{ "id": "1504.05199", "version": "v1", "published": "2015-04-20T20:01:27.000Z", "updated": "2015-04-20T20:01:27.000Z", "title": "K2P$^2$ $-$ A photometry pipeline for the K2 mission", "authors": [ "Mikkel N. Lund", "Rasmus Handberg", "Guy R. Davies", "William J. Chaplin", "Caitlin D. Jones" ], "comment": "14 pages, 20 figures, Accepted for publication in The Astrophysical Journal (Apj)", "categories": [ "astro-ph.SR", "astro-ph.EP", "astro-ph.IM" ], "abstract": "With the loss of a second reaction wheel, resulting in the inability to point continuously and stably at the same field of view, the NASA Kepler satellite recently entered a new mode of observation known as the K2 mission. The data from this redesigned mission present a specific challenge; the targets systematically drift in position on a ~6 hour time scale, inducing a significant instrumental signal in the photometric time series --- this greatly impacts the ability to detect planetary signals and perform asteroseismic analysis. Here we detail our version of a reduction pipeline for K2 target pixel data, which automatically: defines masks for all targets in a given frame; extracts the target's flux- and position time series; corrects the time series based on the apparent movement on the CCD (either in 1D or 2D) combined with the correction of instrumental and/or planetary signals via the KASOC filter (Handberg & Lund 2014), thus rendering the time series ready for asteroseismic analysis; computes power spectra for all targets, and identifies potential contaminations between targets. From a test of our pipeline on a sample of targets from the K2 campaign 0, the recovery of data for multiple targets increases the amount of potential light curves by a factor ${\\geq}10$. Our pipeline could be applied to the upcoming TESS (Ricker et al. 2014) and PLATO 2.0 (Rauer et al. 2013) missions.", "revisions": [ { "version": "v1", "updated": "2015-04-20T20:01:27.000Z" } ], "analyses": { "keywords": [ "k2 mission", "photometry pipeline", "k2 target pixel data", "planetary signals", "perform asteroseismic analysis" ], "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable" } } }