Systematics in lensing reconstruction: dark matter rings in the sky?
12 páginas, 8 figuras.-- El Pdf del artículo es la versión pre-print: arXiv:1110.3979v1
| Autores: | , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2011 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/46747 |
| Acceso en línea: | http://hdl.handle.net/10261/46747 |
| Access Level: | acceso abierto |
| Palabra clave: | Cosmology: observations Gravitational lensing: weak Galaxies: clusters: general Dark matter Gravitational lensing: strong |
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Systematics in lensing reconstruction: dark matter rings in the sky?Ponente, P. P.Diego, José MaríaCosmology: observationsGravitational lensing: weakGalaxies: clusters: generalDark matterGravitational lensing: strong12 páginas, 8 figuras.-- El Pdf del artículo es la versión pre-print: arXiv:1110.3979v1[Context]: Non-parametric lensing methods are a useful way of reconstructing the lensing mass of a cluster without making assumptions about the way the mass is distributed in the cluster. These methods are particularly powerful in the case of galaxy clusters with a large number of constraints. The advantage of not assuming implicitly that the luminous matter follows the dark matter is particularly interesting in those cases where the cluster is in a non-relaxed dynamical state. On the other hand, non-parametric methods have several limitations that should be taken into account carefully. [Aims]: We explore some of these limitations and focus on their implications for the possible ring of dark matter around the galaxy cluster CL0024+17. [Methods]: We project three background galaxies through a mock cluster of known radial profile density and obtain a map for the arcs (θ map). We also calculate the shear field associated with the mock cluster across the whole field of view (3.3 arcmin). Combining the positions of the arcs and the two-direction shear, we perform an inversion of the lens equation using two separate methods, the biconjugate gradient, and the quadratic programming (QADP) to reconstruct the convergence map of the mock cluster. [Results]: We explore the space of the solutions of the convergence map and compare the radial density profiles to the density profile of the mock cluster. When the inversion matrix algorithms are forced to find the exact solution, we encounter systematic effects resembling ring structures, that clearly depart from the original convergence map. [Conclusions]: Overfitting lensing data with a non-parametric method can produce ring-like structures similar to the alleged one in CL0024.We acknowledge partial financial support from the Ministerio de Ciencia e Innovación project AYA2007-68058-C03-02. PPP acknowledges support from the Spanish Ministerio de Educación y Ciencia and CSIC for an I3P grant.Peer reviewedEDP Sciences201220122011info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501http://hdl.handle.net/10261/46747reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1051/0004-6361/201117382info:eu-repo/semantics/openAccessoai:digital.csic.es:10261/467472026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| title |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| spellingShingle |
Systematics in lensing reconstruction: dark matter rings in the sky? Ponente, P. P. Cosmology: observations Gravitational lensing: weak Galaxies: clusters: general Dark matter Gravitational lensing: strong |
| title_short |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| title_full |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| title_fullStr |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| title_full_unstemmed |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| title_sort |
Systematics in lensing reconstruction: dark matter rings in the sky? |
| dc.creator.none.fl_str_mv |
Ponente, P. P. Diego, José María |
| author |
Ponente, P. P. |
| author_facet |
Ponente, P. P. Diego, José María |
| author_role |
author |
| author2 |
Diego, José María |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Cosmology: observations Gravitational lensing: weak Galaxies: clusters: general Dark matter Gravitational lensing: strong |
| topic |
Cosmology: observations Gravitational lensing: weak Galaxies: clusters: general Dark matter Gravitational lensing: strong |
| description |
12 páginas, 8 figuras.-- El Pdf del artículo es la versión pre-print: arXiv:1110.3979v1 |
| publishDate |
2011 |
| dc.date.none.fl_str_mv |
2011 2012 2012 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 |
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article |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/46747 |
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http://hdl.handle.net/10261/46747 |
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Inglés |
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Inglés |
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http://dx.doi.org/10.1051/0004-6361/201117382 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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EDP Sciences |
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EDP Sciences |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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1869421797074534400 |
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15,81155 |