Constraining the Reionization History using Bayesian Normalizing Flows
@article{Hortua2020ConstrainingTR, title={Constraining the Reionization History using Bayesian Normalizing Flows}, author={H'ector J. Hort'ua and Luigi Malag{\`o} and Riccardo Volpi}, journal={Machine Learning: Science and Technology}, year={2020}, volume={1} }
Upcoming experiments such as Hydrogen Epoch of Reionization Array(HERA) and the Square Kilometre Array (SKA) are intended to measure the 21 cm signal over a wide range of redshifts, representing an incredible opportunity in advancing our understanding about the nature of cosmic reionization. At the same time these kind of experiments will present new challenges in processing the extensive amount of data generated, calling for the development of automated methods capable of precisely estimating…
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References
SHOWING 1-10 OF 41 REFERENCES
Simultaneously constraining the astrophysics of reionisation and the epoch of heating with 21CMMC
- PhysicsProceedings of the International Astronomical Union
- 2017
Abstract We extend our MCMC sampler of 3D EoR simulations, 21CMMC, to perform parameter estimation directly on light-cones of the cosmic 21cm signal. This brings theoretical analysis one step closer…
Constraining the astrophysics and cosmology from 21 cm tomography using deep learning with the SKA
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2020
Future Square Kilometre Array (SKA) surveys are expected to generate huge data sets of 21 cm maps on cosmological scales from the Epoch of Reionization. We assess the viability of exploiting…
Parameters Estimation for the Cosmic Microwave Background with Bayesian Neural Networks
- Computer ScienceArXiv
- 2019
Flipout outperforms all other methods regardless of the architecture used, and provides tighter constraints for the cosmological parameters, and the correct calibration of these networks does not change the behavior for the aleatoric and epistemic uncertainties provided for BNNs when the size of the training dataset changes.
Identifying Reionization Sources from 21cm Maps using Convolutional Neural Networks
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2018
Active Galactic Nuclei (AGN) and star-forming galaxies are leading candidates for being the luminous sources that reionized our Universe. Next-generation 21cm surveys are promising to break…
Parameters Estimation from the 21 cm signal using Variational Inference
- PhysicsArXiv
- 2020
Variational Inference, and in particular Bayesian Neural Networks, are employed as an alternative to MCMC in 21 cm observations to report credible estimations for cosmological and astrophysical parameters and assess the correlations among them.
Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization
- Physics
- 2005
A number of radio interferometers are currently being planned or constructed to observe 21 cm emission from reionization. Not only will such measurements provide a detailed view of that epoch, but,…
21CMMC: an MCMC analysis tool enabling astrophysical parameter studies of the cosmic 21 cm signal
- Physics
- 2015
We introduce 21CMMC: a parallelized, Monte Carlo Markov Chain analysis tool, incorporating the epoch of reionization (EoR) seminumerical simulation 21CMFAST. 21CMMC estimates astrophysical parameter…
Deep learning from 21-cm tomography of the Cosmic Dawn and Reionization
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2019
The 21-cm power spectrum (PS) has been shown to be a powerful discriminant of reionization and cosmic dawn astrophysical parameters. However, the 21-cm tomographic signal is highly non-Gaussian.…
Improving cosmological parameter estimation with the future 21 cm observation from SKA
- PhysicsPhysics Letters B
- 2019
21cmfast: a fast, seminumerical simulation of the high‐redshift 21‐cm signal
- Physics
- 2010
We introduce a powerful semi-numeric modeling tool, 21cmFAST, designed to efficiently simulate the cosmological 21-cm signal. Our code generates 3D realizations of evolved density, ionization,…