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DeepSphere: Efficient spherical convolutional neural network with HEALPix sampling for cosmological applications
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Gradient-based learning applied to document recognition
Lecun, Y., Bottou, L., Bengio, Y., & Haffner, P. (1998) · Proceedings of the IEEE · doi:10.1109/5.726791 · Cited by 58,805 · cited 1×
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BackgroundFully convolutional networks for semantic segmentation
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MethodBatch Normalization: Accelerating Deep Network Training by Reducing Internal Covariate Shift
Ioffe, S., & Szegedy, C. (2015) · arXiv · doi:10.48550/arxiv.1502.03167 · Cited by 27,818 · cited 2×
“The batch normalization layer [33] computes Y = BN(X) such as”
BackgroundSEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Smith, K. M., Dunkley, J., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M. R., Page, L., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/18 · Cited by 8,802 · cited 1×
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BackgroundAdvances In Deep Learning On Graphs (Gsp'18 Workshop)Preprint
Defferrard, M., Bresson, X., & Vandergheynst, P. (2016) · arXiv (Cornell University) · doi:10.48550/arxiv.1606.09375 · Cited by 7,021 · cited 3×
“We use the graph CNN formulation introduced in [26], and a pooling strategy that exploits a hierarchical pixelisation of the sphere to analyse the data at multiple scales.”
MethodSelf-citationGórski, K., Hivon, E., Banday, A., Wandelt, B. D., Hansen, F., Reinecke, M., & Bartelmann, M. (2004) · The Astrophysical Journal · doi:10.1086/427976 · Cited by 5,217 · cited 3×
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MethodPlanck 2015 results. II. Low Frequency Instrument data processings
Ade, P., Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A., Barreiro, R., Bartolo, N., Basak, S., et al. (2013) · doi:10.1051/0004-6361/201525818 · Cited by 4,758
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BackgroundMethodGeometric Deep Learning: Going beyond Euclidean data
Bronstein, M. M., Bruna, J., LeCun, Y., Szlam, A., & Vandergheynst, P. (2017) · IEEE Signal Processing Magazine · doi:10.1109/msp.2017.2693418 · Cited by 3,661 · cited 1×
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BackgroundA Convolutional Neural Network for Modelling Sentences
Kalchbrenner, N., Grefenstette, E., & Blunsom, P. (2014) · Proceedings of the 52nd Annual Meeting of the Association for Computational Linguistics (Volume 1: Long Papers) · doi:10.3115/v1/p14-1062 · Cited by 3,601 · cited 1×
“Second, they did not take 11 Heisenberg’s uncertainty principle states that a filter cannot be arbitrarily concentrated in one domain without being de-concentrated in the other. advantage of a hierarchical pixelization of the sphere and resorted to dynamic pooling [58].”
BackgroundStriving for Simplicity: The All Convolutional Net
Springenberg, J. T., Dosovitskiy, A., Brox, T., & Riedmiller, M. (2014) · arXiv · doi:10.48550/arxiv.1412.6806 · Cited by 3,447
Gated Graph Sequence Neural NetworksPreprint
Li, Y., Tarlow, D., Brockschmidt, M., & Zemel, R. S. (2015) · arXiv (Cornell University) · doi:10.48550/arxiv.1511.05493 · Cited by 3,329 · cited 1×
“Such global summarization as the AV layer is commonly used along graph convolutions to classify graphs of varying sizes (as it is invariant to vertex permutation) [45, 46].”
MethodAlam, S., Ata, M., Bailey, S., Beutler, F., Bizyaev, D., Blazek, J. A., Bolton, A. S., Brownstein, J. R., Burden, A., Chuang, C.-H., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx721 · Cited by 3,056 · cited 1×
“Observables that cover large parts of the sky, such as the Cosmic Microwave Background (CMB) [1–3], neutral hydrogen [4, 5], galaxy clustering [6], gravitational lensing [7, 8], and others, have been used to constrain cosmological and astrophysical models.”
