Seismic inference of 57 stars using full-length Kepler data sets

Orlagh Creevey; Travis S. Metcalfe; David Salabert; Savita Mathur; Mathias Schultheis; Rafael A. García; Frédéric Thévenin; Michaël Bazot; Haiying Xu

doi:10.1051/epjconf/201716003007

Seismic inference of 57 stars using full-length Kepler data sets

Orlagh Creevey
, Travis S. Metcalfe
, David Salabert
, Savita Mathur
, Mathias Schultheis
, Rafael A. García
, Frédéric Thévenin
, Michaël Bazot
, Haiying Xu

Application Scalability and Performance Group

Research output: Contribution to journal › Conference article › peer-review

Abstract

We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems. We validate the distances derived from the astrometric Gaia-Tycho solution. Ensemble analysis of the stellar properties reveals a trend of mixing-length parameter with the surface gravity and effective temperature. We derive a linear relationship with the seismic quantity "r₀₂" to estimate the stellar age. Finally, we define the stellar regimes where the Kjeldsen et al (2008) empirical surface correction for 1D model frequencies is valid.

Original language	English
Article number	03007
Journal	EPJ Web of Conferences
Volume	160
DOIs	https://doi.org/10.1051/epjconf/201716003007
State	Published - Oct 27 2017
Event	Seismology of the Sun and the Distant Stars 2016 - Using Today's Successes to Prepare the Future - TASC2 and KASC9 Workshop - SPACEINN and HELAS8 Conference - Terceira, Acores Islands, Portugal Duration: Jul 11 2016 → Jul 25 2016

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@article{092e2321eca2401ea2455c166a4959fc,

title = "Seismic inference of 57 stars using full-length Kepler data sets",

abstract = "We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems. We validate the distances derived from the astrometric Gaia-Tycho solution. Ensemble analysis of the stellar properties reveals a trend of mixing-length parameter with the surface gravity and effective temperature. We derive a linear relationship with the seismic quantity {"}r02{"} to estimate the stellar age. Finally, we define the stellar regimes where the Kjeldsen et al (2008) empirical surface correction for 1D model frequencies is valid.",

author = "Orlagh Creevey and Metcalfe, \{Travis S.\} and David Salabert and Savita Mathur and Mathias Schultheis and Garc{\'i}a, \{Rafael A.\} and Fr{\'e}d{\'e}ric Th{\'e}venin and Micha{\"e}l Bazot and Haiying Xu",

note = "Publisher Copyright: {\textcopyright} Owned by the authors, published by EDP Sciences, 2017.; Seismology of the Sun and the Distant Stars 2016 - Using Today's Successes to Prepare the Future - TASC2 and KASC9 Workshop - SPACEINN and HELAS8 Conference ; Conference date: 11-07-2016 Through 25-07-2016",

year = "2017",

month = oct,

day = "27",

doi = "10.1051/epjconf/201716003007",

language = "English",

volume = "160",

journal = "EPJ Web of Conferences",

issn = "2101-6275",

publisher = "EDP Sciences",

}

TY - JOUR

T1 - Seismic inference of 57 stars using full-length Kepler data sets

AU - Creevey, Orlagh

AU - Metcalfe, Travis S.

AU - Salabert, David

AU - Mathur, Savita

AU - Schultheis, Mathias

AU - García, Rafael A.

AU - Thévenin, Frédéric

AU - Bazot, Michaël

AU - Xu, Haiying

PY - 2017/10/27

Y1 - 2017/10/27

N2 - We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems. We validate the distances derived from the astrometric Gaia-Tycho solution. Ensemble analysis of the stellar properties reveals a trend of mixing-length parameter with the surface gravity and effective temperature. We derive a linear relationship with the seismic quantity "r02" to estimate the stellar age. Finally, we define the stellar regimes where the Kjeldsen et al (2008) empirical surface correction for 1D model frequencies is valid.

AB - We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems. We validate the distances derived from the astrometric Gaia-Tycho solution. Ensemble analysis of the stellar properties reveals a trend of mixing-length parameter with the surface gravity and effective temperature. We derive a linear relationship with the seismic quantity "r02" to estimate the stellar age. Finally, we define the stellar regimes where the Kjeldsen et al (2008) empirical surface correction for 1D model frequencies is valid.

UR - https://www.scopus.com/pages/publications/85033455500

U2 - 10.1051/epjconf/201716003007

DO - 10.1051/epjconf/201716003007

M3 - Conference article

AN - SCOPUS:85033455500

SN - 2101-6275

VL - 160

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

M1 - 03007

T2 - Seismology of the Sun and the Distant Stars 2016 - Using Today's Successes to Prepare the Future - TASC2 and KASC9 Workshop - SPACEINN and HELAS8 Conference

Y2 - 11 July 2016 through 25 July 2016

ER -

Seismic inference of 57 stars using full-length Kepler data sets

Abstract

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