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Revealing Hidden Cosmic Flows through the Zone of Avoidance with Deep Learning

  • Authors: Alexandra Dupuy, Donghui Jeong, Sungwook E. Hong, Ho Seong Hwang, Juhan Kim, Hélène M. Courtois

Alexandra Dupuy et al 2026 The Astrophysical Journal 997 .

  • Provider: AAS Journals

Caption: Figure 2.

Input and output quantities for the deep learning algorithm. Each panel corresponds to the same SGX–SGY slice of width −7.5 < SGZ < 7.5 Mpc h−1 and of various quantities. From left to right: (a) mock data from which the input and output quantities have been generated, (b) galaxy number density Ngal, (c) mean radial peculiar velocity Vpec, (d) true dark matter density field, and (e) true gravitational potential field.

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