First measurement of the cross-correlation of CMB lensing and galaxy lensing
- Univ. of California, Berkeley, CA (United States)
- Univ. of Tokyo, Chiba (Japan)
- Argonne National Lab. (ANL), Lemont, IL (United States); Berkeley Center for Cosmological Physics, Berkeley, CA (United States)
- Univ. of California, Berkeley, CA (United States); Berkeley Center for Cosmological Physics, Berkeley, CA (United States)
- Univ. of British Columbia, Vancouver, BC (Canada)
- Univ. of Toronto, Toronto, ON (Canada)
- Univ. of Oxford, Oxford (United Kingdom)
- Univ. Federal do Rio de Janeiro, Rio de Janeiro (Brazil); Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro (Brazil)
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Univ. of Bonn, Bonn (Germany)
- Univ. of British Columbia, Vancouver, BC (Canada); Univ. of Toronto, Toronto, ON (Canada)
- Univ. of Edinburgh, Edinburgh (United Kingdom)
- Ecole Polytechnique Federal de Lausanne (EPFL), Versoix (Switzerland); Aix Marseille Univ., Marseille (France)
- Univ. of Pittsburgh, Pittsburgh, PA (United States)
- Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro (Brazil)
- Univ. of KwaZulu-Natal, Durban (South Africa)
- Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro (Brazil); Univ. College London, London (United Kingdom); Ministry of Education of Brazil (Brazil)
- Cornell Univ., Ithaca, NY (United States)
- Princeton Univ., Princeton, NJ (United States)
- Haverford College, Haverford, PA (United States)
- Stony Brook Univ., Stony Brook, NY (United States)
- Ecole Polytechnique Federale de Lausanne (EPFL), Versoix (Switzerland)
- Univ. of KwaZulu-Natal, Durban (South Africa); Princeton Univ., Princeton, NJ (United States); Univ. of Toronto, Toronto, ON (Canada)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Toronto, Toronto, ON (Canada)
- Univ. of Waterloo, Waterloo, ON (Canada)
- Institut d'Astrophysique de Paris, Paris (France); UPMC Paris, Paris (France)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
Here, 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 ~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.
- Research Organization:
- Argonne National Lab. (ANL), Argonne, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- Grant/Contract Number:
- AC02-06CH11357
- OSTI ID:
- 1363804
- Journal Information:
- Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 91, Issue 6; ISSN 1550-7998
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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