A measurement of CMB cluster lensing with SPT and DES year 1 data

E. J. Baxter; S. Raghunathan; T. M. Crawford; P. Fosalba; Z. Hou; G. P. Holder; Y. Omori; S. Patil; E. Rozo; T. M.C. Abbott; J. Annis; K. Aylor; A. Benoit-Lévy; B. A. Benson; E. Bertin; L. Bleem; E. Buckley-Geer; D. L. Burke; J. Carlstrom; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; C. L. Chang; H. M. Cho; A. T. Crites; M. Crocce; C. E. Cunha; L. N. da Costa; C. B. D'Andrea; C. Davis; T. de Haan; S. Desai; J. P. Dietrich; M. A. Dobbs; S. Dodelson; P. Doel; A. Drlica-Wagner; J. Estrada; W. B. Everett; A. Fausti Neto; B. Flaugher; J. Frieman; J. García-Bellido; E. M. George; E. Gaztanaga; T. Giannantonio; D. Gruen; R. A. Gruendl; J. Gschwend; G. Gutierrez; N. W. Halverson; N. L. Harrington; W. G. Hartley; W. L. Holzapfel; K. Honscheid; J. D. Hrubes; B. Jain; D. J. James; M. Jarvis; T. Jeltema; L. Knox; E. Krause; K. Kuehn; S. Kuhlmann; N. Kuropatkin; O. Lahav; A. T. Lee; E. M. Leitch; T. S. Li; M. Lima; D. Luong-Van; A. Manzotti; M. March; D. P. Marrone; J. L. Marshall; P. Martini; J. J. McMahon; P. Melchior; F. Menanteau; S. S. Meyer; C. J. Miller; R. Miquel; L. M. Mocanu; J. J. Mohr; T. Natoli; B. Nord; R. L.C. Ogando; S. Padin; A. A. Plazas; C. Pryke; D. Rapetti; C. L. Reichardt; A. K. Romer; A. Roodman; J. E. Ruhl; E. Rykoff; M. Sako; E. Sanchez; J. T. Sayre; V. Scarpine

doi:10.1093/MNRAS/STY305

A measurement of CMB cluster lensing with SPT and DES year 1 data

E. J. Baxter, S. Raghunathan, T. M. Crawford, P. Fosalba, Z. Hou, G. P. Holder, Y. Omori, S. Patil, E. Rozo, T. M.C. Abbott, J. Annis, K. Aylor, A. Benoit-Lévy, B. A. Benson, E. Bertin, L. Bleem, E. Buckley-Geer, D. L. Burke, J. Carlstrom, A. Carnero RosellM. Carrasco Kind, J. Carretero, C. L. Chang, H. M. Cho, A. T. Crites, M. Crocce, C. E. Cunha, L. N. da Costa, C. B. D'Andrea, C. Davis, T. de Haan, S. Desai, J. P. Dietrich, M. A. Dobbs, S. Dodelson, P. Doel, A. Drlica-Wagner, J. Estrada, W. B. Everett, A. Fausti Neto, B. Flaugher, J. Frieman, J. García-Bellido, E. M. George, E. Gaztanaga, T. Giannantonio, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, N. W. Halverson, N. L. Harrington, W. G. Hartley, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, B. Jain, D. J. James, M. Jarvis, T. Jeltema, L. Knox, E. Krause, K. Kuehn, S. Kuhlmann, N. Kuropatkin, O. Lahav, A. T. Lee, E. M. Leitch, T. S. Li, M. Lima, D. Luong-Van, A. Manzotti, M. March, D. P. Marrone, J. L. Marshall, P. Martini, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, C. J. Miller, R. Miquel, L. M. Mocanu, J. J. Mohr, T. Natoli, B. Nord, R. L.C. Ogando, S. Padin, A. A. Plazas, C. Pryke, D. Rapetti, C. L. Reichardt, A. K. Romer, A. Roodman, J. E. Ruhl, E. Rykoff, M. Sako, E. Sanchez, J. T. Sayre, V. Scarpine

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© 2018 The Author(s). Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev-Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalogue used in this analysis contains 3697 members with mean redshift of z = 0.45. We detect lensing of the CMB by the galaxy clusters at 8.1s significance. Using the measured lensing signal, we constrain the amplitude of the relation between cluster mass and optical richness to roughly 17 per cent precision, finding good agreement with recent constraints obtained with galaxy lensing. The error budget is dominated by statistical noise but includes significant contributions from systematic biases due to the thermal SZ effect and cluster miscentring.

