Matches in SemOpenAlex for { <https://semopenalex.org/work/W3109059996> ?p ?o ?g. }
- W3109059996 endingPage "170" @default.
- W3109059996 startingPage "170" @default.
- W3109059996 abstract "Stellar light curves are well known to encode physical stellar properties. Precise, automated and computationally inexpensive methods to derive physical parameters from light curves are needed to cope with the large influx of these data from space-based missions such as Kepler and TESS. Here we present a new methodology which we call The Swan, a fast, generalizable and effective approach for deriving stellar surface gravity ($log g$) for main sequence, subgiant and red giant stars from Kepler light curves using local linear regression on the full frequency content of Kepler long cadence power spectra. With this inexpensive data-driven approach, we recover $log g$ to a precision of $sim$0.02 dex for 13,822 stars with seismic $log g$ values between 0.2-4.4 dex, and $sim$0.11 dex for 4,646 stars with Gaia derived $log g$ values between 2.3-4.6 dex. We further develop a signal-to-noise metric and find that granulation is difficult to detect in many cool main sequence stars ($T_{text{eff}}$ $lesssim$ 5500 K), in particular K dwarfs. By combining our $log g$ measurements with Gaia radii, we derive empirical masses for 4,646 subgiant and main sequence stars with a median precision of $sim$7%. Finally, we demonstrate that our method can be used to recover $log g$ to a similar mean absolute deviation precision for TESS-baseline of 27 days. Our methodology can be readily applied to photometric time-series observations to infer stellar surface gravities to high precision across evolutionary states." @default.
- W3109059996 created "2020-12-07" @default.
- W3109059996 creator A5005304021 @default.
- W3109059996 creator A5026700263 @default.
- W3109059996 creator A5035303223 @default.
- W3109059996 creator A5072389194 @default.
- W3109059996 date "2021-03-09" @default.
- W3109059996 modified "2023-09-23" @default.
- W3109059996 title "The Swan: Data-driven Inference of Stellar Surface Gravities for Cool Stars from Photometric Light Curves" @default.
- W3109059996 cites W1836177459 @default.
- W3109059996 cites W1933422323 @default.
- W3109059996 cites W1973500133 @default.
- W3109059996 cites W1986099565 @default.
- W3109059996 cites W2002731525 @default.
- W3109059996 cites W2006124034 @default.
- W3109059996 cites W2010885363 @default.
- W3109059996 cites W2011301426 @default.
- W3109059996 cites W2027724151 @default.
- W3109059996 cites W2035305287 @default.
- W3109059996 cites W2042268798 @default.
- W3109059996 cites W2042283668 @default.
- W3109059996 cites W2043250362 @default.
- W3109059996 cites W2061759127 @default.
- W3109059996 cites W2070508637 @default.
- W3109059996 cites W2077333009 @default.
- W3109059996 cites W2084992352 @default.
- W3109059996 cites W2088404988 @default.
- W3109059996 cites W2130023882 @default.
- W3109059996 cites W2135625048 @default.
- W3109059996 cites W2140035063 @default.
- W3109059996 cites W2142239297 @default.
- W3109059996 cites W2145159448 @default.
- W3109059996 cites W2146292423 @default.
- W3109059996 cites W2148205276 @default.
- W3109059996 cites W2151224589 @default.
- W3109059996 cites W2154470714 @default.
- W3109059996 cites W2158674056 @default.
- W3109059996 cites W2228974043 @default.
- W3109059996 cites W2287912467 @default.
- W3109059996 cites W2344233738 @default.
- W3109059996 cites W2531334071 @default.
- W3109059996 cites W2558422827 @default.
- W3109059996 cites W2739200487 @default.
- W3109059996 cites W2749229678 @default.
- W3109059996 cites W2757022617 @default.
- W3109059996 cites W2798158223 @default.
- W3109059996 cites W2798336535 @default.
- W3109059996 cites W2798341770 @default.
- W3109059996 cites W2802225833 @default.
- W3109059996 cites W2878410860 @default.
- W3109059996 cites W2885274016 @default.
- W3109059996 cites W2919458541 @default.
- W3109059996 cites W2919641564 @default.
- W3109059996 cites W2963266732 @default.
- W3109059996 cites W3000704192 @default.
- W3109059996 cites W3011221771 @default.
- W3109059996 cites W3019150006 @default.
- W3109059996 cites W3028685339 @default.
- W3109059996 cites W3032874046 @default.
- W3109059996 cites W3033055953 @default.
- W3109059996 cites W3038615701 @default.
- W3109059996 cites W3097976388 @default.
- W3109059996 cites W3098530261 @default.
- W3109059996 cites W3098986277 @default.
- W3109059996 cites W3099353780 @default.
- W3109059996 cites W3099706456 @default.
- W3109059996 cites W3100084450 @default.
- W3109059996 cites W3100149672 @default.
- W3109059996 cites W3100485643 @default.
- W3109059996 cites W3100729127 @default.
- W3109059996 cites W3100835200 @default.
- W3109059996 cites W3100874760 @default.
- W3109059996 cites W3101357606 @default.
- W3109059996 cites W3101404428 @default.
- W3109059996 cites W3101471258 @default.
- W3109059996 cites W3101482359 @default.
- W3109059996 cites W3101627046 @default.
- W3109059996 cites W3101742057 @default.
- W3109059996 cites W3102052121 @default.
- W3109059996 cites W3102262595 @default.
- W3109059996 cites W3102535523 @default.
- W3109059996 cites W3102910756 @default.
- W3109059996 cites W3103006437 @default.
- W3109059996 cites W3103145119 @default.
- W3109059996 cites W3103233164 @default.
- W3109059996 cites W3103709099 @default.
- W3109059996 cites W3103832984 @default.
- W3109059996 cites W3103876592 @default.
- W3109059996 cites W3103999057 @default.
- W3109059996 cites W3104019631 @default.
- W3109059996 cites W3104045077 @default.
- W3109059996 cites W3104487947 @default.
- W3109059996 cites W3104542759 @default.
- W3109059996 cites W3105153290 @default.
- W3109059996 cites W3105593080 @default.
- W3109059996 cites W3105934001 @default.
- W3109059996 cites W3106294757 @default.
- W3109059996 cites W3106402285 @default.