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Title: Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope + Planck

Abstract

We analyze the cross-correlation between redMaGiC galaxies selected from the Dark Energy Survey (DES) year 1 data and gravitational lensing of the cosmic microwave background (CMB) reconstructed from South Pole Telescope (SPT) and Planck data over 1289 deg2. When combining measurements across multiple galaxy redshift bins spanning the redshift range of 0.15 < z < 0.90, we reject the hypothesis of no correlation at 19.9σ significance. When removing small-scale data points where thermal Sunyaev-Zel’dovich signal and nonlinear galaxy bias could potentially bias our results, the detection significance is reduced to 9.9σ. We perform a joint analysis of galaxy-CMB lensing cross-correlations and galaxy clustering to constrain cosmology, finding Ωm=0.276$$^{+0.029}_{-0.030}$$ and S8=σ8$$\sqrt{Ω -m/0.3}$$ = 0.800$$^{+0.090}_{-0.094}$$. We additionally perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, discovering consistency with predictions from the concordance ΛCDM model. The measurements presented here are part of a joint cosmological analysis that combines galaxy clustering, galaxy lensing and CMB lensing using data from DES, SPT and Planck.

Authors:
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Publication Date:
Research Org.:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR); USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Org.:
DES and SPT Collaborations
OSTI Identifier:
1560423
Alternate Identifier(s):
OSTI ID: 1546826; OSTI ID: 1560632; OSTI ID: 1561940; OSTI ID: 1644019; OSTI ID: 1705068
Grant/Contract Number:  
AC05-00OR22725; SC0019193; SC0007859; AC02-76SF00515; AST-1138766; AST-1536171; ACI-1445606; AYA2015-71825; FPA2015-68048; SEV-2016-0588; SEV-2016-0597; MDM-2015-0509; 240672; 291329; 306478; FP7/2007-2013; CE110001020; AC02-07CH11359; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review D
Additional Journal Information:
Journal Volume: 100; Journal Issue: 4; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Cosmic microwave background; Cosmological parameters; Large scale structure of the Universe

