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Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space

We present new wide-field weak lensing mass maps for the Year 1 Dark Energy Survey data, generated via a forward fitting approach. This method of producing maps does not impose any prior constraints on the mass distribution to be reconstructed. The technique is found to improve the map reconstructio...

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Published in:arXiv.org 2019-05
Main Authors: Mawdsley, B, Bacon, D, Chang, C, Melchior, P, Rozo, E, Seitz, S, Jeffrey, N, Gatti, M, Gaztanaga, E, Gruen, D, Hartley, W G, Hoyle, B, Samuroff, S, Sheldon, E, Troxel, M A, Zuntz, J, Abbott, T M C, Annis, J, Bertin, E, Bridle, S L, Brooks, D, Buckley-Geer, E, Burke, D L, A Carnero Rosell, M Car- rasco Kind, Carretero, J, da Costa, L N, De Vicente, J, Desai, S, Diehl, H T, Doel, P, Evrard, A E, Flaugher, B, Fosalba, P, Frieman, J, Garcia-Bellido, J, Gerdes, D W, Gruendl, R A, Gschwend, J, Gutierrez, G, Hollowood, D L, Honscheid, K, James, D J, Jarvis, M, Jeltema, T, Kuehn, K, Kuropatkin, N, Lima, M, Maia, M A G, Marshall, J L, Miquel, R, Plazas, A A, Roodman, A, Sanchez, E, Scarpine, V, Serrano, S, Sevilla-Noarbe, I, Smith, M, Smith, R C, Sobreira, F, Suchyta, E, Swanson, M E C, Tarle, G, Tucker, D L, Vikram, V, Walker, A R
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creator Mawdsley, B
Bacon, D
Chang, C
Melchior, P
Rozo, E
Seitz, S
Jeffrey, N
Gatti, M
Gaztanaga, E
Gruen, D
Hartley, W G
Hoyle, B
Samuroff, S
Sheldon, E
Troxel, M A
Zuntz, J
Abbott, T M C
Annis, J
Bertin, E
Bridle, S L
Brooks, D
Buckley-Geer, E
Burke, D L
A Carnero Rosell
M Car- rasco Kind
Carretero, J
da Costa, L N
De Vicente, J
Desai, S
Diehl, H T
Doel, P
Evrard, A E
Flaugher, B
Fosalba, P
Frieman, J
Garcia-Bellido, J
Gerdes, D W
Gruendl, R A
Gschwend, J
Gutierrez, G
Hollowood, D L
Honscheid, K
James, D J
Jarvis, M
Jeltema, T
Kuehn, K
Kuropatkin, N
Lima, M
Maia, M A G
Marshall, J L
Miquel, R
Plazas, A A
Roodman, A
Sanchez, E
Scarpine, V
Serrano, S
Sevilla-Noarbe, I
Smith, M
Smith, R C
Sobreira, F
Suchyta, E
Swanson, M E C
Tarle, G
Tucker, D L
Vikram, V
Walker, A R
description We present new wide-field weak lensing mass maps for the Year 1 Dark Energy Survey data, generated via a forward fitting approach. This method of producing maps does not impose any prior constraints on the mass distribution to be reconstructed. The technique is found to improve the map reconstruction on the edges of the field compared to the conventional Kaiser-Squires method, which applies a direct inversion on the data; our approach is in good agreement with the previous direct approach in the central regions of the footprint. The mapping technique is assessed and verified with tests on simulations; together with the Kaiser-Squires method, the technique is then applied to data from the Dark Energy Survey Year 1 data and the differences between the two methods are compared. We also produce the first DES measurements of the convergence Minkowski functionals and compare them to those measured in simulations.
doi_str_mv 10.48550/arxiv.1905.12682
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Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mawdsley, B</au><au>Bacon, D</au><au>Chang, C</au><au>Melchior, P</au><au>Rozo, E</au><au>Seitz, S</au><au>Jeffrey, N</au><au>Gatti, M</au><au>Gaztanaga, E</au><au>Gruen, D</au><au>Hartley, W G</au><au>Hoyle, B</au><au>Samuroff, S</au><au>Sheldon, E</au><au>Troxel, M A</au><au>Zuntz, J</au><au>Abbott, T M C</au><au>Annis, J</au><au>Bertin, E</au><au>Bridle, S L</au><au>Brooks, D</au><au>Buckley-Geer, E</au><au>Burke, D L</au><au>A Carnero Rosell</au><au>M Car- rasco Kind</au><au>Carretero, J</au><au>da Costa, L N</au><au>De Vicente, J</au><au>Desai, S</au><au>Diehl, H T</au><au>Doel, P</au><au>Evrard, A E</au><au>Flaugher, B</au><au>Fosalba, P</au><au>Frieman, J</au><au>Garcia-Bellido, J</au><au>Gerdes, D W</au><au>Gruendl, R A</au><au>Gschwend, J</au><au>Gutierrez, G</au><au>Hollowood, D L</au><au>Honscheid, K</au><au>James, D J</au><au>Jarvis, M</au><au>Jeltema, T</au><au>Kuehn, K</au><au>Kuropatkin, N</au><au>Lima, M</au><au>Maia, M A G</au><au>Marshall, J L</au><au>Miquel, R</au><au>Plazas, A A</au><au>Roodman, A</au><au>Sanchez, E</au><au>Scarpine, V</au><au>Serrano, S</au><au>Sevilla-Noarbe, I</au><au>Smith, M</au><au>Smith, R C</au><au>Sobreira, F</au><au>Suchyta, E</au><au>Swanson, M E C</au><au>Tarle, G</au><au>Tucker, D L</au><au>Vikram, V</au><au>Walker, A R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space</atitle><jtitle>arXiv.org</jtitle><date>2019-05-29</date><risdate>2019</risdate><eissn>2331-8422</eissn><abstract>We present new wide-field weak lensing mass maps for the Year 1 Dark Energy Survey data, generated via a forward fitting approach. This method of producing maps does not impose any prior constraints on the mass distribution to be reconstructed. The technique is found to improve the map reconstruction on the edges of the field compared to the conventional Kaiser-Squires method, which applies a direct inversion on the data; our approach is in good agreement with the previous direct approach in the central regions of the footprint. The mapping technique is assessed and verified with tests on simulations; together with the Kaiser-Squires method, the technique is then applied to data from the Dark Energy Survey Year 1 data and the differences between the two methods are compared. We also produce the first DES measurements of the convergence Minkowski functionals and compare them to those measured in simulations.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1905.12682</doi><oa>free_for_read</oa></addata></record>
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identifier EISSN: 2331-8422
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subjects Dark energy
Mapping
Mass distribution
Production methods
Sky surveys (astronomy)
title Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
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