Cosmic shear measurements with Dark Energy Survey Science Verification data

M. R. Becker; M. A. Troxel; N. Maccrann; E. Krause; T. F. Eifler; O. Friedrich; A. Nicola; A. Refregier; A. Amara; D. Bacon; G. M. Bernstein; C. Bonnett; S. L. Bridle; M. T. Busha; C. Chang; S. Dodelson; B. Erickson; A. E. Evrard; J. Frieman; E. Gaztanaga; D. Gruen; W. Hartley; B. Jain; M. Jarvis; T. Kacprzak; D. Kirk; A. Kravtsov; B. Leistedt; H. V. Peiris; E. S. Rykoff; C. Sabiu; C. Sánchez; H. Seo; E. Sheldon; R. H. Wechsler; J. Zuntz; T. Abbott; F. B. Abdalla; S. Allam; R. Armstrong; M. Banerji; A. H. Bauer; A. Benoit-Lévy; E. Bertin; D. Brooks; E. Buckley-Geer; D. L. Burke; D. Capozzi; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; F. J. Castander; M. Crocce; C. E. Cunha; C. B. D'Andrea; L. N. Da Costa; D. L. Depoy; S. Desai; H. T. Diehl; J. P. Dietrich; P. Doel; A. Fausti Neto; E. Fernandez; D. A. Finley; B. Flaugher; P. Fosalba; D. W. Gerdes; R. A. Gruendl; G. Gutierrez; K. Honscheid; D. J. James; K. Kuehn; N. Kuropatkin; O. Lahav; T. S. Li; M. Lima; M. A.G. Maia; M. March; P. Martini; P. Melchior; C. J. Miller; R. Miquel; J. J. Mohr; R. C. Nichol; B. Nord; R. Ogando; A. A. Plazas; K. Reil; A. K. Romer; A. Roodman; M. Sako; E. Sanchez; V. Scarpine; M. Schubnell; I. Sevilla-Noarbe; R. C. Smith; M. Soares-Santos; F. Sobreira; E. Suchyta; M. E.C. Swanson

doi:10.1103/PhysRevD.94.022002

Cosmic shear measurements with Dark Energy Survey Science Verification data

M. R. Becker, M. A. Troxel, N. Maccrann, E. Krause, T. F. Eifler, O. Friedrich, A. Nicola, A. Refregier, A. Amara, D. Bacon, G. M. Bernstein, C. Bonnett, S. L. Bridle, M. T. Busha, C. Chang, S. Dodelson, B. Erickson, A. E. Evrard, J. Frieman, E. GaztanagaD. Gruen, W. Hartley, B. Jain, M. Jarvis, T. Kacprzak, D. Kirk, A. Kravtsov, B. Leistedt, H. V. Peiris, E. S. Rykoff, C. Sabiu, C. Sánchez, H. Seo, E. Sheldon, R. H. Wechsler, J. Zuntz, T. Abbott, F. B. Abdalla, S. Allam, R. Armstrong, M. Banerji, A. H. Bauer, A. Benoit-Lévy, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, D. Capozzi, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, M. Crocce, C. E. Cunha, C. B. D'Andrea, L. N. Da Costa, D. L. Depoy, S. Desai, H. T. Diehl, J. P. Dietrich, P. Doel, A. Fausti Neto, E. Fernandez, D. A. Finley, B. Flaugher, P. Fosalba, D. W. Gerdes, R. A. Gruendl, G. Gutierrez, K. Honscheid, D. J. James, K. Kuehn, N. Kuropatkin, O. Lahav, T. S. Li, M. Lima, M. A.G. Maia, M. March, P. Martini, P. Melchior, C. J. Miller, R. Miquel, J. J. Mohr, R. C. Nichol, B. Nord, R. Ogando, A. A. Plazas, K. Reil, A. K. Romer, A. Roodman, M. Sako, E. Sanchez, V. Scarpine, M. Schubnell, I. Sevilla-Noarbe, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E.C. Swanson

