A Guide to Distribution Theory and Fourier Transforms
By Robert S. Strichartz. 1994
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
- Bernhard Schölkopf
- Arthur Gretton
- Bharath K. Sriperumbudur
- Kenji Fukumizu
- Krikamol Muandet
- Yoshua Bengio
- Dacheng Tao
- Mingsheng Long
Citations in the corpus
- Collaborative Deep Learning for Recommender Systems (2014, background): “Note that if λs goes to infinity, the Gaussian distribution in Equation (1) will become a Dirac delta distribution [31] centered at σ(Xl−1,j∗Wl + bl), where σ(·) is the sigmoid function.”
- Infinite propagation speed for a two component Camassa-Holm equation (2009, methodology): “The reverse is also true, we can recover u from m by means of taking Fourier transforms [ 43 ], giving us”
- Approximation rates for neural networks with general activation functions (2019, background): “ (7) is a polynomialfor any ε>0. 3. supp(σˆ)⊂{0}. Proof. We begin by proving that (3) and (1) are equivalent. This follows from a characterization of distributions supported at a single point (see [21], section 6.3). In particular, a distribution supported at 0 must be a finite linear combinationo”
- Compactly Supported Solutions of the Camassa-Holm Equation (2005, methodology): “The reverse is also true by means of taking Fourier transforms [21], namely 2u(x) = e ∫ x”
- Universally optimal distribution of points on spheres (2006, background): “(See [ St , p. 124] or [R, p. 303].) That property follows immediately from the corresponding property of hN,g, because the set of positive-semidefinite matrices is closed.”
- Mathematics of thermoacoustic tomography (2007, background): “One can find simple introduction to the notions of microlocal analysis, such as the wave front set, for instance in [118].”
- A Survey on Bayesian Deep Learning (2016, methodology): “Note that if λs goes to infinity, the Gaussian distribution in Equation (5) will become a Dirac delta distribution [106] centered at σ (Xl−1, j∗Wl + bl ), where σ (·) is the sigmoid function, and the model will degenerate into a Bayesian formulation of vanilla SDAE.”
- Injective Hilbert Space Embeddings of Probability Measures (2008, background): “Conversely, every positive distribution comes from a locally finite positive measure [Str03, § 6.4].”
- Sampling-50 years after Shannon (2000, background): “From the point of view of computation, the Shannon model has a serious handicap because there are no band-limited functions that are compactly supported—a consequence of the Paley–Wiener theorem [117].”
- COSMOS - A Representation Scheme for 3D Free-Form Objects (1997, background): “Strictly speaking, for a suitably chosen set of all “test functions” on the domain of x [31], which places no restriction on us in practice.”
- A Note on the Degasperis-Procesi Equation (2005, methodology): “We recall that, by the Paley-Wiener theorem [21], an entire (analytic) function g(ξ), where ξ = η + iζ and η, ζ ∈ R, is the Fourier transform of a smooth function f : R → R with compact support in [−a, a] (for a > 0), namely”
- Towards Bayesian Deep Learning: A Survey (2016, background): “Note that if λs goes to infinity, the Gaussian distribution in Equation (8) will become a Dirac delta distribution [52] centered at σ(Xl−1,j∗Wl + bl), where σ(·) is the sigmoid function.”