BackgroundConvolutional Networks on Graphs for Learning Molecular Fingerprints
Duvenaud, D., Maclaurin, D., Aguilera-Iparraguirre, J., Gómez-Bombarelli, R., Hirzel, T., Aspuru-Guzik, A., & Adams, R. P. (2015) · arXiv · doi:10.48550/arxiv.1509.09292 · Cited by 2,628 · cited 1×
“Such global summarization as the AV layer is commonly used along graph convolutions to classify graphs of varying sizes (as it is invariant to vertex permutation) [45, 46].”
MethodRepresentation Learning on Graphs: Methods and ApplicationsPreprint
Hamilton, W. L., Ying, R., & Leskovec, J. (2017) · IEEE Data Engineering Bulletin · doi:10.48550/arxiv.1709.05584 · Cited by 2,203 · cited 1×
“Many formulations of graph neural networks, reviewed by [59] and [60], have been proposed.”
BackgroundPlanck 2015 results. I. Overview of products and scientific results
Planck Collaboration R. Adam, Ade, P., Aghanim, N., Akrami, Y., Alves, M., Arnaud, M., Arroja, F., Aumont, J., Baccigalupi, C., Ballardini, M., et al. (2015) · HAL · doi:10.1051/0004-6361/201527101 · Cited by 2,072
Geometric Deep Learning on Graphs and Manifolds Using Mixture Model CNNs
Monti, F., Boscaini, D., Masci, J., Rodola, E., Svoboda, J., & Bronstein, M. M. (2017) · 2017 IEEE Conference on Computer Vision and Pattern Recognition (CVPR) · doi:10.1109/cvpr.2017.576 · Cited by 1,820 · cited 1×
“This idea has been generalized to arbitrary 2D manifolds for shape alignment and retrieval [50–52].”
MethodMallat, S. (2012) · Communications on Pure and Applied Mathematics · doi:10.1002/cpa.21413 · Cited by 1,127 · cited 1×
“Localization is desired for the transformation to be stable to local deformation [57], and most interactions in the data are local anyway.”
BackgroundHI4PI: a full-sky H i survey based on EBHIS and GASS
Bekhti, N., Flöer, L., Keller, R., Kerp, J., Lenz, D., Winkel, B., Bailin, J., Calabretta, M., Dedes, L., Ford, H., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201629178 · Cited by 1,035
Structured Sequence Modeling with Graph Convolutional Recurrent Networks
Seo, Y., Defferrard, M., Vandergheynst, P., & Bresson, X. (2018) · Lecture notes in computer science · doi:10.1007/978-3-030-04167-0_33 · Cited by 977 · cited 1×
“By combining graph convolutional layers and recurrent layers [66], they can, for example, model structured time series such as tra ffi c on road networks [67], or recursively complete matrices for recommendation [68].”
Self-citationKiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
Hildebrandt, H., Viola, M., Heymans, C., Joudaki, S., Kuijken, K., Blake, C., Erben, T., Joachimi, B., Klaes, D., Miller, L., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2805 · Cited by 817 · cited 1×
“Observables that cover large parts of the sky, such as the Cosmic Microwave Background (CMB) [1–3], neutral hydrogen [4, 5], galaxy clustering [6], gravitational lensing [7, 8], and others, have been used to constrain cosmological and astrophysical models.”
BackgroundAbolfathi, B., Aguado, D., Aguilar, G., Prieto, C., Almeida, A., Ananna, T., Anders, F., Anderson, S., Andrews, B., Anguiano, B., et al. (2017) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/aa9e8a · Cited by 810 · cited 2×
“…of modeling the data domain with a graph allows one to easily model [17], with galactic plane masked, (middle) map of galaxy number counts (number of galaxies per arcmin 2 ) in SDSS DR14 [18], and (right) simulated weak lensing convergence map (dimensionless) simulated with DES DR1 mask [19].”
BackgroundMethodGeodesic Convolutional Neural Networks on Riemannian Manifolds
Masci, J., Boscaini, D., Bronstein, M. M., & Vandergheynst, P. (2015) · 2015 IEEE International Conference on Computer Vision Workshop (ICCVW) · doi:10.1109/iccvw.2015.112 · Cited by 721 · cited 1×
“This idea has been generalized to arbitrary 2D manifolds for shape alignment and retrieval [50–52].”
