A Python package for blind component separation of microwave sky maps.
Project description
BROOM: Blind Reconstruction Of signals from Observations in the Microwaves
BROOM is a Python package for blind component separation and Cosmic Microwave Background (CMB) data analysis.
📦 Installation
You can install the base package using:
pip install cmbroom
This installs the core functionality.
If you plan to use the few functions that depend on pymaster, you must install it separately (version >=2.4).
🔧 To include pymaster automatically:
You can install cmbroom along with its optional pymaster dependency by running:
pip install cmbroom[pymaster]
However, pymaster requires some additional system libraries to be installed before running the above command.
✅ On Ubuntu/Debian:
sudo apt update
sudo apt install build-essential python3-dev libfftw3-dev libcfitsio-dev libgsl-dev
✅ On macOS (using Homebrew):
brew install fftw cfitsio gsl
Documentation
A detailed introduction to the parameters and simulation pipeline is available in:
- tutorials/tutorial_satellite.ipynb
- configs/config_demo.yaml — Example configuration file
Component separation methods are covered in:
Power spectrum estimation is demonstrated in:
For partial-sky, ground-based experiment analysis, see:
🔗 Full online documentation:
👉 https://alecarones.github.io/broom/
References
Paper on broom package is in preparation.
If you use the following methodologies please cite the corresponding papers:
- ILC or NILC: Bennett et al., 2003, Delabrouille et al., 2009
- cMILC: Remazeilles et al., 2021, Carones et al., 2024
- MC-ILC or MC-NILC: Carones et al., 2023
- PILC: Fernández-Cobos et al., 2016
- cPILC: Adak, 2021
- GILC, GNILC, GPILC: Remazeilles et al., 2011, Planck Collaboration, 2016
- foreground diagnostic: Carones et al., 2024
- power spectrum computation: Gorski et al., 2005, Zonca et al., 2019, Alonso et al., 2019
📦 Dependencies
This package relies on several scientific Python libraries:
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