ensemble asteroseimology of 16,000 kepler red giants · ensemble asteroseimology of 16,000 kepler...

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Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu 1,2 , Tim Bedding 1,2 , Daniel Huber 1,2,3 , Dennis Stello 1,2,4 , and Marc Hon 4 1. University of Sydney. 2. Aarhus University. 3. University of Hawaii, 4. University of New South Wales.

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Page 1: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Ensemble Asteroseimology of 16,000 Kepler red giants

Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3,

Dennis Stello1,2,4, and Marc Hon4

1. University of Sydney. 2. Aarhus University. 3. University of Hawaii, 4. University of New South Wales.

Page 2: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Motivation1. Homogeneity: Largest sample

2. Precision: Full-length Kepler light curves

3. Measurements: , ,Amp, Width, Granulation

4. Output: Catalog of M, R, log g

2

Page 3: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

“SYD Pipeline”: Observables

Page 4: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Sample selection

4misclassified as MSunclassified in KIC

misclassified as Subgiantsmajority

Page 5: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Long-cadence datasets16,136 oscillators

𝜈max cutoff: >5 𝛍Hz“SYD”pipeline + visual inspection!!

0 5 10. 15Quarters

Page 6: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Seismic parameter comparison with literatureComparison

6Hekker et al. 2011

Page 7: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Seismic parameter comparisonComparison

7Hekker et al. 2011

Page 8: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Seismic parameter comparisonComparison

Peaking bagging: Davies et al. in prep.

Page 9: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

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“Nike Diagram”

Red Clump

Secondary Clump

RGB

Page 10: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Huber et al. (2011). The correction factor f is determined using the method from Sharma et al. (2016)

Masses and radii determination

Where

Masses and radii are inferred with the scaling relations:

Teff, [Fe/H]: KIC, LAMOST, APOGEE, CFOP…

Mathur et al. (2017)

Page 11: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Evolutionary Phase Classification from literature

Page 12: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Seismically-inferred M, R, and log g

mass loss ?

uncertain scaling relations ?

Page 13: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Massive oscillator

HeB

Page 14: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Massive oscillator

[37.13, 40.77] [3.10, 3.60]

Page 15: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Characterisation of power excess: Amp, Width, Granulation

Evolution

Page 16: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

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Characterisation of power excess: Amp, Width, Granulation

oscillation amplitude

oscillation amplitude

power excess width

granulation amplitude

Page 17: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

[Fe/H] influence on Amplitude[Fe/H]: Photometry + Spectroscopy

from Mathur et al. (2017)RGB only

Kjeldsen & Bedding (2008)Stello el al. (2011)

Page 18: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

[Fe/H] influence on Amplitude

Mathur et al. (2017)[Fe/H]: photometry+spectroscopy

MedianStandard Deviation

Page 19: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Pinsonneault et al. (2014)

How accurate are KIC [Fe/H] values ?

Page 20: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

Uncertainties

Page 21: Ensemble Asteroseimology of 16,000 Kepler red giants · Ensemble Asteroseimology of 16,000 Kepler red giants Jie Yu1,2, Tim Bedding1,2, Daniel Huber1,2,3, Dennis Stello1,2,4, and

1. We provided a catalog of seismic masses, radii and logg for ~16,000 oscillating red giants.

2. Oscillation and granulation amplitudes have dependencies on mass and Metallicity.

3. Power-excess width is an increasing function of mass.

Summary

Yu et al in prep.