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A.S. gratefully acknowledges support by a National Science Foundation Graduate Research Fellowship (DGE-1745303). D.F. acknowledges support by NSF grant AST-1614941, "Exploring the Galaxy: 3-Dimensional Structure and Stellar Streams." We acknowledge Cammarata et al., whose figure pushed us to improve Figure 3, and found this up-to-date literature list highly helpful. We thank Taco Cohen, Erwan Allys, Josh Speagle, Catherine Zucker, Core Francisco Park, and Nayantara Mudur for helpful discussions. A.S. acknowledges Sophia S\'{a}nchez-Maes for helpful discussion and much support. Computations in this paper were run on the FASRC Cannon cluster supported by the FAS Division of Science Research Computing Group at Harvard University.
Data products and code associated with the paper "Equivariant Wavelets: Fast Rotation and Translation Invariant Wavelet Scattering Transforms" are made publicly available. This includes a snapshot of a wavelet scattering code and wavelet filter bank developed as part of this work, selected wavelet scattering coefficients used within the text, and code to reproduce the analysis and figures.
FOS: Computer and information sciences, wavelet transforms, machine learning, Computer Vision and Pattern Recognition (cs.CV), Computer Science - Computer Vision and Pattern Recognition, FOS: Physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), image classification
FOS: Computer and information sciences, wavelet transforms, machine learning, Computer Vision and Pattern Recognition (cs.CV), Computer Science - Computer Vision and Pattern Recognition, FOS: Physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), image classification
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 7 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |
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