MethodKondor, R., & Trivedi, S. (2018) · International Conference on Machine Learning · doi:10.48550/arxiv.1802.03690 · Cited by 684 · cited 1×
“See [56] for a rigorous treatment of convolution and equivariance in NNs.”
BackgroundGeometric Matrix Completion with Recurrent Multi-Graph Neural NetworksPreprint
Monti, F., Bronstein, M., & Bresson, X. (2017) · Neural Information Processing Systems · doi:10.48550/arxiv.1704.06803 · Cited by 558 · cited 1×
“By combining graph convolutional layers and recurrent layers [66], they can, for example, model structured time series such as tra ffi c on road networks [67], or recursively complete matrices for recommendation [68].”
Learning shape correspondence with anisotropic convolutional neural networksPreprint
Boscaini, D., Masci, J., Rodolà, E., & Bronstein, M. (2016) · Neural Information Processing Systems · doi:10.48550/arxiv.1605.06437 · Cited by 540 · cited 1×
“This idea has been generalized to arbitrary 2D manifolds for shape alignment and retrieval [50–52].”
MethodBartelmann, M. (2010) · Classical and Quantum Gravity · doi:10.1088/0264-9381/27/23/233001 · Cited by 495
3D Graph Neural Networks for RGBD Semantic Segmentation
Qi, X., Liao, R., Jia, J., Fidler, S., & Urtasun, R. (2017) · 2017 IEEE International Conference on Computer Vision (ICCV) · doi:10.1109/iccv.2017.556 · Cited by 482 · cited 1×
“Thanks to their versatility, graph neural networks have been used in a variety of tasks, such as identifying diseases from brain connectivity networks [61] or population graphs [62], designing drugs using molecular graphs [63], segmenting 3D point clouds [64], optimizing shapes to be aerodynamic [65], and many more.”
MethodCoors, B., Condurache, A., & Geiger, A. (2018) · European Conference on Computer Vision · doi:10.1007/978-3-030-01240-3_32 · Cited by 457 · cited 4×
“A first approach, explored by [20] for molecular modeling and [21, 22] for omnidirectional imaging, is to use a 2D CNN on a discretisation of the sphere that is a grid, such as the equirectangular projection (Figure 6, left panel), or a set of grids, such as the cubed-sphere defined by [47] (Figure…”
BackgroundMethodInfluentialRecognizing scene viewpoint using panoramic place representation
Xiao, J.-X., Ehinger, K. A., Oliva, A., & Torralba, A. (2012) · 2012 IEEE Conference on Computer Vision and Pattern Recognition · doi:10.1109/cvpr.2012.6247991 · Cited by 414 · cited 1×
“This approach has been extensively used for cosmological maps [9, 11, 12, 23] and omnidirectional imaging [48, 49].”
MethodClebsch-Gordan Nets: a Fully Fourier Space Spherical Convolutional Neural Network
Kondor, R., Lin, Z., & Trivedi, S. (2018) · Neural Information Processing Systems · doi:10.48550/arxiv.1806.09231 · Cited by 395 · cited 1×
“…log N pix , plus N pix matrix multiplications of size N pix for a total cost of O N 3 / 2 pix operations. leveraged to avoid SHTs between layers (it does a non-linear transformation in the spectral domain), the transform itself costs O ( N 3 / 2 pix ), for no reduction of overall complexity [55].”
BackgroundMetric learning with spectral graph convolutions on brain connectivity networks
Ktena, S. I., Parisot, S., Ferrante, E., Rajchl, M., Lee, M., Glocker, B., & Rueckert, D. (2017) · NeuroImage · doi:10.1016/j.neuroimage.2017.12.052 · Cited by 382 · cited 1×
“…to their versatility, graph neural networks have been used in a variety of tasks, such as identifying diseases from brain connectivity networks [61] or population graphs [62], designing drugs using molecular graphs [63], segmenting 3D point clouds [64], optimizing shapes to be aerodynamic…”
MethodRonchi, C., Iacono, R., & Paolucci, P. (1996) · Journal of Computational Physics · doi:10.1006/jcph.1996.0047 · Cited by 381 · cited 2×
“Left: a grid using equiang l r spacing in a standard spherical-pol r c ordinate syst m, and Right: An equiang lar c bed-sphere rep sentatio , as describ d in Ronchi et al. (1996).”
