Abstract
We measure the cross-correlation of cosmic microwave background (CMB) lensing convergence maps derived from Atacama Cosmology Telescope data with galaxy lensing convergence maps as measured by the Canada-France-Hawaii Telescope Stripe 82 Survey. The CMB-galaxy lensing cross power spectrum is measured for the first time with a significance of 4.2 sigma, which corresponds to a 12% constraint on the amplitude of density fluctuations at redshifts similar to 0.9. With upcoming improved lensing data, this novel type of measurement will become a powerful cosmological probe, providing a precise measurement of the mass distribution at intermediate redshifts and serving as a calibrator for systematic biases in weak lensing measurements.
Original language | English |
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Article number | 062001 |
Number of pages | 11 |
Journal | Physical Review D |
Volume | 91 |
Issue number | 6 |
DOIs | |
Publication status | Published - 2 Mar 2015 |
Keywords
- ATACAMA COSMOLOGY TELESCOPE
- SOUTH-POLE TELESCOPE
- POWER SPECTRUM
- COSMIC SHEAR
- CFHTLS-WIDE
- WEAK
- MODEL
- MATTER
- BIAS