First measurement of the cross-correlation of CMB lensing and galaxy lensing

Nick Hand; Alexie Leauthaud; Sudeep Das; Blake D. Sherwin; Graeme E. Addison; J. Richard Bond; Erminia Calabrese; Aldée Charbonnier; Mark J. Devlin; Joanna Dunkley; Thomas Erben; Amir Hajian; Mark Halpern; Joachim Harnois-Déraps; Catherine Heymans; Hendrik Hildebrandt; Adam D. Hincks; Jean Paul Kneib; Arthur Kosowsky; Martin Makler; Lance Miller; Kavilan Moodley; Bruno Moraes; Michael D. Niemack; Lyman A. Page; Bruce Partridge; Neelima Sehgal; Huanyuan Shan; Jonathan L. Sievers; David N. Spergel; Suzanne T. Staggs; Eric R. Switzer; James E. Taylor; Ludovic Van Waerbeke; Charlotte Welker; Edward J. Wollack

doi:10.1103/PhysRevD.91.062001

First measurement of the cross-correlation of CMB lensing and galaxy lensing

Nick Hand
, Alexie Leauthaud
, Sudeep Das
, Blake D. Sherwin
, Graeme E. Addison
, J. Richard Bond
, Erminia Calabrese
, Aldée Charbonnier
, Mark J. Devlin
, Joanna Dunkley
, Thomas Erben
, Amir Hajian
, Mark Halpern
, Joachim Harnois-Déraps
, Catherine Heymans
, Hendrik Hildebrandt
, Adam D. Hincks
, Jean Paul Kneib
, Arthur Kosowsky
, Martin Makler

Lance Miller, Kavilan Moodley, Bruno Moraes, Michael D. Niemack, Lyman A. Page, Bruce Partridge, Neelima Sehgal, Huanyuan Shan, Jonathan L. Sievers, David N. Spergel, Suzanne T. Staggs, Eric R. Switzer, James E. Taylor, Ludovic Van Waerbeke, Charlotte Welker, Edward J. Wollack

Physics and Astronomy

University of California at Berkeley
The University of Tokyo
Argonne National Laboratory
University of British Columbia
University of Toronto
University of Oxford
Universidade Federal do Rio de Janeiro
Centro Brasileiro de Pesquisas Físicas
University of Pennsylvania
University of Bonn
University of Edinburgh
Swiss Federal Institute of Technology Lausanne
LAM
University of Pittsburgh
University of KwaZulu-Natal
University College London
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior
Cornell University
Princeton University
Haverford College
NASA Goddard Space Flight Center
University of Waterloo
Institut d'Astrophysique de Paris
Sorbonne Université

Research output: Contribution to journal › Article › peer-review

67 Scopus citations

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 4.2σ, 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.

Original language	English
Article number	062001
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	91
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevD.91.062001
State	Published - Mar 2 2015

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10.1103/PhysRevD.91.062001

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Hand, N., Leauthaud, A., Das, S., Sherwin, B. D., Addison, G. E., Bond, J. R., Calabrese, E., Charbonnier, A., Devlin, M. J., Dunkley, J., Erben, T., Hajian, A., Halpern, M., Harnois-Déraps, J., Heymans, C., Hildebrandt, H., Hincks, A. D., Kneib, J. P., Kosowsky, A., ... Wollack, E. J. (2015). First measurement of the cross-correlation of CMB lensing and galaxy lensing. Physical Review D - Particles, Fields, Gravitation and Cosmology, 91(6), Article 062001. https://doi.org/10.1103/PhysRevD.91.062001

@article{ca3f2fb5aa5a4bae8005cb9991732820,

title = "First measurement of the cross-correlation of CMB lensing and galaxy lensing",

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 4.2σ, 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.",

author = "Nick Hand and Alexie Leauthaud and Sudeep Das and Sherwin, \{Blake D.\} and Addison, \{Graeme E.\} and Bond, \{J. Richard\} and Erminia Calabrese and Ald{\'e}e Charbonnier and Devlin, \{Mark J.\} and Joanna Dunkley and Thomas Erben and Amir Hajian and Mark Halpern and Joachim Harnois-D{\'e}raps and Catherine Heymans and Hendrik Hildebrandt and Hincks, \{Adam D.\} and Kneib, \{Jean Paul\} and Arthur Kosowsky and Martin Makler and Lance Miller and Kavilan Moodley and Bruno Moraes and Niemack, \{Michael D.\} and Page, \{Lyman A.\} and Bruce Partridge and Neelima Sehgal and Huanyuan Shan and Sievers, \{Jonathan L.\} and Spergel, \{David N.\} and Staggs, \{Suzanne T.\} and Switzer, \{Eric R.\} and Taylor, \{James E.\} and \{Van Waerbeke\}, Ludovic and Charlotte Welker and Wollack, \{Edward J.\}",

note = "Publisher Copyright: {\textcopyright} 2015 American Physical Society.",

year = "2015",

month = mar,

day = "2",

doi = "10.1103/PhysRevD.91.062001",

language = "English",

volume = "91",

journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",

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Hand, N, Leauthaud, A, Das, S, Sherwin, BD, Addison, GE, Bond, JR, Calabrese, E, Charbonnier, A, Devlin, MJ, Dunkley, J, Erben, T, Hajian, A, Halpern, M, Harnois-Déraps, J, Heymans, C, Hildebrandt, H, Hincks, AD, Kneib, JP, Kosowsky, A, Makler, M, Miller, L, Moodley, K, Moraes, B, Niemack, MD, Page, LA, Partridge, B, Sehgal, N, Shan, H, Sievers, JL, Spergel, DN, Staggs, ST, Switzer, ER, Taylor, JE, Van Waerbeke, L, Welker, C & Wollack, EJ 2015, 'First measurement of the cross-correlation of CMB lensing and galaxy lensing', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 91, no. 6, 062001. https://doi.org/10.1103/PhysRevD.91.062001

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.

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.

UR - https://www.scopus.com/pages/publications/84924388758

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 -

First measurement of the cross-correlation of CMB lensing and galaxy lensing

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