That's How We Roll: The NASA K2 Mission Science Products and Their Performance Metrics
arXiv:1512.06162 · doi:10.1088/1538-3873/128/965/075002
Abstract
NASA's exoplanet Discovery mission Kepler was reconstituted as the K2 mission a year after the failure of the 2nd of Kepler's 4 reaction wheels in May 2013. The new spacecraft pointing method now gives typical roll motion of 1.0 pixels peak-to-peak over 6 hours at the edges of the field, two orders of magnitude greater than for Kepler. Despite these roll errors, the flight system and its modified science data processing pipeline restores much of the photometric precision of the primary mission while viewing a wide variety of targets, thus turning adversity into diversity. We define metrics for data compression and pixel budget available in each campaign; the photometric noise on exoplanet transit and stellar activity time scales; residual correlations in corrected long cadence light curves; and the protection of test sinusoidal signals from overfitting in the systematic error removal process. We find that data compression and noise both increase linearly with radial distance from the center of the field of view, with the data compression proportional to star count as well. At the center, where roll motion is nearly negligible, the limiting 6 hour photometric precision for a quiet 12th magnitude star can be as low as 30 ppm, only 25% higher than that of Kepler. This noise performance is achieved without sacrificing signal fidelity; test sinusoids injected into the data are attenuated by less than 10% for signals with periods up 15 days. At time scales relevant to asteroseismology, light curves derived from K2 archive calibrated pixels have high-frequency noise amplitude within 40% of that achieved by Kepler. The improvements in K2 operations and science data analysis resulting from 1.5 yr of experience with this new mission concept, and quantified by the metrics in this paper, will support continuation of K2's already high level of scientific productivity in an extended K2 mission.
24 pages, 12 figures, accepted by PASP 1/21/2016
References in corpus (9)
- The K2 Mission: Characterization and Early results
- A Technique for Extracting Highly Precise Photometry for the Two-Wheeled Kepler Mission
- The K2 Ecliptic Plane Input Catalog (EPIC) and Stellar Classifications of 138,600 Targets in Campaigns 1-8
- Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)
- Planetary Candidates from the First Year of the K2 Mission
- A nearby M star with three transiting super-Earths discovered by K2
- Automated preparation of Kepler time series of planet hosts for asteroseismic analysis
- K2 Variable Catalogue II: Machine Learning Classification of Variable Stars and Eclipsing Binaries in K2 Fields 0-4
- K2P A photometry pipeline for the K2 mission
Cited by in corpus (65)
- Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25
- 197 Candidates and 104 Validated Planets in K2's First Five Fields
- K2SC: Flexible systematics correction and detrending of K2 light curves using Gaussian Process regression
- Zodiacal Exoplanets in Time (ZEIT) IV: seven transiting planets in the Praesepe cluster
- The flare catalog and the flare activity in the Kepler mission
- Characterizing K2 Candidate Planetary Systems Orbiting Low-Mass Stars II: Planetary Systems Observed During Campaigns 1-7
- TESS Hunt for Young and Maturing Exoplanets (THYME) III: a two-planet system in the 400 Myr Ursa Major Group
- Zodiacal Exoplanets in Time (ZEIT) VIII: A Two Planet System in Praesepe from K2 Campaign 16
- Superflares on solar-type stars from the first year observation of TESS
- TESS Hunt for Young and Maturing Exoplanets (THYME) VI: an 11 Myr giant planet transiting a very low-mass star in Lower Centaurus Crux
- Detection of Potential Transit Signals in 17 Quarters of Kepler Data: Results of the Final Kepler Mission Transiting Planet Search (DR25)
- Long Term Photometric Variability in Kepler Full Frame Images: Magnetic Cycles of Sun-Like Stars
- Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades
- Flares in Open Clusters with K2. II. Pleiades, Hyades, Praesepe, Ruprecht 147, and M67
- A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) -- I. Search for exoplanets and variable stars in the field of 47 Tuc
- Investigating the Rotational Phase of Stellar Flares on M dwarfs Using K2 Short Cadence Data