MethodConvergence of Laplacian Eigenmaps
Belkin, M., & Niyogi, P. (2006) · Neural Information Processing Systems · doi:10.7551/mitpress/7503.003.0021 · Cited by 341 · cited 1×
“Indeed, [34] showed that the graph Laplacian converges to the Laplace-Beltrami when the number of pixels goes to in-finity providing uniform sampling of the manifold and a fully connected graph built with exponentially decaying weights.”
BackgroundSpectral Graph Convolutions for Population-Based Disease Prediction
Parisot, S., Ktena, S. I., Ferrante, E., Lee, M., Moreno, R. G., Glocker, B., & Rueckert, D. (2017) · Lecture notes in computer science · doi:10.1007/978-3-319-66179-7_21 · Cited by 260 · cited 1×
“…graph neural networks have been used in a variety of tasks, such as identifying diseases from brain connectivity networks [61] or population graphs [62], designing drugs using molecular graphs [63], segmenting 3D point clouds [64], optimizing shapes to be aerodynamic [65], and many more.”
MethodStationary Signal Processing on Graphs
Perraudin, N., & Vandergheynst, P. (2017) · IEEE Transactions on Signal Processing · doi:10.1109/tsp.2017.2690388 · Cited by 240 · cited 1×
“We refer the reader to [37, Sec 2.2] for a detailed discussion of the connection between translation T i and localization T i .”
MethodInfluentialSelf-citationPanoContext: A Whole-Room 3D Context Model for Panoramic Scene Understanding
Zhang, Y., Song, S., Tan, P., & Xiao, J. (2014) · Lecture notes in computer science · doi:10.1007/978-3-319-10599-4_43 · Cited by 239 · cited 1×
“This approach has been extensively used for cosmological maps [9, 11, 12, 23] and omnidirectional imaging [48, 49].”
MethodA fast transform for spherical harmonics
Mohlenkamp, M. J. (1997) · doi:10.1007/bf01261607 · Cited by 237 · cited 1×
“Accelerated schemes however exist for some sampling sets [see 39, 53, 54, for examples].”
BackgroundCosmology with a SKA HI intensity mapping survey
Santos, M. G., Bull, P., Alonso, D., Camera, S., Ferreira, P., Bernardi, G., Maartens, R., Viel, M., Villaescusa-Navarro, F., Abdalla, F., et al. (2015) · doi:10.22323/1.215.0019 · Cited by 172 · cited 1×
“Observables that cover large parts of the sky, such as the Cosmic Microwave Background (CMB) [1–3], neutral hydrogen [4, 5], galaxy clustering [6], gravitational lensing [7, 8], and others, have been used to constrain cosmological and astrophysical models.”
BackgroundFast Algorithms for Spherical Harmonic Expansions
Rokhlin, V., & Tygert, M. (2006) · SIAM Journal on Scientific Computing · doi:10.21236/ada461342 · Cited by 135 · cited 1×
“Accelerated schemes however exist for some sampling sets [see 39, 53, 54, for examples].”
BackgroundL-PICOLA: A parallel code for fast dark matter simulation
Howlett, C., Manera, M., & Percival, W. (2015) · Astronomy and Computing · doi:10.1016/j.ascom.2015.07.003 · Cited by 131 · cited 2×
“L-PICOLA [72] is used for fast and approximate N-body simulations.”
MethodNon-Gaussian information from weak lensing data via deep learning
Gupta, A., Matilla, J. M. Z., Hsu, D., & Haiman, Z. (2018) · Physical Review D · doi:10.1103/physrevd.97.103515 · Cited by 128 · cited 4×
“A typical global regression task is to infer the parameters of a cosmological model from maps [11, 23].”
