Predicting the detectability of oscillations in solar-type stars observed by Kepler

Abstract

Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.

arXiv comment21 pages, 6 figures, accepted for publication Astrophysical Journal

References in corpus (25)

• Evolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models
• Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets
• Kepler Mission Design, Realized Photometric Performance, and Early Science
• Overview of the Kepler Science Processing Pipeline
• Kepler Asteroseismology Program: Introduction and First Results
• Selection, Prioritization, and Characteristics of Kepler Target Stars
• Initial Characteristics of Kepler Short Cadence Data
• Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system
• Determining global parameters of the oscillations of solar-like stars
• The relation between $\Delta \nu$ and ${\nu }_{max}$ for solar-like oscillations
• Red-giant seismic properties analyzed with CoRoT
• On detecting the large separation in the autocorrelation of stellar oscillation times series
• Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission
• A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764
• Asteroseismic Investigation of Known Planet Hosts in the Kepler Field
• The asteroseismic potential of Kepler: first results for solar-type stars
• An in-depth study of grid-based asteroseismic analysis
• The Kepler Pixel Response Function
• The amplitude of solar oscillations using stellar techniques
• The Octave (Birmingham - Sheffield Hallam) automated pipeline for extracting oscillation parameters of solar-like main-sequence stars
• Excitation of solar-like oscillations across the HR diagram
• Determination of stellar radii from asteroseismic Data
• Automatic Determination of Stellar Parameters via Asteroseismology of Stochastically Oscillating Stars: Comparison with Direct Measurements
• Multisite campaign on the open cluster M67. II. Evidence for solar-like oscillations in red giant stars
• Modelling the Autocovariance of the Power Spectrum of a Solar-Type Oscillator

