http://arxiv.org/abs/1809.04599
We study the effect of diffuse intra-cluster light on the critical surface mass density estimated from photometric redshifts of lensing source galaxies, and the resulting bias in a weak lensing measurement of galaxy cluster mass. Under conservative assumptions, we find the bias to be negligible for imaging surveys like the Dark Energy Survey (DES) with a recommended scale cut of >=200 kpc distance from cluster centers. For significantly deeper source catalogs from present and future surveys like the Large Synoptic Survey Telescope (LSST) program, more conservative scale and source magnitude cuts or a correction of the effect may be necessary to achieve per-cent level lensing measurement accuracy, especially at the massive end of the cluster population.
D. Gruen, Y. Zhang, A. Palmese, et. al.
Fri, 14 Sep 18
23/65
Comments: 11 pages, 4 figures, submitted to MNRAS
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