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Radiometer calibration using machine learning
S A K Leeney1,2,3, H T J Bevins4,5,6, E de Lera Acedo4,5,6
1Astrophysics Group, Cavendish Laboratory, University of Cambridge, J. J. Thomson Avenue, Cambridge, CB3 0HE, UK. sakl2@cam.ac.uk.
Machine learning calibrates radiometers for radio astronomy, improving precision for detecting the faint 21-cm signal. This new framework models complex instrumental effects, overcoming limitations of traditional methods.
Area of Science:
- Radio astronomy
- Cosmology
- Instrumental calibration
Background:
- Radiometers are key radio astronomy instruments, measuring electromagnetic radiation intensity.
- Impedance mismatches in receivers cause signal distortions, challenging traditional calibration like Dicke switching.
- Detecting the faint, high-redshift 21-cm signal is a major cosmological challenge.
Purpose of the Study:
- Introduce and test a novel machine learning (ML) calibration framework for radiometric experiments.
- Achieve the precision necessary for detecting the challenging sky-averaged 21-cm signal.
- Provide an alternative to traditional calibration methods for complex radio astronomical systems.
Main Methods:
- Utilize neural networks trained on known signal sources to model instrumental effects.
- Develop a machine learning-based calibration framework for radiometers.
- Test the framework's performance in achieving required radiometric precision.
Main Results:
- The ML calibration framework demonstrates capability for high-precision radiometric measurements.
- Successfully models and corrects for complex instrumental effects.
- Achieves precision suitable for detecting the faint 21-cm signal.
Conclusions:
- Machine learning offers a powerful approach to calibrate complex radiometric systems.
- The developed ML framework meets the precision requirements for 21-cm signal detection experiments.
- This work advances observational cosmology by enabling new detection capabilities.
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