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© 2016 American Physical Society. We present measurements of weak gravitational lensing cosmic shear two-point statistics using Dark Energy Survey Science Verification data. We demonstrate that our results are robust to the choice of shear measurement pipeline, either ngmix or im3shape, and robust to the choice of two-point statistic, including both real and Fourier-space statistics. Our results pass a suite of null tests including tests for B-mode contamination and direct tests for any dependence of the two-point functions on a set of 16 observing conditions and galaxy properties, such as seeing, airmass, galaxy color, galaxy magnitude, etc. We furthermore use a large suite of simulations to compute the covariance matrix of the cosmic shear measurements and assign statistical significance to our null tests. We find that our covariance matrix is consistent with the halo model prediction, indicating that it has the appropriate level of halo sample variance. We compare the same jackknife procedure applied to the data and the simulations in order to search for additional sources of noise not captured by the simulations. We find no statistically significant extra sources of noise in the data. The overall detection significance with tomography for our highest source density catalog is 9.7σ. Cosmological constraints from the measurements in this work are presented in a companion paper [DES, Phys. Rev. D 94, 022001 (2016).].

Idioma original	Anglès
Número d’article	022002
Revista	Physical Review D
Volum	94
Número	2
DOIs	https://doi.org/10.1103/PhysRevD.94.022002
Estat de la publicació	Publicada - 6 de jul. 2016

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10.1103/PhysRevD.94.022002

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Becker, M. R., Troxel, M. A., Maccrann, N., Krause, E., Eifler, T. F., Friedrich, O., Nicola, A., Refregier, A., Amara, A., Bacon, D., Bernstein, G. M., Bonnett, C., Bridle, S. L., Busha, M. T., Chang, C., Dodelson, S., Erickson, B., Evrard, A. E., Frieman, J., ... Swanson, M. E. C. (2016). Cosmic shear measurements with Dark Energy Survey Science Verification data. Physical Review D, 94(2), Article 022002. https://doi.org/10.1103/PhysRevD.94.022002

@article{9202b7a604ca44209d0ed45395a60c3f,

title = "Cosmic shear measurements with Dark Energy Survey Science Verification data",

abstract = "{\textcopyright} 2016 American Physical Society. We present measurements of weak gravitational lensing cosmic shear two-point statistics using Dark Energy Survey Science Verification data. We demonstrate that our results are robust to the choice of shear measurement pipeline, either ngmix or im3shape, and robust to the choice of two-point statistic, including both real and Fourier-space statistics. Our results pass a suite of null tests including tests for B-mode contamination and direct tests for any dependence of the two-point functions on a set of 16 observing conditions and galaxy properties, such as seeing, airmass, galaxy color, galaxy magnitude, etc. We furthermore use a large suite of simulations to compute the covariance matrix of the cosmic shear measurements and assign statistical significance to our null tests. We find that our covariance matrix is consistent with the halo model prediction, indicating that it has the appropriate level of halo sample variance. We compare the same jackknife procedure applied to the data and the simulations in order to search for additional sources of noise not captured by the simulations. We find no statistically significant extra sources of noise in the data. The overall detection significance with tomography for our highest source density catalog is 9.7σ. Cosmological constraints from the measurements in this work are presented in a companion paper [DES, Phys. Rev. D 94, 022001 (2016).].",

author = "Becker, {M. R.} and Troxel, {M. A.} and N. Maccrann and E. Krause and Eifler, {T. F.} and O. Friedrich and A. Nicola and A. Refregier and A. Amara and D. Bacon and Bernstein, {G. M.} and C. Bonnett and Bridle, {S. L.} and Busha, {M. T.} and C. Chang and S. Dodelson and B. Erickson and Evrard, {A. E.} and J. Frieman and E. Gaztanaga and D. Gruen and W. Hartley and B. Jain and M. Jarvis and T. Kacprzak and D. Kirk and A. Kravtsov and B. Leistedt and Peiris, {H. V.} and Rykoff, {E. S.} and C. Sabiu and C. S{\'a}nchez and H. Seo and E. Sheldon and Wechsler, {R. H.} and J. Zuntz and T. Abbott and Abdalla, {F. B.} and S. Allam and R. Armstrong and M. Banerji and Bauer, {A. H.} and A. Benoit-L{\'e}vy and E. Bertin and D. Brooks and E. Buckley-Geer and Burke, {D. L.} and D. Capozzi and {Carnero Rosell}, A. and {Carrasco Kind}, M. and J. Carretero and Castander, {F. J.} and M. Crocce and Cunha, {C. E.} and D'Andrea, {C. B.} and {Da Costa}, {L. N.} and Depoy, {D. L.} and S. Desai and Diehl, {H. T.} and Dietrich, {J. P.} and P. Doel and {Fausti Neto}, A. and E. Fernandez and Finley, {D. A.} and B. Flaugher and P. Fosalba and Gerdes, {D. W.} and Gruendl, {R. A.} and G. Gutierrez and K. Honscheid and James, {D. J.} and K. Kuehn and N. Kuropatkin and O. Lahav and Li, {T. S.} and M. Lima and Maia, {M. A.G.} and M. March and P. Martini and P. Melchior and Miller, {C. J.} and R. Miquel and Mohr, {J. J.} and Nichol, {R. C.} and B. Nord and R. Ogando and Plazas, {A. A.} and K. Reil and Romer, {A. K.} and A. Roodman and M. Sako and E. Sanchez and V. Scarpine and M. Schubnell and I. Sevilla-Noarbe and Smith, {R. C.} and M. Soares-Santos and F. Sobreira and E. Suchyta and Swanson, {M. E.C.}",