BackgroundMethodInfluentialLearning Spherical Convolution for Fast Features from 360° ImageryPreprint
Su, Y.-C., & Grauman, K. L. (2017) · arXiv (Cornell University) · doi:10.48550/arxiv.1708.00919 · Cited by 127 · cited 3×
“One approach is to apply a standard 2D CNN to a grid discretisation of the sphere [20–22].”
BackgroundMethodLearning SO(3) Equivariant Representations with Spherical CNNs
Esteves, C., Allen-Blanchette, C., Makadia, A., & Daniilidis, K. (2019) · International Journal of Computer Vision · doi:10.1007/s11263-019-01220-1 · Cited by 119 · cited 3×
“Ideally, we would compare DeepSphere to alternative spherical CNNs like [24] and [25].”
MethodInfluentialDeep learning from 21-cm tomography of the Cosmic Dawn and Reionization
Gillet, N., Mesinger, A., Greig, B., Liu, A., & Ucci, G. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz010 · Cited by 115
Geodesic Convolutional Shape OptimizationPreprint
Baqué, P., Remelli, E., Fleuret, F., & Fua, P. (2018) · International Conference on Machine Learning · doi:10.48550/arxiv.1802.04016 · Cited by 94 · cited 1×
“Thanks to their versatility, graph neural networks have been used in a variety of tasks, such as identifying diseases from brain connectivity networks [61] or population graphs [62], designing drugs using molecular graphs [63], segmenting 3D point clouds [64], optimizing shapes to be aerodynamic [65], and many more.”
MethodEstimating Cosmological Parameters from the Dark Matter DistributionPreprint
Ravanbakhsh, S., Oliva, J. B., Fromenteau, S., Price, L. C., Ho, S., Schneider, J., & Póczos, B. (2017) · arXiv (Cornell University) · doi:10.48550/arxiv.1711.02033 · Cited by 85 · cited 1×
“Convolutional Neural Networks (CNNs) have been proposed as an alternative analysis tool in cosmology thanks to their ability to automatically design relevant statistics to maximise the precision 1 of the parameter estimation [9–16], while maintaining robustness to noise.”
BackgroundCosmological constraints from noisy convergence maps through deep learning
Fluri, J., Kacprzak, T., Refregier, A., Amara, A., Lucchi, A., & Hofmann, T. (2018) · Physical Review D · doi:10.1103/physrevd.98.123518 · Cited by 83 · cited 4×
“A typical global regression task is to infer the parameters of a cosmological model from maps [11, 23].”
BackgroundMethodInfluentialSelf-citationGraph-Based Classification of Omnidirectional Images
Pascal Frossard, B., & Khasanova, R. (2017) · IEEE International Conference on Computer Vision Workshops · doi:10.1109/iccvw.2017.106 · Cited by 76 · cited 2×
“For example, [35] uses the inverse of the distance instead.”
MethodDark energy survey year 1 results: curved-sky weak lensing mass map
Chang, C., Pujol, A., Mawdsley, B., Bacon, D., Elvin-Poole, J., Melchior, P., Kovács, A., Jain, B., Leistedt, B., Giannantonio, T., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx3363 · Cited by 75
Self-citationLibsharp – spherical harmonic transforms revisited
Reinecke, M., & Seljebotn, D. S. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321494 · Cited by 75 · cited 3×
“On a single core, a naive implementation of our method is ten to twenty times faster for N side = 2048, with K = 20 and K = 5, respectively, than using the spherical harmonic transform at (cid:96) max = 3 N side implemented by the highly optimized libsharp [39] library used by HEALPix.”
BackgroundMethodApproximate Fast Graph Fourier Transforms via Multilayer Sparse Approximations
Magoarou, L. L., Gribonval, R., & Tremblay, N. (2017) · IEEE Transactions on Signal and Information Processing over Networks · doi:10.1109/tsipn.2017.2710619 · Cited by 67 · cited 1×
“As no efficient and general fast Fourier transform (FFT) exists for graphs [38], the execution of the Fourier transform by multiplication of the signal f by the dense matrix U costs O(N2 pix) operations.”
