CMB lensing tomography with the DES Science Verification galaxies
We measure the cross-correlation between the galaxy density in the Dark Energy Survey (DES) Science Verification data and the lensing of the cosmic microwave background (CMB) as reconstructed with the Planck satellite and the South Pole Telescope (SPT). When using the DES main galaxy sample over the...
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ftdatacite:10.48550/arxiv.1507.05551 2023-05-15T18:22:43+02:00 CMB lensing tomography with the DES Science Verification galaxies Giannantonio, T. Fosalba, P. Cawthon, R. Omori, Y. Crocce, M. Elsner, F. Leistedt, B. Dodelson, S. Benoit-Levy, A. Gaztanaga, E. Holder, G. Peiris, H. V. Percival, W. J. Kirk, D. Bauer, A. H. Benson, B. A. Bernstein, G. M. Carretero, J. Crawford, T. M. Crittenden, R. Huterer, D. Jain, B. Krause, E. Reichardt, C. L. Ross, A. J. Simard, G. Soergel, B. Stark, A. Story, K. T. Vieira, J. D. Weller, J. Abbott, T. Abdalla, F. B. Allam, S. Armstrong, R. Banerji, M. Bernstein, R. A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D. L. Capozzi, D. Carlstrom, J. E. Rosell, A. Carnero Kind, M. Carrasco Castander, F. J. Chang, C. L. Cunha, C. E. da Costa, L. N. D'Andrea, C. B. DePoy, D. L. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Eifler, T. F. Evrard, A. E. Neto, A. Fausti Fernandez, E. Finley, D. A. Flaugher, B. Frieman, J. Gerdes, D. Gruen, D. Gruendl, R. A. Gutierrez, G. Holzapfel, W. L. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Li, T. S. Lima, M. March, M. Marshall, J. L. Martini, P. Melchior, P. Miquel, R. Mohr, J. J. Nichol, R. C. Nord, B. Ogando, R. Plazas, A. A. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Saliwanchik, B. R. Sanchez, E. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarle, G. Thaler, J. Thomas, D. Vikram, V. Walker, A. R. Wechsler, R. H. Zuntz, J. 2015 https://dx.doi.org/10.48550/arxiv.1507.05551 https://arxiv.org/abs/1507.05551 unknown arXiv https://dx.doi.org/10.1093/mnras/stv2678 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences article-journal Article ScholarlyArticle Text 2015 ftdatacite https://doi.org/10.48550/arxiv.1507.05551 https://doi.org/10.1093/mnras/stv2678 2022-04-01T12:12:37Z We measure the cross-correlation between the galaxy density in the Dark Energy Survey (DES) Science Verification data and the lensing of the cosmic microwave background (CMB) as reconstructed with the Planck satellite and the South Pole Telescope (SPT). When using the DES main galaxy sample over the full redshift range $0.2 < z < 1.2$, a cross-correlation signal is detected at $6 σ$ and $4σ$ with SPT and Planck respectively. We then divide the DES galaxies into five photometric redshift bins, finding significant ($>$$2 σ$) detections in all bins. Comparing to the fiducial Planck cosmology, we find the redshift evolution of the signal matches expectations, although the amplitude is consistently lower than predicted across redshift bins. We test for possible systematics that could affect our result and find no evidence for significant contamination. Finally, we demonstrate how these measurements can be used to constrain the growth of structure across cosmic time. We find the data are fit by a model in which the amplitude of structure in the $z<1.2$ universe is $0.73 \pm 0.16$ times as large as predicted in the LCDM Planck cosmology, a $1.7σ$ deviation. : 32 pages, 29 figures, minor modifications to match version published by MNRAS Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Giannantonio, T. Fosalba, P. Cawthon, R. Omori, Y. Crocce, M. Elsner, F. Leistedt, B. Dodelson, S. Benoit-Levy, A. Gaztanaga, E. Holder, G. Peiris, H. V. Percival, W. J. Kirk, D. Bauer, A. H. Benson, B. A. Bernstein, G. M. Carretero, J. Crawford, T. M. Crittenden, R. Huterer, D. Jain, B. Krause, E. Reichardt, C. L. Ross, A. J. Simard, G. Soergel, B. Stark, A. Story, K. T. Vieira, J. D. Weller, J. Abbott, T. Abdalla, F. B. Allam, S. Armstrong, R. Banerji, M. Bernstein, R. A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D. L. Capozzi, D. Carlstrom, J. E. Rosell, A. Carnero Kind, M. Carrasco Castander, F. J. Chang, C. L. Cunha, C. E. da Costa, L. N. D'Andrea, C. B. DePoy, D. L. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Eifler, T. F. Evrard, A. E. Neto, A. Fausti Fernandez, E. Finley, D. A. Flaugher, B. Frieman, J. Gerdes, D. Gruen, D. Gruendl, R. A. Gutierrez, G. Holzapfel, W. L. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Li, T. S. Lima, M. March, M. Marshall, J. L. Martini, P. Melchior, P. Miquel, R. Mohr, J. J. Nichol, R. C. Nord, B. Ogando, R. Plazas, A. A. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Saliwanchik, B. R. Sanchez, E. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarle, G. Thaler, J. Thomas, D. Vikram, V. Walker, A. R. Wechsler, R. H. Zuntz, J. CMB lensing tomography with the DES Science Verification galaxies |