year = "2016",

month = jul,

day = "6",

doi = "10.1103/PhysRevD.94.022002",

language = "English",

volume = "94",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "2",

}

Becker, MR, Troxel, MA, Maccrann, N, Krause, E, Eifler, TF, Friedrich, O, Nicola, A, Refregier, A, Amara, A, Bacon, D, Bernstein, GM, Bonnett, C, Bridle, SL, Busha, MT, Chang, C, Dodelson, S, Erickson, B, Evrard, AE, Frieman, J, Gaztanaga, E, Gruen, D, Hartley, W, Jain, B, Jarvis, M, Kacprzak, T, Kirk, D, Kravtsov, A, Leistedt, B, Peiris, HV, Rykoff, ES, Sabiu, C, Sánchez, C, Seo, H, Sheldon, E, Wechsler, RH, Zuntz, J, Abbott, T, Abdalla, FB, Allam, S, Armstrong, R, Banerji, M, Bauer, AH, Benoit-Lévy, A, Bertin, E, Brooks, D, Buckley-Geer, E, Burke, DL, Capozzi, D, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, FJ, Crocce, M, Cunha, CE, D'Andrea, CB, Da Costa, LN, Depoy, DL, Desai, S, Diehl, HT, Dietrich, JP, Doel, P, Fausti Neto, A, Fernandez, E, Finley, DA, Flaugher, B, Fosalba, P, Gerdes, DW, Gruendl, RA, Gutierrez, G, Honscheid, K, James, DJ, Kuehn, K, Kuropatkin, N, Lahav, O, Li, TS, Lima, M, Maia, MAG, March, M, Martini, P, Melchior, P, Miller, CJ, Miquel, R, Mohr, JJ, Nichol, RC, Nord, B, Ogando, R, Plazas, AA, Reil, K, Romer, AK, Roodman, A, Sako, M, Sanchez, E, Scarpine, V, Schubnell, M, Sevilla-Noarbe, I, Smith, RC, Soares-Santos, M, Sobreira, F, Suchyta, E & Swanson, MEC 2016, 'Cosmic shear measurements with Dark Energy Survey Science Verification data', Physical Review D, vol. 94, núm. 2, 022002. https://doi.org/10.1103/PhysRevD.94.022002

TY - JOUR

T1 - Cosmic shear measurements with Dark Energy Survey Science Verification data

AU - Becker, M. R.

AU - Troxel, M. A.

AU - Maccrann, N.

AU - Krause, E.

AU - Eifler, T. F.

AU - Friedrich, O.

AU - Nicola, A.

AU - Refregier, A.

AU - Amara, A.

AU - Bacon, D.

AU - Bernstein, G. M.

AU - Bonnett, C.

AU - Bridle, S. L.

AU - Busha, M. T.

AU - Chang, C.

AU - Dodelson, S.

AU - Erickson, B.

AU - Evrard, A. E.

AU - Frieman, J.

AU - Gaztanaga, E.

AU - Gruen, D.

AU - Hartley, W.

AU - Jain, B.

AU - Jarvis, M.

AU - Kacprzak, T.

AU - Kirk, D.

AU - Kravtsov, A.

AU - Leistedt, B.

AU - Peiris, H. V.

AU - Rykoff, E. S.

AU - Sabiu, C.

AU - Sánchez, C.

AU - Seo, H.