- Flares in Open Clusters with K2. I. M45 (Pleiades), M44 (Praesepe) and M67
- Two white dwarfs in ultrashort binaries with detached, eclipsing, likely substellar companions detected by K2
- Characterizing K2 Candidate Planetary Systems Orbiting Low-Mass Stars I: Classifying Low-mass Host Stars Observed During Campaigns 1-7
- A Low-Mass Exoplanet Candidate Detected By Transiting the Praesepe M Dwarf JS 183
- TOI-2076 and TOI-1807: Two young, comoving planetary systems within 50 pc identified by TESS that are ideal candidates for further follow-up
- The first sub-70 minute non-interacting WD-BD system: EPIC212235321
- Zodiacal Exoplanets in Time. X. The Orbit and Atmosphere of the Young "Neptune Desert"-Dwelling Planet K2-100b
- Scaling K2. VI. Reduced Small Planet Occurrence in High Galactic Amplitude Stars
- RAVE stars in K2 - I. Improving RAVE red giants spectroscopy using asteroseismology from K2 Campaign 1
- Three K2 Campaigns Yield Rotation Periods for 1013 Stars in Praesepe
- When flux standards go wild: white dwarfs in the age of Kepler
- The RAdial Velocity Experiment (RAVE): Parameterisation of RAVE spectra based on convolutional neural networks
- The Rotational Evolution of Young, Binary M Dwarfs
- Scaling K2. IV. A Uniform Planet Sample for Campaigns 1-8 and 10-18
- Zodiacal Exoplanets in Time (ZEIT) IX: a flat transmission spectrum and a highly eccentric orbit for the young Neptune K2-25b as revealed by Spitzer
- Scaling K2. II. Assembly of a Fully Automated C5 Planet Candidate Catalog Using EDI-Vetter
- Destroying Aliases from the Ground and Space: Super-Nyquist ZZ Cetis in K2 Long Cadence Data
- Data preparation for asteroseismology with TESS
- Re-Evaluating Small Long-Period Confirmed Planets From Kepler
- Asteroseismological analysis of the ultra-massive ZZ Ceti stars BPM~37093, GD~518, and SDSS~J0840+5222
- Asteroseismology of the Hyades with K2: first detection of main-sequence solar-like oscillations in an open cluster
- Extended Aperture Photometry of K2 RR Lyrae stars
- Orbital Architectures of Kepler Multis From Dynamical Instabilities
- Assessing 's Yield of Rocky Planets Around Nearby M Dwarfs
- The determination of asteroid H and G phase function parameters using GAIA DR2
- Asteroseismology of the Multiplanet System K2-93
- The SOPHIE search for northern extrasolar planets-XIX. A system including a cold sub-Neptune potentially transiting a V = 6.5 star HD88986
- New insights into the rotational evolution of near-solar age stars from the open cluster M67
- Critical Analysis of TESS Transit Photometric Data: Improved Physical Properties for Five Exoplanets
- Effects of Planetesimal Scattering: Explaining the Observed Offsets from Period Ratios 3:2 and 2:1
- The K2 M67 Study: Establishing the Limits of Stellar Rotation Period Measurements in M67 with K2 Campaign 5 Data
- Linearized Field Deblending: PSF Photometry for Impatient Astronomers
- Automated Extended Aperture Photometry of K2 variable stars
- The Period Distribution of Hot Jupiters is Not Dependent on Host Star Metallicity
- The K2 Asteroseismic KEYSTONE sample of Dwarf and Subgiant Solar-Like Oscillators. I: Data and Asteroseismic parameters
- Properties of a Previously Unidentified Instrumental Signature in that was Confused for AGN Variability
- K2 study of the Magnetic Precataclysmic Variable V1082 Sagittarius
- Convolutional Neural Networks for Searching Superflares from Pixel-level Data of the Transiting Exoplanet Survey Satellite
- Comparing the asteroseismic properties of pulsating pre-extremely low mass white dwarf and delta Scuti stars
- K2P: Reduced data from campaigns 0-4 of the K2 mission
- K2 Optical Emission from OJ 287 and Other Gamma-Ray Blazars on Hours-to-Weeks Timescales from 2014-2018
- Small and Close-In Planets are Uncommon Around A-type Stars
- TOI-3568 b: a super-Neptune in the sub-Jovian desert
- FALCO: a Foundation model of Astronomical Light Curves for time dOmain astronomy
- Uncovering the Rapidly Evolving Orbits of the Dynamic TOI-201 System
- K2 Photometry of RR Lyrae Stars
- Visual inspection of potential exocomet transits identified through machine learning and statistical methods
- Transit Hunt for Young and Maturing Exoplanets (THYME) VIII: a Pleiades-age association harboring two transiting planetary systems from Kepler
- A magnetic field detection in the massive O-type bright giant 63 Oph