Showing 1–20 of 44 results
/ Date/ Name
Jan 19, 2018Reionization Models Classifier using 21cm Map Deep LearningSep 13, 2024Towards Implementation of the Pressure-Regulated, Feedback-Modulated Model of Star Formation in Cosmological Simulations: Methods and Application to TNGNov 1, 2023HIDM: Emulating Large Scale HI Maps using Score-based Diffusion ModelsSep 8, 2021Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?Oct 6, 2021HIFlow: Generating Diverse HI Maps and Inferring Cosmology while Marginalizing over Astrophysics using Normalizing FlowsJul 17, 2019Constraining the astrophysics and cosmology from 21cm tomography using deep learning with the SKANov 14, 2025Towards Mitigating Systematics in Large-Scale Surveys via Few-Shot Optimal Transport-Based Feature AlignmentJul 9, 2018Identifying Reionization Sources from 21cm Maps using Convolutional Neural NetworksDec 17, 2016Epoch of Reionisation 21cm Forecasting From MCMC-Constrained Semi-Numerical ModelsMar 10, 2020Constraining the reionization history using deep learning from 21cm tomography with the Square Kilometre ArraySep 30, 2020Can galaxy evolution mimic cosmic reionization?Oct 14, 2015Simulating the 21-cm signal from reionisation including non-linear ionisations and inhomogeneous recombinationsMay 4, 2023JWST constraints on the UV luminosity density at cosmic dawn: implications for 21-cm cosmologyOct 16, 2019Testing Galaxy Formation Simulations with Damped Lyman-$α$ Abundance and Metallicity EvolutionMay 15, 2017Constraining the contribution of active galactic nuclei to reionisationNov 29, 2023Towards out-of-distribution generalization in large-scale astronomical surveys: robust networks learn similar representationsNov 23, 2022HIGlow: Conditional Normalizing Flows for High-Fidelity HI Map ModelingJul 13, 2023A Hierarchy of Normalizing Flows for Modelling the Galaxy-Halo RelationshipSep 28, 2022Bridging the Gap between Cosmic Dawn and Reionization favors Faint Galaxies-dominated ModelsMay 29, 2024Metallicity Dependence of Pressure-Regulated Feedback-Modulated Star Formation in the TIGRESS-NCR Simulation Suite