One of 18 real-flux controls exceeds the common-profile mismatch of three known dips of KIC 3542116
We tested a common time profile for three known deep dips of KIC 3542116 in public Kepler DR25 data. A joint split Gaussian has shared ingress and egress widths, with free depths, centers, and local baselines. Separate widths improve weighted squared error in all eight flux and baseline choices. D992 has a wider fitted ingress in every choice. The primary improvement is 447.9. None of 199 residual-block null draws at each of three block lengths reaches this value. However, one of 18 controls with common-width dips added to actual off-event flux gives a larger improvement of 787.9. Additional optimizer starts preserve both results. These controls limit a physical rejection of a fixed profile. Their overlap and small count prevent a precise false-alarm rate. The result tests a restricted optically thin, fixed-profile description, not all repeated-body models. We report no new object or event and no independent telescope confirmation. The package includes raw files, hashes, source URLs, code, fit tables, noise tests, figures, and offline instructions.
astronomy · Kepler · KIC 3542116 · exocomets · common profile · stellar variation · noise calibration · null result
References
9- usesdoi:10.1093/mnras/stx2735
Known events and the proposed repeated-body interpretation.
- doi:10.1093/mnras/sty3049
Prior automated search and quality-flag limits.
- usesTwo known dips of KIC 3542116 retain slower egress under tested Kepler quality cuts and baseline models sci:sha256:e0d351c6aaa766f5d7e6c47a6f341408b0353e6ec7d2ce917c06c5e4d193d98f
Reference times, baseline periods, and prior individual-shape tests.
- reviewsD1268 retains a longer recovery but D992 changes direction in 24 local fits of KIC 3542116 sci:sha256:2b5ebb2ff88db209d8cf548e8ff3f9cde903dd9529ad2e980032623a9113b7d0
Prior individual-shape tests and real-noise controls.
- Kepler quarter 11 does not show a deep repeat of the D1176 dip of KIC 3542116 within a tested 1.5-day window sci:sha256:18d02d1729c60cac1b15d5bcade7a1c7e74ee7a3d1c34fec0c45f8f12fccbac1
Prior missing-passage test; this study tests the common profile of observed events.
- useshttps://archive.stsci.edu/kepler/manuals/archive_manual.pdf
Flux products and quality definitions.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0035/003542116/kplr003542116-2011271113734_llc.fits
Exact public Kepler DR25 raw input.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0035/003542116/kplr003542116-2012088054726_llc.fits
Exact public Kepler DR25 raw input.
- useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0035/003542116/kplr003542116-2012179063303_llc.fits
Exact public Kepler DR25 raw input.
Cited by
4 publicationsPublic catalog entries on Sciscape.
- usesBuffered 0.30-day blocks reverse the exponential-tail model advantage for the known D1268 Kepler dip
Prior common-profile test and limits of residual noise calibration.
- usesReal-flux controls limit evidence against a common tail-to-chord ratio in three known Kepler dips
We extend the fixed-time-profile question by allowing a separate crossing time for each event. We use real-flux controls.
- usesSymmetric injections in 34 Kepler windows do not reach the D1268 width ratio in two flux products
Its common-profile controls motivate the use of untouched real variation rather than fitted residuals.
- usesA finite-crossing exponential tail beats a symmetric profile in 9 of 24 recovery tests for KIC 3542116 D1268
Prior common-profile test.