FluxCT V2.0: Updates to a Web Tool Identifying Contaminating Flux in Space Telescope Data
arXiv:2504.02326 · doi:10.3847/2515-5172/ad8fa7
Abstract
We present FluxCT V2.0, an updated web tool for identifying contaminating flux in Kepler and TESS target pixel files. FluxCT V2.0 focuses on enhancing functionality, user experience, and data processing capabilities. We resolved existing issues to allow for an extended user base, removed known bugs, and extended the tool to any TESS pixel file, allowing the user to search any TESS point object. A batch code for TESS is now available on the companion GitHub. Additional output parameters, such as amplitude dilution and a magnitude cut, have been added to the tool, allowing users more freedom to analyze the possible effects of target sources.
Published to Research Notes of the American Astronomical Society in November 2024. Code available at this GitHub: https://github.com/Jesstella/FluxCT
References in corpus (6)
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- The Transiting Exoplanet Survey Satellite
- astroquery: An Astronomical Web-Querying Package in Python
- Stellar flares from blended and neighbouring stars in Kepler short cadence observations
- Probability of Physical Association of 104 Blended Companions to \textit{Kepler} Objects of Interest Using Visible and Near-Infrared Adaptive Optics Photometry
- FluxCT: A Web Tool for Identifying Contaminating Flux in Kepler and TESS Target Pixel Files