- Raghunathan & Omori 2023; arXiv:2304.09166; Submitted to ApJ.
- Cross-ILC technique:
- For kSZ: Compute cross-spectrum between tSZ-free and CIB-free ILC maps to measure the kSZ power spectrum.
- For CMB lensing: Pass tSZ-free and CIB-free ILC maps in the two legs of lensing quadratic estimator to mitigate both tSZ and CIB-induced lensing biases.
- make_paper_plots.ipynb: Reproduce plots in the paper.
- Fisher formalism:
- s1_get_fisher_matrix.ipynb: Forecasts total SNR of the kSZ power spectrum and also cosmological / reionisation constraints for current and future CMB surveys.
- s2_analyse_fisher_matrix.ipynb: Analyse the results from s1_get_fisher_matrix.ipynb. This notebook will help in making tables and figures.
- get_bandpower_errors.ipynb: Obtain the bandpower errors for different ILC techniques / CMB experiments analytically using Knox formula.
-
estimate_bias_using_fisher.ipynb: Estimate biases in kSZ and cosmological parameters due to unmodelled CIB/tSZ residuals. This used a modifed Fisher formalism based on Amara & Refregier 2007.
- There are also couple of more example notebooks to understand Fisher-based bias estimation in fisher_bias folder.
- example1_bias_in_line_fitting.ipynb - Bias estimation in simple line fitting and a comparison of the result using a lileihood approach.
-
example2_bias_in_cosmo.ipynb - Inject biases as xx
$\sigma$ of cosmological parameters and recover them using the modified Fisher appraoch.
- There are also couple of more example notebooks to understand Fisher-based bias estimation in fisher_bias folder.
- get_radio_residuals.ipynb: Modelling the power spectrum of radio sources and also get the ILCed radio residuals analytically.
-
Data:
-
lagache_2019_ns150_radio.dat: Radio
$dN/dS$ = Lagache et al. 2020 model (arXiv: 1911.09466) used to model radio point source power. - ilc_weights_residuals_agora_fg_model.npy: ILC residuals for multiple ILC combinations and all experiments considered in this work.
-
CAMB: CMB power spectra and derivatives of the power spectra as a function of cosmological parameters:
- Both Planck 2018 and Planck 2015 are available.
- Planck 2018 is the default.
- These are used for Fisher forecasting.
- Both lensed and unlensed versions are available.
- Fiducial: Lensed spectra.
-
lagache_2019_ns150_radio.dat: Radio
-
- ilc_weights_residuals_agora_fg_model.npy - ILC residuals and weights for AGORA foreground model.
-
- fiducial - Results from TTEETE; 3mJy source mask; Total parameters = 14: 6 LCDM + 2 radio parameters + 1 CIB/tSZ + 1 kSZ amplitude + 2 homogeneous kSZ + 2 reionisation kSZ.
-
-
Lensing N0: Results available for standard QE, MH18, and the cross-ILC.
- Simply do:
ls *qewithcmbmv*
orls *mh*
orls *xilc*
to see the files in the linked Lensing N0 folder.
- Simply do:
- Lensing cross-correlations:
-
Lensing N0: Results available for standard QE, MH18, and the cross-ILC.
- Standard python packages: jupyter notebook, numpy, scipy, matplotlib.
- For Fisher bias calculations:
- CAMB.