Citation Formats

Omori, Y., Giannantonio, T., Porredon, A., Baxter, E. J., Chang, C., Crocce, M., Fosalba, P., Alarcon, A., Banik, N., Blazek, J., Bleem, L. E., Bridle, S. L., Cawthon, R., Choi, A., Chown, R., Crawford, T., Dodelson, S., Drlica-Wagner, A., Eifler, T. F., Elvin-Poole, J., Friedrich, O., Gruen, D., Holder, G. P., Huterer, D., Jain, B., Jarvis, M., Kirk, D., Kokron, N., Krause, E., MacCrann, N., Muir, J., Prat, J., Reichardt, C. L., Ross, A. J., Rozo, E., Rykoff, E. S., Sánchez, C., Secco, L. F., Simard, G., Wechsler, R. H., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Allam, S., Avila, S., Aylor, K., Benson, B. A., Bernstein, G. M., Bertin, E., Bianchini, F., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Chang, C. L., Cho, H-M., Crites, A. T., Cunha, C. E., da Costa, L. N., de Haan, T., Davis, C., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dobbs, M. A., Everett, W. B., Doel, P., Estrada, J., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., George, E. M., Gruendl, R. A., Gschwend, J., Gutierrez, G., Halverson, N. W., Harrington, N. L., Hartley, W. G., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hou, Z., Hoyle, B., Hrubes, J. D., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lee, A. T., Leitch, E. M., Lima, M., Luong-Van, D., Manzotti, A., Marrone, D. P., Marshall, J. L., McMahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miller, C. J., Miquel, R., Mocanu, L. M., Mohr, J. J., Natoli, T., Padin, S., Plazas, A. A., Pryke, C., Romer, A. K., Roodman, A., Ruhl, J. E., Sanchez, E., Scarpine, V., Schaffer, K. K., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Shirokoff, E., Smith, M., Soares-Santos, M., Sobreira, F., Staniszewski, Z., Stark, A. A., Story, K. T., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Troxel, M. A., Vanderlinde, K., Vieira, J. D., Walker, A. R., Wu, W. L. K., and Zahn, O. Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck. United States: N. p., 2019. Web. doi:10.1103/PhysRevD.100.043501.
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Omori, Y., Giannantonio, T., Porredon, A., Baxter, E. J., Chang, C., Crocce, M., Fosalba, P., Alarcon, A., Banik, N., Blazek, J., Bleem, L. E., Bridle, S. L., Cawthon, R., Choi, A., Chown, R., Crawford, T., Dodelson, S., Drlica-Wagner, A., Eifler, T. F., Elvin-Poole, J., Friedrich, O., Gruen, D., Holder, G. P., Huterer, D., Jain, B., Jarvis, M., Kirk, D., Kokron, N., Krause, E., MacCrann, N., Muir, J., Prat, J., Reichardt, C. L., Ross, A. J., Rozo, E., Rykoff, E. S., Sánchez, C., Secco, L. F., Simard, G., Wechsler, R. H., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Allam, S., Avila, S., Aylor, K., Benson, B. A., Bernstein, G. M., Bertin, E., Bianchini, F., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Chang, C. L., Cho, H-M., Crites, A. T., Cunha, C. E., da Costa, L. N., de Haan, T., Davis, C., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dobbs, M. A., Everett, W. B., Doel, P., Estrada, J., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., George, E. M., Gruendl, R. A., Gschwend, J., Gutierrez, G., Halverson, N. W., Harrington, N. L., Hartley, W. G., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hou, Z., Hoyle, B., Hrubes, J. D., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lee, A. T., Leitch, E. M., Lima, M., Luong-Van, D., Manzotti, A., Marrone, D. P., Marshall, J. L., McMahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miller, C. J., Miquel, R., Mocanu, L. M., Mohr, J. J., Natoli, T., Padin, S., Plazas, A. A., Pryke, C., Romer, A. K., Roodman, A., Ruhl, J. E., Sanchez, E., Scarpine, V., Schaffer, K. K., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Shirokoff, E., Smith, M., Soares-Santos, M., Sobreira, F., Staniszewski, Z., Stark, A. A., Story, K. T., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Troxel, M. A., Vanderlinde, K., Vieira, J. D., Walker, A. R., Wu, W. L. K., & Zahn, O. Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck. United States. doi:10.1103/PhysRevD.100.043501.
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Omori, Y., Giannantonio, T., Porredon, A., Baxter, E. J., Chang, C., Crocce, M., Fosalba, P., Alarcon, A., Banik, N., Blazek, J., Bleem, L. E., Bridle, S. L., Cawthon, R., Choi, A., Chown, R., Crawford, T., Dodelson, S., Drlica-Wagner, A., Eifler, T. F., Elvin-Poole, J., Friedrich, O., Gruen, D., Holder, G. P., Huterer, D., Jain, B., Jarvis, M., Kirk, D., Kokron, N., Krause, E., MacCrann, N., Muir, J., Prat, J., Reichardt, C. L., Ross, A. J., Rozo, E., Rykoff, E. S., Sánchez, C., Secco, L. F., Simard, G., Wechsler, R. H., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Allam, S., Avila, S., Aylor, K., Benson, B. A., Bernstein, G. M., Bertin, E., Bianchini, F., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Chang, C. L., Cho, H-M., Crites, A. T., Cunha, C. E., da Costa, L. N., de Haan, T., Davis, C., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dobbs, M. A., Everett, W. B., Doel, P., Estrada, J., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., George, E. M., Gruendl, R. A., Gschwend, J., Gutierrez, G., Halverson, N. W., Harrington, N. L., Hartley, W. G., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hou, Z., Hoyle, B., Hrubes, J. D., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lee, A. T., Leitch, E. M., Lima, M., Luong-Van, D., Manzotti, A., Marrone, D. P., Marshall, J. L., McMahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miller, C. J., Miquel, R., Mocanu, L. M., Mohr, J. J., Natoli, T., Padin, S., Plazas, A. A., Pryke, C., Romer, A. K., Roodman, A., Ruhl, J. E., Sanchez, E., Scarpine, V., Schaffer, K. K., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Shirokoff, E., Smith, M., Soares-Santos, M., Sobreira, F., Staniszewski, Z., Stark, A. A., Story, K. T., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Troxel, M. A., Vanderlinde, K., Vieira, J. D., Walker, A. R., Wu, W. L. K., and Zahn, O. Thu . "Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck". United States. doi:10.1103/PhysRevD.100.043501. https://www.osti.gov/servlets/purl/1560423.