Idioma original	Inglés
Páginas (desde-hasta)	2674-2688
Publicación	Monthly Notices of the Royal Astronomical Society
Volumen	476
N.º	2
DOI	https://doi.org/10.1093/MNRAS/STY305
Estado	Publicada - 11 may 2018

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Baxter, E. J., Raghunathan, S., Crawford, T. M., Fosalba, P., Hou, Z., Holder, G. P., Omori, Y., Patil, S., Rozo, E., Abbott, T. M. C., Annis, J., Aylor, K., Benoit-Lévy, A., Benson, B. A., Bertin, E., Bleem, L., Buckley-Geer, E., Burke, D. L., Carlstrom, J., ... Scarpine, V. (2018). A measurement of CMB cluster lensing with SPT and DES year 1 data. Monthly Notices of the Royal Astronomical Society, 476(2), 2674-2688. https://doi.org/10.1093/MNRAS/STY305

@article{59b6c830ef6c404ebba0e1a5d5ad91fa,

title = "A measurement of CMB cluster lensing with SPT and DES year 1 data",

abstract = "{\textcopyright} 2018 The Author(s). Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev-Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalogue used in this analysis contains 3697 members with mean redshift of z = 0.45. We detect lensing of the CMB by the galaxy clusters at 8.1s significance. Using the measured lensing signal, we constrain the amplitude of the relation between cluster mass and optical richness to roughly 17 per cent precision, finding good agreement with recent constraints obtained with galaxy lensing. The error budget is dominated by statistical noise but includes significant contributions from systematic biases due to the thermal SZ effect and cluster miscentring.",

keywords = "Cosmic background radiation, Galaxies: clusters: general, Gravitational lensing: weak",

author = "Baxter, {E. J.} and S. Raghunathan and Crawford, {T. M.} and P. Fosalba and Z. Hou and Holder, {G. P.} and Y. Omori and S. Patil and E. Rozo and Abbott, {T. M.C.} and J. Annis and K. Aylor and A. Benoit-L{\'e}vy and Benson, {B. A.} and E. Bertin and L. Bleem and E. Buckley-Geer and Burke, {D. L.} and J. Carlstrom and {Carnero Rosell}, A. and {Carrasco Kind}, M. and J. Carretero and Chang, {C. L.} and Cho, {H. M.} and Crites, {A. T.} and M. Crocce and Cunha, {C. E.} and {da Costa}, {L. N.} and D'Andrea, {C. B.} and C. Davis and {de Haan}, T. and S. Desai and Dietrich, {J. P.} and Dobbs, {M. A.} and S. Dodelson and P. Doel and A. Drlica-Wagner and J. Estrada and Everett, {W. B.} and {Fausti Neto}, A. and B. Flaugher and J. Frieman and J. Garc{\'i}a-Bellido and George, {E. M.} and E. Gaztanaga and T. Giannantonio and D. Gruen and Gruendl, {R. A.} and J. Gschwend and G. Gutierrez and Halverson, {N. W.} and Harrington, {N. L.} and Hartley, {W. G.} and Holzapfel, {W. L.} and K. Honscheid and Hrubes, {J. D.} and B. Jain and James, {D. J.} and M. Jarvis and T. Jeltema and L. Knox and E. Krause and K. Kuehn and S. Kuhlmann and N. Kuropatkin and O. Lahav and Lee, {A. T.} and Leitch, {E. M.} and Li, {T. S.} and M. Lima and D. Luong-Van and A. Manzotti and M. March and Marrone, {D. P.} and Marshall, {J. L.} and P. Martini and McMahon, {J. J.} and P. Melchior and F. Menanteau and Meyer, {S. S.} and Miller, {C. J.} and R. Miquel and Mocanu, {L. M.} and Mohr, {J. J.} and T. Natoli and B. Nord and Ogando, {R. L.C.} and S. Padin and Plazas, {A. A.} and C. Pryke and D. Rapetti and Reichardt, {C. L.} and Romer, {A. K.} and A. Roodman and Ruhl, {J. E.} and E. Rykoff and M. Sako and E. Sanchez and Sayre, {J. T.} and V. Scarpine",

year = "2018",

month = may,

day = "11",

doi = "10.1093/MNRAS/STY305",

language = "English",

volume = "476",

pages = "2674--2688",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

number = "2",

}

Baxter, EJ, Raghunathan, S, Crawford, TM, Fosalba, P, Hou, Z, Holder, GP, Omori, Y, Patil, S, Rozo, E, Abbott, TMC, Annis, J, Aylor, K, Benoit-Lévy, A, Benson, BA, Bertin, E, Bleem, L, Buckley-Geer, E, Burke, DL, Carlstrom, J, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Chang, CL, Cho, HM, Crites, AT, Crocce, M, Cunha, CE, da Costa, LN, D'Andrea, CB, Davis, C, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Dodelson, S, Doel, P, Drlica-Wagner, A, Estrada, J, Everett, WB, Fausti Neto, A, Flaugher, B, Frieman, J, García-Bellido, J, George, EM, Gaztanaga, E, Giannantonio, T, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Halverson, NW, Harrington, NL, Hartley, WG, Holzapfel, WL, Honscheid, K, Hrubes, JD, Jain, B, James, DJ, Jarvis, M, Jeltema, T, Knox, L, Krause, E, Kuehn, K, Kuhlmann, S, Kuropatkin, N, Lahav, O, Lee, AT, Leitch, EM, Li, TS, Lima, M, Luong-Van, D, Manzotti, A, March, M, Marrone, DP, Marshall, JL, Martini, P, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miller, CJ, Miquel, R, Mocanu, LM, Mohr, JJ, Natoli, T, Nord, B, Ogando, RLC, Padin, S, Plazas, AA, Pryke, C, Rapetti, D, Reichardt, CL, Romer, AK, Roodman, A, Ruhl, JE, Rykoff, E, Sako, M, Sanchez, E, Sayre, JT & Scarpine, V 2018, 'A measurement of CMB cluster lensing with SPT and DES year 1 data', Monthly Notices of the Royal Astronomical Society, vol. 476, n.º 2, pp. 2674-2688. https://doi.org/10.1093/MNRAS/STY305

