supported by the National Key Basic Research and Development Program of China(No.2018YFA0404504);the National Natural Science Foundation of China(Grant Nos.11773048,11621303 and 11890691);the science research grants from the China Manned Space Project(No.CMS-CSST-2021B01);the“111”Project of the Ministry of Education(Grant No.B20019)。
Measuring weak lensing cosmic magnification signal is very challenging due to the overwhelming intrinsic clustering in the observed galaxy distribution.In this paper,we modify the Internal Linear Combination(ILC)metho...
partly supported by the National Key Basic Research and Development Program of China(No.2018YFA0404501 to SM);the National Natural Science Foundation of China(Grant Nos.11821303 and 11761131004 to SM)
Strong lensing is one of the most spectacular views in the universe.Many cosmological applications have been proposed,but the number of such lensing systems is still limited.In this work,we applied an improved version...
supported in part by the National Natural Science Foundation of China (Grant Nos. 10373001,10533010 and 10773001);the National Basic Research Program of China (973 program,No. 2007CB815401);Huan-Yuan Shan is very grateful for the hospitality of CPPM
Taking into account the noise from intrinsic ellipticities of source galaxies, we study the efficiency and completeness of halo detections from weak lensing convergence maps. Particularly, with numerical simulations, ...
supported by the National Natural Science Foundation of China (Grant 11073023);the National Basic Research Program of China (973 Program;Grant 2009CB24901);the National Science Foundation of the United States (Grant AST0908370)
Standard cosmology has many successes on large scales, but faces some fundamental difficulties on small, galactic scales. One such difficulty is the cusp/core problem. High resolution observations of the rotation curv...