MethodGlobal and local uncertainty principles for signals on graphs
Perraudin, N., Ricaud, B., Shuman, D. I., & Vandergheynst, P. (2018) · APSIPA Transactions on Signal and Information Processing · doi:10.1017/atsip.2018.2 · Cited by 58
Self-citationDetecting cosmic strings in the CMB with the Canny algorithm
Amsel, S., Berger, J., & Brandenberger, R. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/04/015 · Cited by 58 · cited 1×
“Segmentation and feature detection [41] are examples of dense classification tasks.”
BackgroundClassifying the large-scale structure of the universe with deep neural networks
Aragón-Calvo, M. A. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz393 · Cited by 58
Machine learning cosmological structure formation
Lucie-Smith, L., Peiris, H., Pontzen, A., & Lochner, M. (2018) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1719 · Cited by 56 · cited 1×
“Convolutional Neural Networks (CNNs) have been proposed as an alternative analysis tool in cosmology thanks to their ability to automatically design relevant statistics to maximise the precision1 of the parameter estimation [9–16], while maintaining robustness to noise.”
BackgroundHop, P., Allgood, B., & Yu, J. (2018) · Molecular Pharmaceutics · doi:10.1021/acs.molpharmaceut.7b01144 · Cited by 54 · cited 1×
“…graph neural networks have been used in a variety of tasks, such as identifying diseases from brain connectivity networks [61] or population graphs [62], designing drugs using molecular graphs [63], segmenting 3D point clouds [64], optimizing shapes to be aerodynamic [65], and many more.”
MethodRecent discoveries from the cosmic microwave background: a review of recent progress
Staggs, S. T., Dunkley, J., & Page, L. A. (2017) · Reports on Progress in Physics · doi:10.1088/1361-6633/aa94d5 · Cited by 48 · cited 1×
“Observables that cover large parts of the sky, such as the Cosmic Microwave Background (CMB) [1–3], neutral hydrogen [4, 5], galaxy clustering [6], gravitational lensing [7, 8], and others, have been used to constrain cosmological and astrophysical models.”
BackgroundKrachmalnicoff, N., & Tomasi, M. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201935211 · Cited by 47
Cosmological model discrimination with Deep LearningPreprint
Schmelzle, J., Lucchi, A., Kacprzak, T., Amara, A., Sgier, R., Réfrégier, A., & Hofmann, T. (2017) · arXiv (Cornell University) · doi:10.48550/arxiv.1707.05167 · Cited by 40 · cited 8×
“This approach has been extensively used for cosmological maps [9, 11, 12, 23] and omnidirectional imaging [48, 49].”
BackgroundMethodInfluentialSelf-citationCosmological constraints from the convergence 1-point probability distribution
Patton, K., Blazek, J., Honscheid, K., Huff, E., Melchior, P., Ross, A., & Suchyta, E. (2016) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1626 · Cited by 31 · cited 1×
“tures that are (i) the power spectral densities (PSD) of maps, and (ii) the histogram of pixels in the maps [72].”
BackgroundFast generation of covariance matrices for weak lensing
Sgier, R., Réfrégier, A., Amara, A., & Nicola, A. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/01/044 · Cited by 30 · cited 2×
“The simulations are created using the fast lightcone method UFalcon described in [71].”
MethodSelf-citationA convolutional neural network for cosmic string detection in CMB temperature maps
Ciuca, R., Hernández, O. F., & Wolman, M. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz491 · Cited by 29
Harmonic inpainting of the cosmic microwave background sky: Formulation and error estimate
Inoue, K., Cabella, P., & Komatsu, E. (2008) · doi:10.1103/physrevd.77.123539 · Cited by 17 · cited 1×
“Some dense regression tasks are denoising, interpolation of missing values, or inpainting parts of a map [40].”
BackgroundPires, S., Starck, J., Leonard, A., & Refregier, A. R. (2012) · Chapman & Hall/CRC data mining and knowledge discovery series · doi:10.1201/b11822-19 · Cited by 16 · cited 1×
“These kind of maps can be created using the gravitational lensing technique [see 29, for review].”
