Image Details

Choose export citation format:

Improving Power Spectrum Estimation Using Multitapering: Efficient Asteroseismic Analyses for Understanding Stars, the Milky Way, and Beyond

  • Authors: Aarya A. Patil, Gwendolyn M. Eadie, Joshua S. Speagle, 佳士 沈, David J. Thomson

Aarya A. Patil et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 8.

Comparison between distributions of LS and multitaper power spectrum estimates. LS is χ 2 distributed with degrees of freedom df = 2 as shown by the dashed line in black. mtLS and mtNUFFT are ﹩{\chi }_{2K}^{2}﹩ distributed, where K is the number of tapers. We show the K = 2 (df = 4) and K = 7 (df = 14) distributions in blue and dark pink curves. As K (or df) increases, the ﹩{\chi }_{2K}^{2}﹩ approaches a normal distribution with symmetric values around the mean, leading to better noise properties for the mtNUFFT periodogram.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse