Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map

C. Chang; A. Pujol; B. Mawdsley; D. Bacon; J. Elvin-Poole; P. Melchior; A. Kovács; B. Jain; B. Leistedt; T. Giannantonio; A. Alarcon; E. Baxter; K. Bechtol; M. R. Becker; A. Benoit-Lévy; G. M. Bernstein; C. Bonnett; M. T. Busha; A. Carnero Rosell; F. J. Castander; R. Cawthon; L. N. da Costa; C. Davis; J. De Vicente; J. DeRose; A. Drlica-Wagner; P. Fosalba; M. Gatti; E. Gaztanaga; D. Gruen; J. Gschwend; W. G. Hartley; B. Hoyle; E. M. Huff; M. Jarvis; N. Jeffrey; T. Kacprzak; H. Lin; N. MacCrann; M. A.G. Maia; R. L.C. Ogando; J. Prat; M. M. Rau; R. P. Rollins; A. Roodman; E. Rozo; E. S. Rykoff; S. Samuroff; C. Sánchez; I. Sevilla-Noarbe; E. Sheldon; M. A. Troxel; T. N. Varga; P. Vielzeuf; V. Vikram; R. H. Wechsler; J. Zuntz; T. M.C. Abbott; F. B. Abdalla; S. Allam; J. Annis; E. Bertin; D. Brooks; E. Buckley-Geer; D. L. Burke; M. Carrasco Kind; J. Carretero; M. Crocce; C. E. Cunha; C. B. D'Andrea; S. Desai; H. Diehl; J. P. Dietrich; P. Doel; J. Estrada; A. Fausti Neto; E. Fernandez; B. Flaugher; J. Frieman; J. García-Bellido; R. A. Gruendl; G. Gutierrez; K. Honscheid; D. J. James; T. Jeltema; M. W.G. Johnson; M. D. Johnson; S. Kent; D. Kirk; E. Krause; K. Kuehn; S. Kuhlmann; O. Lahav; T. S. Li; M. Lima; M. March; P. Martini; F. Menanteau; R. Miquel; J. J. Mohr

doi:10.1093/mnras/stx3363

Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map

C. Chang, A. Pujol, B. Mawdsley, D. Bacon, J. Elvin-Poole, P. Melchior, A. Kovács, B. Jain, B. Leistedt, T. Giannantonio, A. Alarcon, E. Baxter, K. Bechtol, M. R. Becker, A. Benoit-Lévy, G. M. Bernstein, C. Bonnett, M. T. Busha, A. Carnero Rosell, F. J. CastanderR. Cawthon, L. N. da Costa, C. Davis, J. De Vicente, J. DeRose, A. Drlica-Wagner, P. Fosalba, M. Gatti, E. Gaztanaga, D. Gruen, J. Gschwend, W. G. Hartley, B. Hoyle, E. M. Huff, M. Jarvis, N. Jeffrey, T. Kacprzak, H. Lin, N. MacCrann, M. A.G. Maia, R. L.C. Ogando, J. Prat, M. M. Rau, R. P. Rollins, A. Roodman, E. Rozo, E. S. Rykoff, S. Samuroff, C. Sánchez, I. Sevilla-Noarbe, E. Sheldon, M. A. Troxel, T. N. Varga, P. Vielzeuf, V. Vikram, R. H. Wechsler, J. Zuntz, T. M.C. Abbott, F. B. Abdalla, S. Allam, J. Annis, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, M. Carrasco Kind, J. Carretero, M. Crocce, C. E. Cunha, C. B. D'Andrea, S. Desai, H. Diehl, J. P. Dietrich, P. Doel, J. Estrada, A. Fausti Neto, E. Fernandez, B. Flaugher, J. Frieman, J. García-Bellido, R. A. Gruendl, G. Gutierrez, K. Honscheid, D. J. James, T. Jeltema, M. W.G. Johnson, M. D. Johnson, S. Kent, D. Kirk, E. Krause, K. Kuehn, S. Kuhlmann, O. Lahav, T. S. Li, M. Lima, M. March, P. Martini, F. Menanteau, R. Miquel, J. J. Mohr

