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

Y. Omori; Y. Omori; T. Giannantonio; A. Porredon; E. J. Baxter; C. Chang; M. Crocce; P. Fosalba; A. Alarcon; N. Banik; J. Blazek; L. E. Bleem; S. L. Bridle; R. Cawthon; A. Choi; R. Chown; T. Crawford; S. Dodelson; A. Drlica-Wagner; T. F. Eifler; J. Elvin-Poole; O. Friedrich; D. Gruen; G. P. Holder; D. Huterer; B. Jain; M. Jarvis; D. Kirk; N. Kokron; E. Krause; N. Maccrann; J. Muir; J. Prat; C. L. Reichardt; A. J. Ross; E. Rozo; E. S. Rykoff; C. Sánchez; L. F. Secco; G. Simard; R. H. Wechsler; J. Zuntz; T. M.C. Abbott; F. B. Abdalla; S. Allam; S. Avila; K. Aylor; B. A. Benson; G. M. Bernstein; E. Bertin; F. Bianchini; D. Brooks; E. Buckley-Geer; D. L. Burke; J. E. Carlstrom; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; F. J. Castander; C. L. Chang; H. M. Cho; A. T. Crites; C. E. Cunha; L. N. Da Costa; T. De Haan; C. Davis; J. De Vicente; S. Desai; H. T. Diehl; J. P. Dietrich; M. A. Dobbs; W. B. Everett; P. Doel; J. Estrada; B. Flaugher; J. Frieman; J. García-Bellido; E. Gaztanaga; D. W. Gerdes; E. M. George; R. A. Gruendl; J. Gschwend; G. Gutierrez; N. W. Halverson; N. L. Harrington; W. G. Hartley; D. L. Hollowood; W. L. Holzapfel; K. Honscheid; Z. Hou; B. Hoyle; J. D. Hrubes; D. J. James; T. Jeltema; K. Kuehn; N. Kuropatkin; A. T. Lee; E. M. Leitch; M. Lima; D. Luong-Van

doi:10.1103/PhysRevD.100.043501

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

Y. Omori, Y. Omori, T. Giannantonio, A. Porredon, E. J. Baxter, C. Chang, M. Crocce, P. Fosalba, A. Alarcon, N. Banik, J. Blazek, L. E. Bleem, S. L. Bridle, R. Cawthon, A. Choi, R. Chown, T. Crawford, S. Dodelson, A. Drlica-Wagner, T. F. EiflerJ. Elvin-Poole, O. Friedrich, D. Gruen, G. P. Holder, D. Huterer, B. Jain, M. Jarvis, D. Kirk, N. Kokron, E. Krause, N. Maccrann, J. Muir, J. Prat, C. L. Reichardt, A. J. Ross, E. Rozo, E. S. Rykoff, C. Sánchez, L. F. Secco, G. Simard, R. H. Wechsler, J. Zuntz, T. M.C. Abbott, F. B. Abdalla, S. Allam, S. Avila, K. Aylor, B. A. Benson, G. M. Bernstein, E. Bertin, F. Bianchini, D. Brooks, E. Buckley-Geer, D. L. Burke, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, C. L. Chang, H. M. Cho, A. T. Crites, C. E. Cunha, L. N. Da Costa, T. De Haan, C. Davis, J. De Vicente, S. Desai, H. T. Diehl, J. P. Dietrich, M. A. Dobbs, W. B. Everett, P. Doel, J. Estrada, B. Flaugher, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, E. M. George, R. A. Gruendl, J. Gschwend, G. Gutierrez, N. W. Halverson, N. L. Harrington, W. G. Hartley, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, Z. Hou, B. Hoyle, J. D. Hrubes, D. J. James, T. Jeltema, K. Kuehn, N. Kuropatkin, A. T. Lee, E. M. Leitch, M. Lima, D. Luong-Van

Research output: Contribution to journal › Article › Research

13 Citations (Scopus)

Abstract

© 2019 American Physical Society. We measure 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=0.276-0.030+0.029 and S8=σ8ωm/0.3=0.800-0.094+0.090. We also perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, finding 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.