MethodReionization Models Classifier using 21cm Map Deep Learning
Hassan, S., Liu, A., Kohn, S., Aguirre, J., Plante, P. L., & Lidz, A. (2017) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921317010833 · Cited by 4
Learning from deep learning: better cosmological parameter inference from weak lensing maps
Ribli, D., Pataki, B., & Csabai, I. (2018) · doi:10.48550/arxiv.1806.05995 · Cited by 3
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“Another trend, parallel to the modeling of structured data, is the use of graph neural networks for relational reasoning [69].”
Background
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Deep learning modelling techniques: Current progress, applications, advantages, and challenges
Ahmed, S. F., Alam, M. S. B., Hassan, M., Rozbu, M. R., Ishtiak, T., Rafa, N., Mofijur, M., Shawkat Ali, A. B. M., & Gandomi, A. H. (2023) · Artificial Intelligence Review · doi:10.1007/s10462-023-10466-8 · Cited by 1,079
General E(2)-Equivariant Steerable CNNs
Weiler, M., & Cesa, G. (2019) · Neural Information Processing Systems · doi:10.48550/arxiv.1911.08251 · Cited by 755
“spherical CNNs [19, 5, 20, 21, 22, 23] or more general models of geometric deep learning [24, 25, 26, 27].”
BackgroundWeatherBench: A Benchmark Data Set for Data‐Driven Weather Forecasting
Rasp, S., Dueben, P. D., Scher, S., Weyn, J. A., Mouatadid, S., & Thuerey, N. (2020) · Journal of Advances in Modeling Earth Systems · doi:10.1029/2020ms002203 · Cited by 663
“A possible solution in the horizontal could be to use spherical convolutions (Cohen et al., 2018; Perraudin et al., 2019; Jiang et al., 2019) or to feed in latitude information to the network.”
BackgroundGauge Equivariant Convolutional Networks and the Icosahedral CNNPreprint
Cohen, T., Weiler, M., Kicanaoglu, B., & Welling, M. (2019) · arXiv (Cornell University) · doi:10.48550/arxiv.1902.04615 · Cited by 197
“Spherical CNNs Besides the general theoretical framework of gauge equivariant convolution, we present in this paper a specific model (the Icosahedral CNN), which can be viewed as a fast and simple alternative to Spherical CNNs (Cohen et al., 2018b; Esteves et al., 2018; Boomsma & Frellsen, 2017; Su & Grauman, 2017; Per…”
MethodInfluentialA General Theory of Equivariant CNNs on Homogeneous SpacesPreprint
Cohen, T., Geiger, M., & Weiler, M. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1811.02017 · Cited by 70
Metadata
- Authors
- Perraudin, N., Defferrard, M., Kacprzak, T., & Sgier, R.
- Affiliations
- Swiss Data Science Center (CH)
- École Polytechnique Fédérale de Lausanne (CH)
- ETH Zurich (CH)
- Corresponding author
- Perraudin, N.
- Venue
- Astronomy and Computing
- Publisher
- Elsevier BV
- Published
- 2019-04
- Volume
- 27
- Pages
- 130-146
- ISSN
- 2213-1337 (ISSN-L)
- OpenAlex
- W2898187790
- Cited by
- 184
- References
- 76
- Citations by year
- 2026: 9 · 2025: 24 · 2024: 22 · 2023: 23 · 2022: 29 · 2021: 33 · 2020: 28 · 2019: 14
- FWCI
- 13.88
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Astronomy and Computing (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion, cc-by-nc-nd)
- arXiv (Cornell University)
- Funders
- Swiss Data Science Center (200021_169130)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Computer Science › Computational Theory and Mathematics › Topological and Geometric Data Analysis
- Physical Sciences › Computer Science › Computer Vision and Pattern Recognition › Advanced Neural Network Applications
- Keywords
- spherical convolutional neural networks, HEALPix, graph convolutional networks, rotation equivariance, spherical maps
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