TY - JOUR

T1 - A measurement of CMB cluster lensing with SPT and DES year 1 data

AU - Baxter, E. J.

AU - Raghunathan, S.

AU - Crawford, T. M.

AU - Fosalba, P.

AU - Hou, Z.

AU - Holder, G. P.

AU - Omori, Y.

AU - Patil, S.

AU - Rozo, E.

AU - Abbott, T. M.C.

AU - Annis, J.

AU - Aylor, K.

AU - Benoit-Lévy, A.

AU - Benson, B. A.

AU - Bertin, E.

AU - Bleem, L.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Carlstrom, J.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Chang, C. L.

AU - Cho, H. M.

AU - Crites, A. T.

AU - Crocce, M.

AU - Cunha, C. E.

AU - da Costa, L. N.

AU - D'Andrea, C. B.

AU - Davis, C.

AU - de Haan, T.

AU - Desai, S.

AU - Dietrich, J. P.

AU - Dobbs, M. A.

AU - Dodelson, S.

AU - Doel, P.

AU - Drlica-Wagner, A.

AU - Estrada, J.

AU - Everett, W. B.

AU - Fausti Neto, A.

AU - Flaugher, B.

AU - Frieman, J.

AU - García-Bellido, J.

AU - George, E. M.

AU - Gaztanaga, E.

AU - Giannantonio, T.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Halverson, N. W.

AU - Harrington, N. L.

AU - Hartley, W. G.

AU - Holzapfel, W. L.

AU - Honscheid, K.

AU - Hrubes, J. D.

AU - Jain, B.

AU - James, D. J.

AU - Jarvis, M.

AU - Jeltema, T.

AU - Knox, L.

AU - Krause, E.

AU - Kuehn, K.

AU - Kuhlmann, S.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Li, T. S.

AU - Lima, M.

AU - Luong-Van, D.

AU - Manzotti, A.

AU - March, M.

AU - Marrone, D. P.

AU - Marshall, J. L.

AU - Martini, P.

AU - McMahon, J. J.

AU - Melchior, P.

AU - Menanteau, F.

AU - Meyer, S. S.

AU - Miller, C. J.

AU - Miquel, R.

AU - Mocanu, L. M.

AU - Mohr, J. J.

AU - Natoli, T.

AU - Nord, B.

AU - Ogando, R. L.C.

AU - Padin, S.

AU - Plazas, A. A.

AU - Pryke, C.

AU - Rapetti, D.

AU - Reichardt, C. L.

AU - Romer, A. K.

AU - Roodman, A.

AU - Ruhl, J. E.

AU - Rykoff, E.

AU - Sako, M.

AU - Sanchez, E.

AU - Sayre, J. T.

AU - Scarpine, V.

PY - 2018/5/11

Y1 - 2018/5/11

N2 - © 2018 The Author(s). Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev-Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalogue used in this analysis contains 3697 members with mean redshift of z = 0.45. We detect lensing of the CMB by the galaxy clusters at 8.1s significance. Using the measured lensing signal, we constrain the amplitude of the relation between cluster mass and optical richness to roughly 17 per cent precision, finding good agreement with recent constraints obtained with galaxy lensing. The error budget is dominated by statistical noise but includes significant contributions from systematic biases due to the thermal SZ effect and cluster miscentring.

AB - © 2018 The Author(s). Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev-Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalogue used in this analysis contains 3697 members with mean redshift of z = 0.45. We detect lensing of the CMB by the galaxy clusters at 8.1s significance. Using the measured lensing signal, we constrain the amplitude of the relation between cluster mass and optical richness to roughly 17 per cent precision, finding good agreement with recent constraints obtained with galaxy lensing. The error budget is dominated by statistical noise but includes significant contributions from systematic biases due to the thermal SZ effect and cluster miscentring.

KW - Cosmic background radiation

KW - Galaxies: clusters: general

KW - Gravitational lensing: weak

U2 - 10.1093/MNRAS/STY305

DO - 10.1093/MNRAS/STY305

M3 - Article

SN - 0035-8711

VL - 476

SP - 2674

EP - 2688

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

A measurement of CMB cluster lensing with SPT and DES year 1 data

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