Diagnosing multiplicative error by lensing magnification of type Ia supernovae

TL;DR

This paper proposes a novel method using lensing magnification of type Ia supernovae to diagnose and calibrate multiplicative errors in weak lensing measurements, achieving sub-percent accuracy.

Contribution

It introduces two new methods leveraging cross correlations between supernovae lensing magnification and cosmic shear to constrain multiplicative errors independently of cosmic variance.

Findings

Can detect multiplicative errors of ~0.5% with ~1 million SNe Ia

Methods can calibrate larger errors to 0.5%

Potential to diagnose and calibrate galaxy intrinsic alignment

Abstract

Weak lensing causes spatially coherent fluctuations in flux of type Ia supernovae (SNe Ia). This lensing magnification allows for weak lensing measurement independent of cosmic shear. It is free of shape measurement errors associated with cosmic shear and can therefore be used to diagnose and calibrate multiplicative error. Although this lensing magnification is difficult to measure accurately in auto correlation, its cross correlation with cosmic shear and galaxy distribution in overlapping area can be measured to significantly higher accuracy. Therefore these cross correlations can put useful constraint on multiplicative error, and the obtained constraint is free of cosmic variance in weak lensing field. We present two methods implementing this idea and estimate their performances. We find that, with $\sim 1$ million SNe Ia that can be achieved by the proposed D2k survey with the LSST telescope (Zhan et al. 2008), multiplicative error of $\sim 0.5\%$ for source galaxies at $z_s\sim 1$ can be detected and larger multiplicative error can be corrected to the level of $0.5\%$. It is therefore a promising approach to control the multiplicative to the sub-percent level required for stage IV projects. The combination of the two methods even has the potential to diagnose and calibrate galaxy intrinsic alignment, which is another major systematic error in cosmic shear cosmology.