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© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We construct the largest curved-sky galaxy weak lensing mass map to date from the DES firstyear (DES Y1) data. The map, about 10 times larger than the previous work, is constructed over a contiguous ≈1500 deg2, covering a comoving volume of ≈10 Gpc3. The effects of masking, sampling, and noise are tested using simulations. We generate weak lensing maps from two DES Y1 shear catalogues, METACALIBRATION and IM3SHAPE, with sources at redshift 0.2 < z < 1.3, and in each of four bins in this range. In the highest signal-to-noise map, the ratio between the mean signal to noise in the E-mode map and the B-mode map is ~1.5 (~2) when smoothed with a Gaussian filter of sG = 30 (80) arcmin. The second and third moments of the convergence κ in the maps are in agreement with simulations. We also find no significant correlation of κ with maps of potential systematic contaminants. Finally, we demonstrate two applications of the mass maps: (1) cross-correlation with different foreground tracers of mass and (2) exploration of the largest peaks and voids in the maps.

Idioma original	Anglès
Pàgines (de-a)	3165-3190
Revista	Monthly Notices of the Royal Astronomical Society
Volum	475
Número	3
DOIs	https://doi.org/10.1093/mnras/stx3363
Estat de la publicació	Publicada - 1 d’abr. 2018

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10.1093/mnras/stx3363

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https://www.scopus.com/pages/publications/85042408618

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Chang, C., Pujol, A., Mawdsley, B., Bacon, D., Elvin-Poole, J., Melchior, P., Kovács, A., Jain, B., Leistedt, B., Giannantonio, T., Alarcon, A., Baxter, E., Bechtol, K., Becker, M. R., Benoit-Lévy, A., Bernstein, G. M., Bonnett, C., Busha, M. T., Rosell, A. C., ... Mohr, J. J. (2018). Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map. Monthly Notices of the Royal Astronomical Society, 475(3), 3165-3190. https://doi.org/10.1093/mnras/stx3363

@article{d188f89a7e3a459a9e2fee5e1a8299b1,

title = "Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map",

abstract = "{\textcopyright} 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We construct the largest curved-sky galaxy weak lensing mass map to date from the DES firstyear (DES Y1) data. The map, about 10 times larger than the previous work, is constructed over a contiguous ≈1500 deg2, covering a comoving volume of ≈10 Gpc3. The effects of masking, sampling, and noise are tested using simulations. We generate weak lensing maps from two DES Y1 shear catalogues, METACALIBRATION and IM3SHAPE, with sources at redshift 0.2 < z < 1.3, and in each of four bins in this range. In the highest signal-to-noise map, the ratio between the mean signal to noise in the E-mode map and the B-mode map is \textasciitilde{}1.5 (\textasciitilde{}2) when smoothed with a Gaussian filter of sG = 30 (80) arcmin. The second and third moments of the convergence κ in the maps are in agreement with simulations. We also find no significant correlation of κ with maps of potential systematic contaminants. Finally, we demonstrate two applications of the mass maps: (1) cross-correlation with different foreground tracers of mass and (2) exploration of the largest peaks and voids in the maps.",

keywords = "Dark matter, Gravitational lensing: weak, Surveys",

author = "C. Chang and A. Pujol and B. Mawdsley and D. Bacon and J. Elvin-Poole and P. Melchior and A. Kov{\'a}cs and B. Jain and B. Leistedt and T. Giannantonio and A. Alarcon and E. Baxter and K. Bechtol and Becker, \{M. R.\} and A. Benoit-L{\'e}vy and Bernstein, \{G. M.\} and C. Bonnett and Busha, \{M. T.\} and Rosell, \{A. Carnero\} and Castander, \{F. J.\} and R. Cawthon and \{da Costa\}, \{L. N.\} and C. Davis and \{De Vicente\}, J. and J. DeRose and A. Drlica-Wagner and P. Fosalba and M. Gatti and E. Gaztanaga and D. Gruen and J. Gschwend and Hartley, \{W. G.\} and B. Hoyle and Huff, \{E. M.\} and M. Jarvis and N. Jeffrey and T. Kacprzak and H. Lin and N. MacCrann and Maia, \{M. A.G.\} and Ogando, \{R. L.C.\} and J. Prat and Rau, \{M. M.\} and Rollins, \{R. P.\} and A. Roodman and E. Rozo and Rykoff, \{E. S.\} and S. Samuroff and C. S{\'a}nchez and I. Sevilla-Noarbe and E. Sheldon and Troxel, \{M. A.\} and Varga, \{T. N.\} and P. Vielzeuf and V. Vikram and Wechsler, \{R. H.\} and J. Zuntz and Abbott, \{T. M.C.\} and Abdalla, \{F. B.\} and S. Allam and J. Annis and E. Bertin and D. Brooks and E. Buckley-Geer and Burke, \{D. L.\} and Kind, \{M. Carrasco\} and J. Carretero and M. Crocce and Cunha, \{C. E.\} and D'Andrea, \{C. B.\} and S. Desai and H. Diehl and Dietrich, \{J. P.\} and P. Doel and J. Estrada and Neto, \{A. Fausti\} and E. Fernandez and B. Flaugher and J. Frieman and J. Garc{\'i}a-Bellido and Gruendl, \{R. A.\} and G. Gutierrez and K. Honscheid and James, \{D. J.\} and T. Jeltema and Johnson, \{M. W.G.\} and Johnson, \{M. D.\} and S. Kent and D. Kirk and E. Krause and K. Kuehn and S. Kuhlmann and O. Lahav and Li, \{T. S.\} and M. Lima and M. March and P. Martini and F. Menanteau and R. Miquel and Mohr, \{J. J.\}",