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@article{osti_1560423,
title = {Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck},
author = {Omori, Y. and Giannantonio, T. and Porredon, A. and Baxter, E. J. and Chang, C. and Crocce, M. and Fosalba, P. and Alarcon, A. and Banik, N. and Blazek, J. and Bleem, L. E. and Bridle, S. L. and Cawthon, R. and Choi, A. and Chown, R. and Crawford, T. and Dodelson, S. and Drlica-Wagner, A. and Eifler, T. F. and Elvin-Poole, J. and Friedrich, O. and Gruen, D. and Holder, G. P. and Huterer, D. and Jain, B. and Jarvis, M. and Kirk, D. and Kokron, N. and Krause, E. and MacCrann, N. and Muir, J. and Prat, J. and Reichardt, C. L. and Ross, A. J. and Rozo, E. and Rykoff, E. S. and Sánchez, C. and Secco, L. F. and Simard, G. and Wechsler, R. H. and Zuntz, J. and Abbott, T. M. C. and Abdalla, F. B. and Allam, S. and Avila, S. and Aylor, K. and Benson, B. A. and Bernstein, G. M. and Bertin, E. and Bianchini, F. and Brooks, D. and Buckley-Geer, E. and Burke, D. L. and Carlstrom, J. E. and Carnero Rosell, A. and Carrasco Kind, M. and Carretero, J. and Castander, F. J. and Chang, C. L. and Cho, H-M. and Crites, A. T. and Cunha, C. E. and da Costa, L. N. and de Haan, T. and Davis, C. and De Vicente, J. and Desai, S. and Diehl, H. T. and Dietrich, J. P. and Dobbs, M. A. and Everett, W. B. and Doel, P. and Estrada, J. and Flaugher, B. and Frieman, J. and García-Bellido, J. and Gaztanaga, E. and Gerdes, D. W. and George, E. M. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Halverson, N. W. and Harrington, N. L. and Hartley, W. G. and Hollowood, D. L. and Holzapfel, W. L. and Honscheid, K. and Hou, Z. and Hoyle, B. and Hrubes, J. D. and James, D. J. and Jeltema, T. and Kuehn, K. and Kuropatkin, N. and Lee, A. T. and Leitch, E. M. and Lima, M. and Luong-Van, D. and Manzotti, A. and Marrone, D. P. and Marshall, J. L. and McMahon, J. J. and Melchior, P. and Menanteau, F. and Meyer, S. S. and Miller, C. J. and Miquel, R. and Mocanu, L. M. and Mohr, J. J. and Natoli, T. and Padin, S. and Plazas, A. A. and Pryke, C. and Romer, A. K. and Roodman, A. and Ruhl, J. E. and Sanchez, E. and Scarpine, V. and Schaffer, K. K. and Schubnell, M. and Serrano, S. and Sevilla-Noarbe, I. and Shirokoff, E. and Smith, M. and Soares-Santos, M. and Sobreira, F. and Staniszewski, Z. and Stark, A. A. and Story, K. T. and Suchyta, E. and Swanson, M. E. C. and Tarle, G. and Thomas, D. and Troxel, M. A. and Vanderlinde, K. and Vieira, J. D. and Walker, A. R. and Wu, W. L. K. and Zahn, O.},
abstractNote = {We analyze the cross-correlation between redMaGiC galaxies selected from the Dark Energy Survey (DES) year 1 data and gravitational lensing of the cosmic microwave background (CMB) reconstructed from South Pole Telescope (SPT) and Planck data over 1289 deg2. When combining measurements across multiple galaxy redshift bins spanning the redshift range of 0.15 < z < 0.90, we reject the hypothesis of no correlation at 19.9σ significance. When removing small-scale data points where thermal Sunyaev-Zel’dovich signal and nonlinear galaxy bias could potentially bias our results, the detection significance is reduced to 9.9σ. We perform a joint analysis of galaxy-CMB lensing cross-correlations and galaxy clustering to constrain cosmology, finding Ωm=0.276$^{+0.029}_{-0.030}$ and S8=σ8$\sqrt{Ω -m/0.3}$ = 0.800$^{+0.090}_{-0.094}$. We additionally perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, discovering consistency with predictions from the concordance ΛCDM model. The measurements presented here are part of a joint cosmological analysis that combines galaxy clustering, galaxy lensing and CMB lensing using data from DES, SPT and Planck.},
doi = {10.1103/PhysRevD.100.043501},
journal = {Physical Review D},
number = 4,
volume = 100,
place = {United States},
year = {2019},
month = {8}
}
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DOI:  10.1103/PhysRevD.100.043501
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  • Singh, Sukhdeep; Alam, Shadab; Mandelbaum, Rachel
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journal, December 2016

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conference, July 2014

  • Benson, B. A.; Ade, P. A. R.; Ahmed, Z.
  • SPIE Astronomical Telescopes + Instrumentation, SPIE Proceedings
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Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters
journal, September 2016

Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
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    Works referencing / citing this record:

    CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
    journal, October 2019

    • Fabbian, Giulio; Lewis, Antony; Beck, Dominic
    • Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 10
    • DOI: 10.1088/1475-7516/2019/10/057

    Cross-correlation of CMB Polarization Lensing with High- z Submillimeter Herschel -ATLAS Galaxies
    journal, November 2019

    • Faúndez, M. Aguilar; Arnold, K.; Baccigalupi, C.
    • The Astrophysical Journal, Vol. 886, Issue 1
    • DOI: 10.3847/1538-4357/ab4a78
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