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A detection of weak-lensing magnification using galaxy sizes and magnitudes

Schmidt, F.; Leauthaud, A.; Massey, R.; Rhodes, J.; George, M.R.; Koekemoer, A.M.; Finoguenov, A.; Tanaka, M.

A detection of weak-lensing magnification using galaxy sizes and magnitudes Thumbnail


Authors

F. Schmidt

A. Leauthaud

J. Rhodes

M.R. George

A.M. Koekemoer

A. Finoguenov

M. Tanaka



Abstract

Weak lensing is commonly measured using shear through galaxy ellipticities or using the effect of magnification bias on galaxy number densities. Here, we report on the first detection of weak-lensing magnification with a new, independent technique using the distribution of galaxy sizes and magnitudes. These data come for free in galaxy surveys designed for measuring shear. We present the magnification estimator and apply it to an X-ray-selected sample of galaxy groups in the COSMOS Hubble Space Telescope survey. The measurement of the projected surface density Σ(r) is consistent with the shear measurements within the uncertainties and has roughly 40% of the signal to noise of the latter. We discuss systematic issues and challenges to realizing the potential of this new probe of weak lensing.

Citation

Schmidt, F., Leauthaud, A., Massey, R., Rhodes, J., George, M., Koekemoer, A., …Tanaka, M. (2012). A detection of weak-lensing magnification using galaxy sizes and magnitudes. Astrophysical Journal Letters, 744(2), Article L22. https://doi.org/10.1088/2041-8205/744/2/l22

Journal Article Type Article
Publication Date Jan 10, 2012
Deposit Date Jan 31, 2012
Publicly Available Date Feb 12, 2015
Journal Astrophysical Journal Letters
Print ISSN 2041-8205
Electronic ISSN 2041-8213
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 744
Issue 2
Article Number L22
DOI https://doi.org/10.1088/2041-8205/744/2/l22
Keywords Dark matter, Gravitational lensing: weak, Large-scale structure of universe.

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Copyright Statement
© 2011. The American Astronomical Society. All rights reserved.





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