transit analysis package zach gazak john tonry john johnson

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Transit Analysis Package Zach Gazak John Tonry John Johnson QuickTime™ and a decompressor are needed to see this picture.

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Transit Analysis Package

Zach Gazak

John Tonry

John Johnson

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Extrasolar Planets

1992: First discovered (pulsar timing variations)

1995: First orbiting Main Sequence star (radial velocity)

1999: First photometric transit light curve:

(Charbonneau et al. 2000)

Transiting Extrasolar Planets

~80 transiting exoplanets

Transits give us access to the geometry of the system

(Charbonneau et al. 2000)

NASA

Modeling Transit Photometry

Analytic light curve of (Mandel & Agol 2002)

Period, Inclination, Rp, a, Rs, e, ω, Tmid, limb darkening

Inclination, Rp/Rs, a/Rs:

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Parameter Statistics: MCMC

Markov Chain Monte Carlo

Gives access to Bayesian probability distribution

model x0

trial state x’

Likelihood: –χ

‾2~exp[ ]

ℒ’

ℒ’

ℒ0

meets Jump probability?

Parameter Statistics: MCMC

Markov Chain Monte Carlo

Gives access to Bayesian probability distribution

model x0trial state x’

More likely states always selected, but MCMC can explore.

. . . xN

MCMC Bayesian Distributions

15.1%

MCMC Bayesian Distributions

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MCMC Bayesian Distributions

Testing the MCMC Algorithm

Generate and Analyze Synthetic Transits

WASP 10b HAT 12b

Testing the MCMC Algorithm

Transits of varying precision must agree:

Where is Transit Science Going?

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Is the “Classic” MCMC Enough?

Most light curves show correlated “red” noise:

But “classic” MCMC is not able to compensate.

Wavelet Processing

“Fourier Like” but sensitive to frequency and scale.

Daubechies 4th order

Wavelet Processing

“Fourier Like” but sensitive to frequency and scale.

Daubechies 4th order

Red Noise FilteringHow “Likely” is the noise described by a (σwhite, σred) pair?

(Carter & Winn 2009)

Maximize that “Wavelet Likelihood”:

Wavelet Basis MCMC

Wavelet decompose residuals (data - model fit)

Use wavelet likelihood instead of “Classic”

Wavelet Basis MCMC

For contaminated data, “Classic” MCMC is insufficient!

Severely underestimates probability distributions.

“True” value Classic

Wavelet

TrES-3b

TrES-3b

TrES-3b

TAP in Action

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Transit Analysis Package

Zach Gazak

John Tonry

John Johnson

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