F. Schmidt
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.
Authors
A. Leauthaud
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
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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