Epoch of Reionization(EoR) is one of the crucial periods in the history of our Universe. The origin of the very first stars & galaxies formed during this era are unknown mainly due to various observational challenges that prohibit the detection of preferred H1 21-cm signal (hyperfine transition line from the neutral Hydrogen) coming from the EoR. The Fourier-based signal statistics (e.g. 21-cm power spectrum and Bispectrum) thus provide a much-refined way to probe the EoR. One way of characterizing EoR is constraining the reionization parameters using these statistical models via methods like MCMC and Bayesian Inference.

Simulation-based statistical models cast expansive computational overhead while performing the Bayesian Inference. Thus, we used Artificial Neural Networks (ANN)-based emulation models for the Power spectrum and Bispectrum to replace the simulation models. We generated 550 samples of Power spectrum and Bispectrum by varying 3 parameters (Mhmin, Rmfp, Nion) to train the networks. The parameters are minimum mass of the host dark matter halo, mean free path of ionizing photons (i.e. also the relative size of the ionized region) and the ionizing efficiency of the ionizing photons, respectively. We used semi-numarical code ReionYuga to build the data sets for training and testing our ANNs. The documentation of the project can be found here ReadtheDocs. ANN model evaluation of the unseen test-data, The ANN models shows more than 90% accuracy in the predictions.

We assume the situation where the foregrounds, RFIs and other artifacts are completely removed from the signal. The signal thus only contributed by the sample variance and system noise of the observing instrument (SKA1-low in this case). We simulated system noise of SKA1-low correspond to 1000 hours of observation time.

All ANNs' related tasks are done using keras, a python based deep-learning library, For MCMC analysis we used python cosmoHammer, which uses emcee and for plotting and visualization we used matplotlib and chainconsumer.