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- W3124483811 abstract "We present the first detections by the NASA K2 Mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign,1 (C1). We understand the asteroseismic detection thresholds for C1-like levels of photometric performance, and we can detect oscillations in subgiants having dominant oscillation frequencies around $1000,rm mu Hz$. Changes to the operation of the fine-guidance sensors are expected to give significant improvements in the high-frequency performance from C3 onwards. A reduction in the excess high-frequency noise by a factor of two-and-a-half in amplitude would bring main-sequence stars with dominant oscillation frequencies as high as ${simeq 2500},rm mu Hz$ into play as potential asteroseismic targets for K2." @default.
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- W3124483811 date "2015-10-01" @default.
- W3124483811 modified "2023-09-27" @default.
- W3124483811 title "Asteroseismology of Solar-Type Stars with<i>K2</i>: Detection of Oscillations in C1 Data" @default.
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- W3124483811 doi "https://doi.org/10.1086/683103" @default.
- W3124483811 hasPublicationYear "2015" @default.