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• Oscillation frequencies for 35 \Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning
• The asteroseismic potential of TESS: exoplanet-host stars
• Stellar mass and age determinations - I. Grids of stellar models from Z=0.006 to 0.04 and M=0.5 to 3.5 Msun
• Large eccentricity, low mutual inclination: the three-dimensional architecture of a hierarchical system of giant planets
• Global asteroseismic properties of solar-like oscillations observed by Kepler : A comparison of complementary analysis methods
• PLATO as it is: a legacy mission for Galactic archaeology
• Kepler-68: Three Planets, One With a Density Between That of Earth and Ice Giants
• What asteroseismology can do for exoplanets: Kepler-410A b is a Small Neptune around a bright star, in an eccentric orbit consistent with low obliquity
• First Results From The Hertzsprung Song Telescope: Asteroseismology Of The G5 Subgiant Star {\Mu}Her
• Filtering solar-like oscillations for exoplanet detection in radial velocity observations
• A Bayesian approach to scaling relations for amplitudes of solar-like oscillations in Kepler stars
• The Solar-Stellar Connection
• The K2-HERMES Survey: Age and Metallicity of the Thick Disc
• Asteroseismology from multi-month Kepler photometry: the evolved Sun-like stars KIC 10273246 and KIC 10920273
• The Asteroseismic Target List (ATL) for solar-like oscillators observed in 2-minute cadence with the Transiting Exoplanet Survey Satellite (TESS)
• Kepler-93b: A Terrestrial World Measured to within 120 km, and a Test Case for a New Spitzer Observing Mode
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• Limits on surface gravities of Kepler planet-candidate host stars from non-detection of solar-like oscillations
• Solar-like oscillations in red giants observed with \textit{Kepler}: influence of increased timespan on global oscillation parameters
• Observations of intensity fluctuations attributed to granulation and faculae on Sun-like stars from the Kepler mission
• Probing the deep end of the Milky Way with \emph{Kepler}: Asteroseismic analysis of 854 faint Red Giants misclassified as Cool Dwarfs
• Constructing a one-solar-mass evolutionary sequence using asteroseismic data from \textit{Kepler}
• Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the $TESS$ Continuous Viewing Zones and beyond
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• Super-Nyquist asteroseismology of solar-like oscillators with Kepler and K2 - expanding the asteroseismic cohort at the base of the red-giant branch
• Stellar granulation as seen in disk-integrated intensity. II. Theoretical scaling relations compared with observations
• Asteroseismology of 36 \emph{Kepler} subgiants -- I. Oscillation frequencies, linewidths and amplitudes
• A Search for Red Giant Solar-like Oscillations in All Kepler Data
• SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
• Orbital misalignment of the super-Earth $\pi$ Men c with the spin of its star
• The TESS-Keck Survey: Science Goals and Target Selection
• Asteroseismology of solar-type stars with K2
• FliPer: A global measure of power density to estimate surface gravities of main-sequence Solar-like stars and red giants
• A Catalogue of Solar-Like Oscillators Observed by TESS in 120-second and 20-second Cadence
• The Curious Case of KOI 4: Confirming Kepler's First Exoplanet
• The K2 Galactic Caps Project -- Going Beyond the \textit{Kepler} Field and Ageing the Galactic Disc
• Asteroseismic properties of solar-type stars observed with the NASA K2 mission: results from Campaigns 1-3 and prospects for future observations
• Study of HD 169392A observed by CoRoT and HARPS
• Prospects for detecting asteroseismic binaries in Kepler data
• Science Extraction from TESS Observations of Known Exoplanet Hosts
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• The K2 Galactic Archaeology Program Data Release 2: Asteroseismic results from campaigns 4, 6, & 7
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• Bolometric corrections of stellar oscillation amplitudes as observed by the Kepler, CoRoT, and TESS missions
• Surface gravities for 15,000 Kepler stars measured from stellar granulation and validated with Gaia DR2 parallaxes
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• A synthetic sample of short-cadence solar-like oscillators for TESS
• Detection of l=4 and l=5 modes in 12 years of solar VIRGO-SPM data --- Tests on Kepler observations of 16 Cyg A and B
• Stellar granulation as seen in disk-integrated intensity. I. Simplified theoretical modeling
• Influence of magnetic activity on the determination of stellar parameters through asteroseismology
• The Pulsation Properties of $\lambda$ Bootis Stars I. The Southern TESS Sample
• Rotation at the Fully Convective Boundary: Insights from Wide WD + MS Binary Systems
• Bayesian hierarchical inference of asteroseismic inclination angles
• The asteroseismic potential of CHEOPS
• Asteroseismology of Pulsating Stars
• M dwarf search for pulsations within Kepler GO program
• The Bayesian Asteroseismology data Modeling pipeline and its application to $K2$ data
• Measuring frequency and period separations in red-giant stars using machine learning
• A Distant Mirror: Solar Oscillations Observed on Neptune by the Kepler K2 Mission
• The K2 Asteroseismic KEYSTONE sample of Dwarf and Subgiant Solar-Like Oscillators. I: Data and Asteroseismic parameters
• On the characterization of GJ 504: a magnetically active planet-host star observed by the Transiting Exoplanet Survey Satellite (TESS)
• Luminaries in the Sky: The TESS Legacy Sample of Bright Stars. I. Asteroseismic detections in naked-eye main-sequence and sub-giant solar-like oscillators
• Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey
• The Swan: Data-Driven Inference of Stellar Surface Gravities for Cool Stars from Photometric Light Curves
• KIC 7177553: a quadruple system of two close binaries
• The potential for super-Nyquist asteroseismology with TESS
• A simple method to measure numax for asteroseismology: application to 16,000 oscillating Kepler red giants
• Detection of p-mode Oscillations in HD 35833 with NEID and TESS
• A new method to detect solar-like oscillations at very low S/N using statistical significance testing
• Robo-AO Kepler Asteroseismic Survey. II. Do Stellar Companions Inhibit Stellar Oscillations?
• A probabilistic method for detecting solar-like oscillations using meaningful prior information
• Testing the wavelength dependence of oscillations and granulation in red giants using Kepler and TESS
• The TESS Mission Target Selection Procedure
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• Stellar population synthesis based modelling of the Milky Way using asteroseismology of dwarfs and subgiants from Kepler
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• The K2 Galactic Archaeology Program: Overview, target selection and survey properties
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• The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates
• Solar-like stars observed by Kepler: an incredible adventure
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