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unWISE tomography of Planck CMB lensing
CMB lensing tomography, or the cross-correlation between CMB lensing maps and large-scale structure tracers over a well-defined redshift range, has the potential to map the amplitude and growth of structure over cosmic time, provide some of the most stringent tests of gravity, and break important de...
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Published in: | Journal of cosmology and astroparticle physics 2020-05, Vol.2020 (5), p.47-47 |
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container_end_page | 47 |
container_issue | 5 |
container_start_page | 47 |
container_title | Journal of cosmology and astroparticle physics |
container_volume | 2020 |
creator | Krolewski, Alex Ferraro, Simone Schlafly, Edward F. White, Martin |
description | CMB lensing tomography, or the cross-correlation between CMB lensing maps and large-scale structure tracers over a well-defined redshift range, has the potential to map the amplitude and growth of structure over cosmic time, provide some of the most stringent tests of gravity, and break important degeneracies between cosmological parameters. In this work, we use the unWISE galaxy catalog to provide three samples at median redshifts z∼0.6,1.1 and 1.5, fully spanning the Dark Energy dominated era, together with the most recent Planck CMB lensing maps. We obtain a combined cross-correlation significance S/N=79.3 over the range of scales 100 |
doi_str_mv | 10.1088/1475-7516/2020/05/047 |
format | article |
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subjects | Astronomical models ASTRONOMY AND ASTROPHYSICS Balances (scales) CMB cosmological parameters from LSS Cross correlation Dark energy Galaxies galaxy clustering Large scale structure of the universe Parameter uncertainty power spectrum Quasars Red shift Tomography Tracers |
title | unWISE tomography of Planck CMB lensing |
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