AU - Sheldon, E.

AU - Wechsler, R. H.

AU - Zuntz, J.

AU - Abbott, T.

AU - Abdalla, F. B.

AU - Allam, S.

AU - Armstrong, R.

AU - Banerji, M.

AU - Bauer, A. H.

AU - Benoit-Lévy, A.

AU - Bertin, E.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Capozzi, D.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Castander, F. J.

AU - Crocce, M.

AU - Cunha, C. E.

AU - D'Andrea, C. B.

AU - Da Costa, L. N.

AU - Depoy, D. L.

AU - Desai, S.

AU - Diehl, H. T.

AU - Dietrich, J. P.

AU - Doel, P.

AU - Fausti Neto, A.

AU - Fernandez, E.

AU - Finley, D. A.

AU - Flaugher, B.

AU - Fosalba, P.

AU - Gerdes, D. W.

AU - Gruendl, R. A.

AU - Gutierrez, G.

AU - Honscheid, K.

AU - James, D. J.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Li, T. S.

AU - Lima, M.

AU - Maia, M. A.G.

AU - March, M.

AU - Martini, P.

AU - Melchior, P.

AU - Miller, C. J.

AU - Miquel, R.

AU - Mohr, J. J.

AU - Nichol, R. C.

AU - Nord, B.

AU - Ogando, R.

AU - Plazas, A. A.

AU - Reil, K.

AU - Romer, A. K.

AU - Roodman, A.

AU - Sako, M.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Sevilla-Noarbe, I.

AU - Smith, R. C.

AU - Soares-Santos, M.

AU - Sobreira, F.

AU - Suchyta, E.

AU - Swanson, M. E.C.

PY - 2016/7/6

Y1 - 2016/7/6

N2 - © 2016 American Physical Society. We present measurements of weak gravitational lensing cosmic shear two-point statistics using Dark Energy Survey Science Verification data. We demonstrate that our results are robust to the choice of shear measurement pipeline, either ngmix or im3shape, and robust to the choice of two-point statistic, including both real and Fourier-space statistics. Our results pass a suite of null tests including tests for B-mode contamination and direct tests for any dependence of the two-point functions on a set of 16 observing conditions and galaxy properties, such as seeing, airmass, galaxy color, galaxy magnitude, etc. We furthermore use a large suite of simulations to compute the covariance matrix of the cosmic shear measurements and assign statistical significance to our null tests. We find that our covariance matrix is consistent with the halo model prediction, indicating that it has the appropriate level of halo sample variance. We compare the same jackknife procedure applied to the data and the simulations in order to search for additional sources of noise not captured by the simulations. We find no statistically significant extra sources of noise in the data. The overall detection significance with tomography for our highest source density catalog is 9.7σ. Cosmological constraints from the measurements in this work are presented in a companion paper [DES, Phys. Rev. D 94, 022001 (2016).].

AB - © 2016 American Physical Society. We present measurements of weak gravitational lensing cosmic shear two-point statistics using Dark Energy Survey Science Verification data. We demonstrate that our results are robust to the choice of shear measurement pipeline, either ngmix or im3shape, and robust to the choice of two-point statistic, including both real and Fourier-space statistics. Our results pass a suite of null tests including tests for B-mode contamination and direct tests for any dependence of the two-point functions on a set of 16 observing conditions and galaxy properties, such as seeing, airmass, galaxy color, galaxy magnitude, etc. We furthermore use a large suite of simulations to compute the covariance matrix of the cosmic shear measurements and assign statistical significance to our null tests. We find that our covariance matrix is consistent with the halo model prediction, indicating that it has the appropriate level of halo sample variance. We compare the same jackknife procedure applied to the data and the simulations in order to search for additional sources of noise not captured by the simulations. We find no statistically significant extra sources of noise in the data. The overall detection significance with tomography for our highest source density catalog is 9.7σ. Cosmological constraints from the measurements in this work are presented in a companion paper [DES, Phys. Rev. D 94, 022001 (2016).].

U2 - 10.1103/PhysRevD.94.022002

DO - 10.1103/PhysRevD.94.022002

M3 - Article

SN - 2470-0010

VL - 94

JO - Physical Review D

JF - Physical Review D

IS - 2

M1 - 022002

ER -

Cosmic shear measurements with Dark Energy Survey Science Verification data

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