The impact of correlated noise on galaxy shape estimation for weak lensing
The robust estimation of the tiny distortions (shears) of galaxy shapes caused by weak gravitational lensing in the presence of much larger shape distortions due to the point spread function (PSF) has been widely investigated. One major problem is that most galaxy shape measurement methods are subje...
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Published in | Monthly notices of the Royal Astronomical Society Vol. 457; no. 4; pp. 3522 - 3534 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
London
Oxford University Press
21.04.2016
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Subjects | |
Online Access | Get full text |
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