The Doppler Method for the Detection of Exoplanets. Professor Artie Hatzes

Чтение книги онлайн.

Читать онлайн книгу The Doppler Method for the Detection of Exoplanets - Professor Artie Hatzes страница 3

Жанр:
Серия:
Издательство:
The Doppler Method for the Detection of Exoplanets - Professor Artie Hatzes

Скачать книгу

style="font-size:15px;">       6.4.2 The Template

       6.5 Calculation of the Doppler Shift

       6.6 Construction of an Iodine Cell

       6.7 Closing Remarks

       References

       7 Frequency Analysis of Time Series Data

       7.1 Introduction

       7.2 The Discrete Fourier Transform

       7.2.1 Convolution

       7.2.2 Visualizing Fourier Transforms

       7.3 The Lomb–Scargle Periodogram

       7.4 The Generalized Lomb–Scargle Periodogram

       7.5 The Bayesian Generalized Lomb–Scargle Periodogram

       7.6 Comparison of the Types of Periodograms

       7.7 The Spectral Window

       7.8 The Nyquist Frequency and Aliasing

       7.9 Frequency Resolution

       7.10 Assessing the Statistical Significance

       7.10.1 Using the Lomb–Scargle Periodogram

       7.10.2 Using the Fourier Amplitude Spectrum

       7.10.3 Bootstrap Randomization

       7.11 Finding Multiperiodic Signals in Your Data

       7.12 Required Number of Observations

       7.13 Frequency versus Period

       References

       8 Keplerian Orbits

       8.1 Orbital Parameters

       8.2 Describing the Orbital Motion

       8.3 The Radial Velocity Curve

       8.4 The Mass Function

       8.5 Mean Orbital Inclination

       8.6 Eccentric Orbits

       8.6.1 Observing Biases Caused by Eccentric Orbits

       8.6.2 Eccentric Orbits in the Fourier Domain

       8.6.3 Keplerian Periodograms

       8.7 Calculating Keplerian Orbits

       8.7.1 Transiting Planets

       8.8 Dynamical Effects

       8.8.1 Dynamical Stability

       8.8.2 Planet Interactions

       8.9 Barycentric Corrections

       References

       9 Avoiding False Planets: Rotational Modulation

       9.1 Introduction

       9.2 Spots

       9.3 Plage and Faculae

       9.4 Granulation and Convective Blueshift

       9.4.1 The Sun Viewed as a Star

       9.4.2 Velocity Spots

       9.5 Testing for Rotational Modulation

       9.5.1 Determining the Rotation Period of the Star

       9.5.2 Evolution of Statistical Significance

       9.5.3 Amplitude Variations

       References

       10 Avoiding False Planets: Indicators of Stellar Activity

       10.1 Activity Indicators

       10.1.1 Ca II H & K

       10.1.2 Hα

      

Скачать книгу