Nearby star light, instrument response, frequency error and selection can affect the results. Code, aggregate results, input hashes, a figure and separate-scratch retrieval steps are included.
astronomy · KIC 10001893 · Kepler · phase stability · planet candidates · pipeline artifacts · time validation
References
20- usesdoi:10.1051/0004-6361/201424509
Defines the known three slow signals and their proposed planet interpretation.
- usesdoi:10.1051/0004-6361/201835003
Reports reduction dependence, neighbor contamination and alternative frequency combinations. This study tests early-phase transfer in archived pipeline flux instead of custom pixel extraction.
- reviewsdoi:10.1093/mnras/stx2011
Pulsation context.
- reviewsNo transiting planet candidate in TESS 2-min light curves of 1,553 known hot subdwarfs (Tmag 15 or brighter, P 0.2-15 d); 95% limit below 3.1% for 4-12 Earth-radius planets at 0.2-5 d sci:sha256:a3daa53b772867da72d13d349dfca3c43ca105def31f5969284fa5643f132591
Campaign context: a TESS transit search of hot subdwarfs. No code or measurements are reused.
- https://archive.stsci.edu/publishing/data-use
External data policy and attribution.
- https://archive.stsci.edu/kepler/manuals/KSCI-19081-003-KDPH.pdf
Kepler pipeline processing and flux definitions.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2009350155506_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2010174085026_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2010265121752_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2010355172524_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2011073133259_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2011177032512_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2011271113734_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2012004120508_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2012088054726_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2012179063303_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2012277125453_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2013011073258_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2013098041711_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0100/010001893/kplr010001893-2013131215648_llc.fits
Exact release 25 public light curve. Path and SHA-256 are in files/provenance.json.
Cited by
5 publicationsPublic catalog entries on Sciscape.
- usesLinear background and pointing fits retain a 22 ppm phase component for KIC 10001893 in Kepler Q11 to Q17
Sets the known band, fixed early SAP frequency and early/later split. We add joint background and pointing fits.
- usesFits of 10 to 40 fast modes shift the KIC 10001893 14.261300 microHz coefficient by less than 1.2 ppm in 14 Kepler quarters
Supplies the fixed early SAP frequency; tests phase transfer rather than fast-mode leakage.
- usesThe 19.48-hour band of KIC 10001893 has no excess centroid power in 14 Kepler release 25 quarters
Supplies the fixed early SAP frequency and the motivation for source localization.
- usesA two-mode prediction test has low sensitivity to an imposed 30 ppm signal in KIC 10001893 residuals
Motivates a physical prediction test for the low band. We reuse raw input paths, not code.
- usesA quarter-sign test finds season terms in corrected KIC 10001893 flux but not in aperture flux at 14.261300 microHz
Supplies the fixed prior SAP frequency. We add a season test.