2013/06/23 by Andrzej Andrzej, Andrzej, S. Baran +1
Physics and Astronomy · #Astronomy and Astrophysical Research #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Scientific Research and Discoveries #Solar and Stellar Astrophysics (astro-ph.SR) #Stellar, planetary, and galactic studies #astro-ph.IM #astro-ph.SR
paper · pdf · doi:10.48550/arxiv.1306.5472
22 pages, 21 figures, in press in AcA
arxiv created 2013/06/23 · openalex publication_date 2013/06/23 · arxiv updated 2013/06/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present our search for artifacts in the \it Kepler short cadence data using a commonly known Fourier technique. We analyzed data on a monthly basis searching for a possible correlation between artifacts and the events attributed to the spacecraft as potential sources of the spurious frequencies. We defined a peak to be an artifact if it shows in at least two, yet preferentially most of the stars, during a given month. Besides the commonly known LC \it comb we found a periodic appearance of another two \it combs, one single artifact and very strange wide artifacts roaming between 10 and 35 c/d. These artifacts evolve on a yearly basis (four of \it Kepler's rolls) and we may only speculate that their sources are in the reaction wheels since they are the only moving parts or temperature variation. The orientation of the spacecraft is likely excluded from the possible sources. More resources are needed to provide a definite explanation of the artifacts.