English

Shear measurement bias II: a fast machine learning calibration method

Cosmology and Nongalactic Astrophysics 2020-11-25 v2 Instrumentation and Methods for Astrophysics

Abstract

We present a new shear calibration method based on machine learning. The method estimates the individual shear responses of the objects from the combination of several measured properties on the images using supervised learning. The supervised learning uses the true individual shear responses obtained from copies of the image simulations with different shear values. On simulated GREAT3data, we obtain a residual bias after the calibration compatible with 0 and beyond Euclid requirements for a signal-to-noise ratio > 20 within ~15 CPU hours of training using only ~10^5 objects. This efficient machine-learning approach can use a smaller data set because the method avoids the contribution from shape noise. The low dimensionality of the input data also leads to simple neural network architectures. We compare it to the recently described method Metacalibration, which shows similar performances. The different methods and systematics suggest that the two methods are very good complementary methods. Our method can therefore be applied without much effort to any survey such as Euclid or the Vera C. Rubin Observatory, with fewer than a million images to simulate to learn the calibration function.

Keywords

Cite

@article{arxiv.2006.07011,
  title  = {Shear measurement bias II: a fast machine learning calibration method},
  author = {Arnau Pujol and Jerome Bobin and Florent Sureau and Axel Guinot and Martin Kilbinger},
  journal= {arXiv preprint arXiv:2006.07011},
  year   = {2020}
}

Comments

16 pages, 1 table, 13 figures

R2 v1 2026-06-23T16:16:02.181Z