year = "2018",

month = apr,

day = "1",

doi = "10.1093/mnras/stx3363",

language = "English",

volume = "475",

pages = "3165--3190",

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

issn = "0035-8711",

number = "3",

}

Chang, C, Pujol, A, Mawdsley, B, Bacon, D, Elvin-Poole, J, Melchior, P, Kovács, A, Jain, B, Leistedt, B, Giannantonio, T, Alarcon, A, Baxter, E, Bechtol, K, Becker, MR, Benoit-Lévy, A, Bernstein, GM, Bonnett, C, Busha, MT, Rosell, AC, Castander, FJ, Cawthon, R, da Costa, LN, Davis, C, De Vicente, J, DeRose, J, Drlica-Wagner, A, Fosalba, P, Gatti, M, Gaztanaga, E, Gruen, D, Gschwend, J, Hartley, WG, Hoyle, B, Huff, EM, Jarvis, M, Jeffrey, N, Kacprzak, T, Lin, H, MacCrann, N, Maia, MAG, Ogando, RLC, Prat, J, Rau, MM, Rollins, RP, Roodman, A, Rozo, E, Rykoff, ES, Samuroff, S, Sánchez, C, Sevilla-Noarbe, I, Sheldon, E, Troxel, MA, Varga, TN, Vielzeuf, P, Vikram, V, Wechsler, RH, Zuntz, J, Abbott, TMC, Abdalla, FB, Allam, S, Annis, J, Bertin, E, Brooks, D, Buckley-Geer, E, Burke, DL, Kind, MC, Carretero, J, Crocce, M, Cunha, CE, D'Andrea, CB, Desai, S, Diehl, H, Dietrich, JP, Doel, P, Estrada, J, Neto, AF, Fernandez, E, Flaugher, B, Frieman, J, García-Bellido, J, Gruendl, RA, Gutierrez, G, Honscheid, K, James, DJ, Jeltema, T, Johnson, MWG, Johnson, MD, Kent, S, Kirk, D, Krause, E, Kuehn, K, Kuhlmann, S, Lahav, O, Li, TS, Lima, M, March, M, Martini, P, Menanteau, F, Miquel, R & Mohr, JJ 2018, 'Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map', Monthly Notices of the Royal Astronomical Society, vol. 475, núm. 3, pàg. 3165-3190. https://doi.org/10.1093/mnras/stx3363

TY - JOUR

T1 - Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map

AU - Chang, C.

AU - Pujol, A.

AU - Mawdsley, B.

AU - Bacon, D.

AU - Elvin-Poole, J.

AU - Melchior, P.

AU - Kovács, A.

AU - Jain, B.

AU - Leistedt, B.

AU - Giannantonio, T.

AU - Alarcon, A.

AU - Baxter, E.

AU - Bechtol, K.

AU - Becker, M. R.

AU - Benoit-Lévy, A.

AU - Bernstein, G. M.

AU - Bonnett, C.

AU - Busha, M. T.

AU - Rosell, A. Carnero

AU - Castander, F. J.

AU - Cawthon, R.

AU - da Costa, L. N.

AU - Davis, C.

AU - De Vicente, J.

AU - DeRose, J.

AU - Drlica-Wagner, A.

AU - Fosalba, P.

AU - Gatti, M.

AU - Gaztanaga, E.

AU - Gruen, D.

AU - Gschwend, J.

AU - Hartley, W. G.

AU - Hoyle, B.

AU - Huff, E. M.

AU - Jarvis, M.

AU - Jeffrey, N.

AU - Kacprzak, T.

AU - Lin, H.

AU - MacCrann, N.

AU - Maia, M. A.G.

AU - Ogando, R. L.C.

AU - Prat, J.

AU - Rau, M. M.

AU - Rollins, R. P.

AU - Roodman, A.

AU - Rozo, E.

AU - Rykoff, E. S.

AU - Samuroff, S.

AU - Sánchez, C.

AU - Sevilla-Noarbe, I.

AU - Sheldon, E.

AU - Troxel, M. A.

AU - Varga, T. N.

AU - Vielzeuf, P.

AU - Vikram, V.

AU - Wechsler, R. H.

AU - Zuntz, J.

AU - Abbott, T. M.C.

AU - Abdalla, F. B.

AU - Allam, S.

AU - Annis, J.

AU - Bertin, E.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Kind, M. Carrasco

AU - Carretero, J.

AU - Crocce, M.

AU - Cunha, C. E.

AU - D'Andrea, C. B.

AU - Desai, S.

AU - Diehl, H.

AU - Dietrich, J. P.

AU - Doel, P.

AU - Estrada, J.

AU - Neto, A. Fausti

AU - Fernandez, E.

AU - Flaugher, B.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Gruendl, R. A.

AU - Gutierrez, G.

AU - Honscheid, K.

AU - James, D. J.

AU - Jeltema, T.

AU - Johnson, M. W.G.

AU - Johnson, M. D.

AU - Kent, S.

AU - Kirk, D.

AU - Krause, E.

AU - Kuehn, K.

AU - Kuhlmann, S.

AU - Lahav, O.

AU - Li, T. S.

AU - Lima, M.

AU - March, M.

AU - Martini, P.

AU - Menanteau, F.

AU - Miquel, R.

AU - Mohr, J. J.

PY - 2018/4/1

Y1 - 2018/4/1

N2 - © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We construct the largest curved-sky galaxy weak lensing mass map to date from the DES firstyear (DES Y1) data. The map, about 10 times larger than the previous work, is constructed over a contiguous ≈1500 deg2, covering a comoving volume of ≈10 Gpc3. The effects of masking, sampling, and noise are tested using simulations. We generate weak lensing maps from two DES Y1 shear catalogues, METACALIBRATION and IM3SHAPE, with sources at redshift 0.2 < z < 1.3, and in each of four bins in this range. In the highest signal-to-noise map, the ratio between the mean signal to noise in the E-mode map and the B-mode map is ~1.5 (~2) when smoothed with a Gaussian filter of sG = 30 (80) arcmin. The second and third moments of the convergence κ in the maps are in agreement with simulations. We also find no significant correlation of κ with maps of potential systematic contaminants. Finally, we demonstrate two applications of the mass maps: (1) cross-correlation with different foreground tracers of mass and (2) exploration of the largest peaks and voids in the maps.

AB - © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We construct the largest curved-sky galaxy weak lensing mass map to date from the DES firstyear (DES Y1) data. The map, about 10 times larger than the previous work, is constructed over a contiguous ≈1500 deg2, covering a comoving volume of ≈10 Gpc3. The effects of masking, sampling, and noise are tested using simulations. We generate weak lensing maps from two DES Y1 shear catalogues, METACALIBRATION and IM3SHAPE, with sources at redshift 0.2 < z < 1.3, and in each of four bins in this range. In the highest signal-to-noise map, the ratio between the mean signal to noise in the E-mode map and the B-mode map is ~1.5 (~2) when smoothed with a Gaussian filter of sG = 30 (80) arcmin. The second and third moments of the convergence κ in the maps are in agreement with simulations. We also find no significant correlation of κ with maps of potential systematic contaminants. Finally, we demonstrate two applications of the mass maps: (1) cross-correlation with different foreground tracers of mass and (2) exploration of the largest peaks and voids in the maps.

KW - Dark matter

KW - Gravitational lensing: weak

KW - Surveys

UR - https://www.scopus.com/pages/publications/85042408618

U2 - 10.1093/mnras/stx3363

DO - 10.1093/mnras/stx3363

M3 - Article

SN - 0035-8711

VL - 475

SP - 3165

EP - 3190

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

Dark Energy Survey Year 1 results: Curved-sky weak lensing mass map

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