CMB lensing tomography with the DES Science Verification galaxies
International audience 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...
Published in: | Monthly Notices of the Royal Astronomical Society |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , |
Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2016
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Subjects: | |
Online Access: | https://hal.science/hal-03645201 https://hal.science/hal-03645201/document https://hal.science/hal-03645201/file/stv2678.pdf https://doi.org/10.1093/mnras/stv2678 |
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ftccsdartic:oai:HAL:hal-03645201v1 |
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Open Polar |
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Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
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language |
English |
topic |
cosmic background radiation gravitational lensing: weak large-scale structure of Universe [SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
spellingShingle |
cosmic background radiation gravitational lensing: weak large-scale structure of Universe [SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Giannantonio, T. Fosalba, P. Cawthon, R. Omori, Y. Crocce, M. Elsner, F. Leistedt, B. Dodelson, S. Benoit-Lévy, A. Gaztañaga, 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. Carnero Rosell, A. Carrasco Kind, M. 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 |
cosmic background radiation gravitational lensing: weak large-scale structure of Universe [SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
description |
International audience 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 phot < 1.2, a cross-correlation signal is detected at 6σ and 4σ with SPT and Planck , respectively. We then divide the DES galaxies into five photometric redshift bins, finding significant (>2σ) 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 ± 0.16 times as large as predicted in the Λ cold dark matter Planck cosmology, a 1.7σ deviation. |
author2 |
Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) |
format |
Article in Journal/Newspaper |
author |
Giannantonio, T. Fosalba, P. Cawthon, R. Omori, Y. Crocce, M. Elsner, F. Leistedt, B. Dodelson, S. Benoit-Lévy, A. Gaztañaga, 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. Carnero Rosell, A. Carrasco Kind, M. 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-Lévy, A. Gaztañaga, 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. Carnero Rosell, A. Carrasco Kind, M. 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 |
HAL CCSD |
publishDate |
2016 |
url |
https://hal.science/hal-03645201 https://hal.science/hal-03645201/document https://hal.science/hal-03645201/file/stv2678.pdf https://doi.org/10.1093/mnras/stv2678 |
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South pole |
genre_facet |
South pole |
op_source |
ISSN: 0035-8711 EISSN: 1365-2966 Monthly Notices of the Royal Astronomical Society https://hal.science/hal-03645201 Monthly Notices of the Royal Astronomical Society, 2016, 456, pp.3213-3244. ⟨10.1093/mnras/stv2678⟩ |
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info:eu-repo/semantics/OpenAccess |
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https://doi.org/10.1093/mnras/stv2678 |
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Monthly Notices of the Royal Astronomical Society |
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456 |
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3 |
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3213 |
op_container_end_page |
3244 |
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ftccsdartic:oai:HAL:hal-03645201v1 2023-11-05T03:45:06+01:00 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-Lévy, A. Gaztañaga, 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. Carnero Rosell, A. Carrasco Kind, M. 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. Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) 2016 https://hal.science/hal-03645201 https://hal.science/hal-03645201/document https://hal.science/hal-03645201/file/stv2678.pdf https://doi.org/10.1093/mnras/stv2678 en eng HAL CCSD Oxford University Press (OUP): Policy P - Oxford Open Option A info:eu-repo/semantics/altIdentifier/arxiv/1507.05551 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stv2678 hal-03645201 https://hal.science/hal-03645201 https://hal.science/hal-03645201/document https://hal.science/hal-03645201/file/stv2678.pdf ARXIV: 1507.05551 BIBCODE: 2016MNRAS.456.3213G doi:10.1093/mnras/stv2678 info:eu-repo/semantics/OpenAccess ISSN: 0035-8711 EISSN: 1365-2966 Monthly Notices of the Royal Astronomical Society https://hal.science/hal-03645201 Monthly Notices of the Royal Astronomical Society, 2016, 456, pp.3213-3244. ⟨10.1093/mnras/stv2678⟩ cosmic background radiation gravitational lensing: weak large-scale structure of Universe [SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2016 ftccsdartic https://doi.org/10.1093/mnras/stv2678 2023-10-07T23:03:47Z International audience 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 phot < 1.2, a cross-correlation signal is detected at 6σ and 4σ with SPT and Planck , respectively. We then divide the DES galaxies into five photometric redshift bins, finding significant (>2σ) 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 ± 0.16 times as large as predicted in the Λ cold dark matter Planck cosmology, a 1.7σ deviation. Article in Journal/Newspaper South pole Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Monthly Notices of the Royal Astronomical Society 456 3 3213 3244 |