TY - JOUR
T1 - First measurement of the cross-correlation of CMB lensing and galaxy lensing
AU - Hand, Nick
AU - Leauthaud, Alexie
AU - Das, Sudeep
AU - Sherwin, Blake D.
AU - Addison, Graeme E.
AU - Bond, J. Richard
AU - Calabrese, Erminia
AU - Charbonnier, Aldée
AU - Devlin, Mark J.
AU - Dunkley, Joanna
AU - Erben, Thomas
AU - Hajian, Amir
AU - Halpern, Mark
AU - Harnois-Déraps, Joachim
AU - Heymans, Catherine
AU - Hildebrandt, Hendrik
AU - Hincks, Adam D.
AU - Kneib, Jean Paul
AU - Kosowsky, Arthur
AU - Makler, Martin
AU - Miller, Lance
AU - Moodley, Kavilan
AU - Moraes, Bruno
AU - Niemack, Michael D.
AU - Page, Lyman A.
AU - Partridge, Bruce
AU - Sehgal, Neelima
AU - Shan, Huanyuan
AU - Sievers, Jonathan L.
AU - Spergel, David N.
AU - Staggs, Suzanne T.
AU - Switzer, Eric R.
AU - Taylor, James E.
AU - Van Waerbeke, Ludovic
AU - Welker, Charlotte
AU - Wollack, Edward J.
N1 - Publisher Copyright:
© 2015 American Physical Society.
PY - 2015/3/2
Y1 - 2015/3/2
N2 - 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 4.2σ, which corresponds to a 12% constraint on the amplitude of density fluctuations at redshifts ∼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.
AB - 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 4.2σ, which corresponds to a 12% constraint on the amplitude of density fluctuations at redshifts ∼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.
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U2 - 10.1103/PhysRevD.91.062001
DO - 10.1103/PhysRevD.91.062001
M3 - Article
AN - SCOPUS:84924388758
SN - 1550-7998
VL - 91
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 6
M1 - 062001
ER -