topic_facet |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
We measure the cross-correlation between the galaxy density in the Dark Energy Survey (DES) Science Verification data and the lensing of the cosmic microwave background (CMB) as reconstructed with the Planck satellite and the South Pole Telescope (SPT). When using the DES main galaxy sample over the full redshift range $0.2 < z < 1.2$, a cross-correlation signal is detected at $6 σ$ and $4σ$ with SPT and Planck respectively. We then divide the DES galaxies into five photometric redshift bins, finding significant ($>$$2 σ$) detections in all bins. Comparing to the fiducial Planck cosmology, we find the redshift evolution of the signal matches expectations, although the amplitude is consistently lower than predicted across redshift bins. We test for possible systematics that could affect our result and find no evidence for significant contamination. Finally, we demonstrate how these measurements can be used to constrain the growth of structure across cosmic time. We find the data are fit by a model in which the amplitude of structure in the $z<1.2$ universe is $0.73 \pm 0.16$ times as large as predicted in the LCDM Planck cosmology, a $1.7σ$ deviation. : 32 pages, 29 figures, minor modifications to match version published by MNRAS |
format |
Text |
author |
Giannantonio, T. Fosalba, P. Cawthon, R. Omori, Y. Crocce, M. Elsner, F. Leistedt, B. Dodelson, S. Benoit-Levy, A. Gaztanaga, E. Holder, G. Peiris, H. V. Percival, W. J. Kirk, D. Bauer, A. H. Benson, B. A. Bernstein, G. M. Carretero, J. Crawford, T. M. Crittenden, R. Huterer, D. Jain, B. Krause, E. Reichardt, C. L. Ross, A. J. Simard, G. Soergel, B. Stark, A. Story, K. T. Vieira, J. D. Weller, J. Abbott, T. Abdalla, F. B. Allam, S. Armstrong, R. Banerji, M. Bernstein, R. A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D. L. Capozzi, D. Carlstrom, J. E. Rosell, A. Carnero Kind, M. Carrasco Castander, F. J. Chang, C. L. Cunha, C. E. da Costa, L. N. D'Andrea, C. B. DePoy, D. L. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Eifler, T. F. Evrard, A. E. Neto, A. Fausti Fernandez, E. Finley, D. A. Flaugher, B. Frieman, J. Gerdes, D. Gruen, D. Gruendl, R. A. Gutierrez, G. Holzapfel, W. L. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Li, T. S. Lima, M. March, M. Marshall, J. L. Martini, P. Melchior, P. Miquel, R. Mohr, J. J. Nichol, R. C. Nord, B. Ogando, R. Plazas, A. A. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Saliwanchik, B. R. Sanchez, E. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarle, G. Thaler, J. Thomas, D. Vikram, V. Walker, A. R. Wechsler, R. H. Zuntz, J. |
author_facet |
Giannantonio, T. Fosalba, P. Cawthon, R. Omori, Y. Crocce, M. Elsner, F. Leistedt, B. Dodelson, S. Benoit-Levy, A. Gaztanaga, E. Holder, G. Peiris, H. V. Percival, W. J. Kirk, D. Bauer, A. H. Benson, B. A. Bernstein, G. M. Carretero, J. Crawford, T. M. Crittenden, R. Huterer, D. Jain, B. Krause, E. Reichardt, C. L. Ross, A. J. Simard, G. Soergel, B. Stark, A. Story, K. T. Vieira, J. D. Weller, J. Abbott, T. Abdalla, F. B. Allam, S. Armstrong, R. Banerji, M. Bernstein, R. A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D. L. Capozzi, D. Carlstrom, J. E. Rosell, A. Carnero Kind, M. Carrasco Castander, F. J. Chang, C. L. Cunha, C. E. da Costa, L. N. D'Andrea, C. B. DePoy, D. L. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Eifler, T. F. Evrard, A. E. Neto, A. Fausti Fernandez, E. Finley, D. A. Flaugher, B. Frieman, J. Gerdes, D. Gruen, D. Gruendl, R. A. Gutierrez, G. Holzapfel, W. L. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Li, T. S. Lima, M. March, M. Marshall, J. L. Martini, P. Melchior, P. Miquel, R. Mohr, J. J. Nichol, R. C. Nord, B. Ogando, R. Plazas, A. A. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Saliwanchik, B. R. Sanchez, E. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarle, G. Thaler, J. Thomas, D. Vikram, V. Walker, A. R. Wechsler, R. H. Zuntz, J. |
author_sort |
Giannantonio, T. |
title |
CMB lensing tomography with the DES Science Verification galaxies |
title_short |
CMB lensing tomography with the DES Science Verification galaxies |
title_full |
CMB lensing tomography with the DES Science Verification galaxies |
title_fullStr |
CMB lensing tomography with the DES Science Verification galaxies |
title_full_unstemmed |
CMB lensing tomography with the DES Science Verification galaxies |
title_sort |
cmb lensing tomography with the des science verification galaxies |
publisher |
arXiv |
publishDate |
2015 |
url |
https://dx.doi.org/10.48550/arxiv.1507.05551 https://arxiv.org/abs/1507.05551 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1093/mnras/stv2678 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1507.05551 https://doi.org/10.1093/mnras/stv2678 |
_version_ |
1766202133143617536 |