A fast method of reionization parameter space exploration using GPR trained SCRIPT
Author:
Affiliation:
1. National Centre for Radio Astrophysics (NCRA), TIFR , Pune University Campus, Post Bag 3, Pune 411 007 , India
2. Inter University Centre for Astronomy and Astrophysics (IUCAA) , Pune University Campus, Post Bag 4, Pune 411 007 , India
Abstract
Funder
Department of Atomic Energy
ICTP
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad2984/51824369/stad2984.pdf
Reference145 articles.
1. HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization
2. First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
3. NEW CONSTRAINTS ON THE FAINT END OF THE UV LUMINOSITY FUNCTION ATz∼ 7-8 USING THE GRAVITATIONAL LENSING OF THE HUBBLE FRONTIER FIELDS CLUSTER A2744
4. The extreme faint end of the UV luminosity function at z ∼ 6 through gravitational telescopes: a comprehensive assessment of strong lensing uncertainties
5. An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5
Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. A GPR-based emulator for semi-numerical reionization code SCRIPT: parameter inference from 21 cm data;Journal of Cosmology and Astroparticle Physics;2024-03-01
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