Abstract

We consider the possible gain in the measurement of lensing shear from imaging datain multiple filters. Galaxy shapes may differ significantly across filters, so thatthe same galaxy offers multiple samples of the shear. At the other extreme, ifgalaxy shapes are identical in different filters, one can combine them to improvethe signal-to-noise ratio and thus increase the effective number density of faint,high redshift galaxies. We use the GOODS dataset to test these scenarios bycalculating the covariance matrix of galaxy ellipticities in four visual filters(B,V,i,z). We find that galaxy shapes are highly correlated, and estimate the gain in galaxy numberdensity by combining their shapes.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.