Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-21T13:12:23.756Z Has data issue: false hasContentIssue false

Analysing 21cm signal with artificial neural network

Published online by Cambridge University Press:  08 May 2018

Hayato Shimabukuro
Affiliation:
Sorbonne Universités, UPMC, LERMA, Observatoire de Paris, PSL research university, CNRS, F-75014, Paris, France email: [email protected]
Benoit Semelin
Affiliation:
Sorbonne Universités, UPMC, LERMA, Observatoire de Paris, PSL research university, CNRS, F-75014, Paris, France email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The 21cm signal at epoch of reionization (EoR) should be observed within next decade. We expect that cosmic 21cm signal at the EoR provides us both cosmological and astrophysical information. In order to extract fruitful information from observation data, we need to develop inversion method. For such a method, we introduce artificial neural network (ANN) which is one of the machine learning techniques. We apply the ANN to inversion problem to constrain astrophysical parameters from 21cm power spectrum. We train the architecture of the neural network with 70 training datasets and apply it to 54 test datasets with different value of parameters. We find that the quality of the parameter reconstruction depends on the sensitivity of the power spectrum to the different parameter sets at a given redshift and also find that the accuracy of reconstruction is improved by increasing the number of given redshifts. We conclude that the ANN is viable inversion method whose main strength is that they require a sparse extrapolation of the parameter space and thus should be usable with full simulation.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Ball, N. M. & Brunner, R. J., 2010, International Journal of Modern Physics D, 19, 1049CrossRefGoogle Scholar
Bloom, J. S. & Richards, J. W. 2012, Advances in Machine Learning and Data Mining for Astronomy, 89Google Scholar
Greig, B. & Mesinger, A., 2015, MNRAS, 449, 4246CrossRefGoogle Scholar
Kubota, K., Yoshiura, S., Shimabukuro, H., & Takahashi, K., 2016, PASJ, 68, 61CrossRefGoogle Scholar
Shimabukuro, H., Yoshiura, S., Takahashi, K., Yokoyama, S., & Ichiki, K., 2017, MNRAS, 468, 1542CrossRefGoogle Scholar
Shimabukuro, H. & Semelin, B., 2017, MNRAS, 468, 3869CrossRefGoogle Scholar
Mesinger, A., Furlanetto, S., & Cen, R., 2011, MNRAS, 411, 955CrossRefGoogle Scholar