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Rybicki Press algorithm

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Extended Sparse Matrix arising from a semi-separable matrix whose semi-separable rank is .

The Rybicki–Press algorithm is a fast direct algorithm for inverting a matrix, whose entries are given by , where .[1] It is a computational optimization of a general set of statistical methods developed to determine whether two noisy, irregularly sampled data sets are, in fact, dimensionally shifted representations of the same underlying function.[2][3] The most common use of the algorithm is in the detection of periodicity in astronomical observations[3].

Recently, this method has been extended (Generalized Rybicki Press algorithm) for inverting matrices whose entries of the form [4]. The key observation in the Generalized Rybicki Press (GPP) algorithm is that the matrix is a semi-separable matrix with rank . More precisely, if the matrix has a semi-separable rank is , the cost for solving the linear system and obtaining the determinant of the matrix scales as , thereby making it extremely attractive for large matrices. This implementation of the GPP algorithm can be found here[5]. The key idea is that the dense matrix can be converted into a sparser matrix of a larger size (see figure on the right), whose sparsity structure can be leveraged to reduce the computational complexity.

The fact that matrix is a semi-separable matrix also forms the basis for celerite[6] library, which is a library for fast and scalable Gaussian Process (GP) Regression in one dimension[7] with implementations in C++, Python, and Julia. The celerite method[7] also provides an algorithm for generating samples from a high-dimensional distribution. The method has found attractive applications in a wide range of fields, especially in astronomical data analysis[8][9].

References

  1. ^ Rybicki, George B.; Press, William H. (1995), "Class of fast methods for processing Irregularly sampled or otherwise inhomogeneous one-dimensional data", Physical Review Letters, 74: 1060, arXiv:comp-gas/9405004, Bibcode:1995PhRvL..74.1060R, doi:10.1103/PhysRevLett.74.1060, PMID 10058924 Open access icon
  2. ^ Rybicki, George B.; Press, William H. (October 1992). "Interpolation, realization, and reconstruction of noisy, irregularly sampled data". The Astrophysical Journal. 398: 169. Bibcode:1992ApJ...398..169R. doi:10.1086/171845.Open access icon
  3. ^ a b MacLeod, C. L.; Brooks, K.; Ivezic, Z.; Kochanek, C. S.; Gibson, R.; Meisner, A.; Kozlowski, S.; Sesar, B.; Becker, A. C. (2011-02-10). "Quasar Selection Based on Photometric Variability". The Astrophysical Journal. 728 (1): 26. doi:10.1088/0004-637X/728/1/26. ISSN 0004-637X.
  4. ^ Ambikasaran, Sivaram (2015-12-01). "Generalized Rybicki Press algorithm". Numerical Linear Algebra with Applications. 22 (6): 1102–1114. doi:10.1002/nla.2003. ISSN 1099-1506.
  5. ^ "sivaramambikasaran/ESS". GitHub. Retrieved 2018-04-05.
  6. ^ "celerite — celerite 0.3.0 documentation". celerite.readthedocs.io. Retrieved 2018-04-05.
  7. ^ a b Foreman-Mackey, Daniel; Agol, Eric; Ambikasaran, Sivaram; Angus, Ruth (2017). "Fast and Scalable Gaussian Process Modeling with Applications to Astronomical Time Series". The Astronomical Journal. 154 (6): 220. doi:10.3847/1538-3881/aa9332. ISSN 1538-3881.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  8. ^ Foreman-Mackey, Daniel (2018). "Scalable Backpropagation for Gaussian Processes using Celerite". Research Notes of the AAS. 2 (1): 31. doi:10.3847/2515-5172/aaaf6c. ISSN 2515-5172.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  9. ^ Parviainen, Hannu (2018). Handbook of Exoplanets. Springer, Cham. pp. 1–24. doi:10.1007/978-3-319-30648-3_149-1.pdf. ISBN 9783319306483.

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