Original language	English
Article number	043501
Journal	Physical Review D
Volume	100
DOIs	https://doi.org/10.1103/PhysRevD.100.043501
Publication status	Published - 1 Aug 2019

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Omori, Y., 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., ... Luong-Van, D. (2019). Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck. Physical Review D, 100, [043501]. https://doi.org/10.1103/PhysRevD.100.043501

Omori, Y. ; 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. / Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck. In: Physical Review D. 2019 ; Vol. 100.

@article{f16a3fab74df4612b5e7d5d4113aeeff,

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

abstract = "{\textcopyright} 2019 American Physical Society. We measure 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=0.276-0.030+0.029 and S8=σ8ωm/0.3=0.800-0.094+0.090. We also perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, finding 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.",

author = "Y. Omori and Y. Omori and T. Giannantonio and A. Porredon and Baxter, {E. J.} and C. Chang and M. Crocce and P. Fosalba and A. Alarcon and N. Banik and J. Blazek and Bleem, {L. E.} and Bridle, {S. L.} and R. Cawthon and A. Choi and R. Chown and T. Crawford and S. Dodelson and A. Drlica-Wagner and Eifler, {T. F.} and J. Elvin-Poole and O. Friedrich and D. Gruen and Holder, {G. P.} and D. Huterer and B. Jain and M. Jarvis and D. Kirk and N. Kokron and E. Krause and N. Maccrann and J. Muir and J. Prat and Reichardt, {C. L.} and Ross, {A. J.} and E. Rozo and Rykoff, {E. S.} and C. S{\'a}nchez and Secco, {L. F.} and G. Simard and Wechsler, {R. H.} and J. Zuntz and Abbott, {T. M.C.} and Abdalla, {F. B.} and S. Allam and S. Avila and K. Aylor and Benson, {B. A.} and Bernstein, {G. M.} and E. Bertin and F. Bianchini and D. Brooks and E. Buckley-Geer and Burke, {D. L.} and Carlstrom, {J. E.} and {Carnero Rosell}, A. and {Carrasco Kind}, M. and J. Carretero 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 C. Davis and {De Vicente}, J. and S. Desai and Diehl, {H. T.} and Dietrich, {J. P.} and Dobbs, {M. A.} and Everett, {W. B.} and P. Doel and J. Estrada and B. Flaugher and J. Frieman and J. Garc{\'i}a-Bellido and E. Gaztanaga and Gerdes, {D. W.} and George, {E. M.} and Gruendl, {R. A.} and J. Gschwend and G. Gutierrez and Halverson, {N. W.} and Harrington, {N. L.} and Hartley, {W. G.} and Hollowood, {D. L.} and Holzapfel, {W. L.} and K. Honscheid and Z. Hou and B. Hoyle and Hrubes, {J. D.} and James, {D. J.} and T. Jeltema and K. Kuehn and N. Kuropatkin and Lee, {A. T.} and Leitch, {E. M.} and M. Lima and D. Luong-Van",

year = "2019",

month = aug,

day = "1",

doi = "10.1103/PhysRevD.100.043501",

language = "English",

volume = "100",

journal = "Physical Review D",

issn = "2470-0010",

}

Omori, Y, Omori, Y, Giannantonio, T, Porredon, A, Baxter, EJ, Chang, C, Crocce, M, Fosalba, P, Alarcon, A, Banik, N, Blazek, J, Bleem, LE, Bridle, SL, Cawthon, R, Choi, A, Chown, R, Crawford, T, Dodelson, S, Drlica-Wagner, A, Eifler, TF, Elvin-Poole, J, Friedrich, O, Gruen, D, Holder, GP, Huterer, D, Jain, B, Jarvis, M, Kirk, D, Kokron, N, Krause, E, Maccrann, N, Muir, J, Prat, J, Reichardt, CL, Ross, AJ, Rozo, E, Rykoff, ES, Sánchez, C, Secco, LF, Simard, G, Wechsler, RH, Zuntz, J, Abbott, TMC, Abdalla, FB, Allam, S, Avila, S, Aylor, K, Benson, BA, Bernstein, GM, Bertin, E, Bianchini, F, Brooks, D, Buckley-Geer, E, Burke, DL, Carlstrom, JE, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, FJ, Chang, CL, Cho, HM, Crites, AT, Cunha, CE, Da Costa, LN, De Haan, T, Davis, C, De Vicente, J, Desai, S, Diehl, HT, Dietrich, JP, Dobbs, MA, Everett, WB, Doel, P, Estrada, J, Flaugher, B, Frieman, J, García-Bellido, J, Gaztanaga, E, Gerdes, DW, George, EM, Gruendl, RA, Gschwend, J, Gutierrez, G, Halverson, NW, Harrington, NL, Hartley, WG, Hollowood, DL, Holzapfel, WL, Honscheid, K, Hou, Z, Hoyle, B, Hrubes, JD, James, DJ, Jeltema, T, Kuehn, K, Kuropatkin, N, Lee, AT, Leitch, EM, Lima, M & Luong-Van, D 2019, 'Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck', Physical Review D, vol. 100, 043501. https://doi.org/10.1103/PhysRevD.100.043501

Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck. / Omori, Y.; 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.

In: Physical Review D, Vol. 100, 043501, 01.08.2019.

Research output: Contribution to journal › Article › Research

TY - JOUR

T1 - Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck

AU - Omori, Y.

AU - Giannantonio, T.

AU - Porredon, A.

AU - Baxter, E. J.

AU - Chang, C.

AU - Crocce, M.

AU - Fosalba, P.

AU - Alarcon, A.

AU - Banik, N.

AU - Blazek, J.

AU - Bleem, L. E.

AU - Bridle, S. L.

AU - Cawthon, R.

AU - Choi, A.

AU - Chown, R.

AU - Crawford, T.

AU - Dodelson, S.

AU - Drlica-Wagner, A.

AU - Eifler, T. F.

AU - Elvin-Poole, J.

AU - Friedrich, O.

AU - Gruen, D.

AU - Holder, G. P.

AU - Huterer, D.

AU - Jain, B.

AU - Jarvis, M.

AU - Kirk, D.

AU - Kokron, N.

AU - Krause, E.

AU - Maccrann, N.

AU - Muir, J.

AU - Prat, J.

AU - Reichardt, C. L.

AU - Ross, A. J.

AU - Rozo, E.

AU - Rykoff, E. S.

AU - Sánchez, C.

AU - Secco, L. F.

AU - Simard, G.

AU - Wechsler, R. H.

AU - Zuntz, J.

AU - Abbott, T. M.C.

AU - Abdalla, F. B.

AU - Allam, S.

AU - Avila, S.

AU - Aylor, K.

AU - Benson, B. A.

AU - Bernstein, G. M.

AU - Bertin, E.

AU - Bianchini, F.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Carlstrom, J. E.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Castander, F. J.

AU - Chang, C. L.

AU - Cho, H. M.

AU - Crites, A. T.

AU - Cunha, C. E.

AU - Da Costa, L. N.

AU - De Haan, T.

AU - Davis, C.

AU - De Vicente, J.

AU - Desai, S.

AU - Diehl, H. T.

AU - Dietrich, J. P.

AU - Dobbs, M. A.

AU - Everett, W. B.

AU - Doel, P.

AU - Estrada, J.

AU - Flaugher, B.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Gaztanaga, E.

AU - Gerdes, D. W.

AU - George, E. M.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Halverson, N. W.

AU - Harrington, N. L.

AU - Hartley, W. G.

AU - Hollowood, D. L.

AU - Holzapfel, W. L.

AU - Honscheid, K.

AU - Hou, Z.

AU - Hoyle, B.

AU - Hrubes, J. D.

AU - James, D. J.

AU - Jeltema, T.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Lima, M.

AU - Luong-Van, D.

PY - 2019/8/1

Y1 - 2019/8/1

N2 - © 2019 American Physical Society. We measure 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=0.276-0.030+0.029 and S8=σ8ωm/0.3=0.800-0.094+0.090. We also perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, finding 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.

AB - © 2019 American Physical Society. We measure 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=0.276-0.030+0.029 and S8=σ8ωm/0.3=0.800-0.094+0.090. We also perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, finding 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.

U2 - 10.1103/PhysRevD.100.043501

DO - 10.1103/PhysRevD.100.043501

M3 - Article

VL - 100

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

M1 - 043501

ER -