Non-parametric mass reconstruction of A1689 from strong lensing data with the Strong Lensing Analysis Package
- Author
- DIEGO, J. M1 2 ; SANDVIK, H. B3 ; PROTOPAPAS, P4 ; TEGMARK, M1 2 ; BENITEZ, N5 6 ; BROADHURST, T7
[1] MIT Center for Space Research, Cambridge, MA 02138, United States
[2] University of Pennsylvania, 209S, 33rd St. Department of Physics and Astronomy, Philadelphia, PA 19104, United States
[3] Max-Planck-Institut für A stirlphysik, 85748 Garching, Germany
[4] Harvard-Smithsmian Center for Astrophysics, 60 Graden St, Cambridge, MA 02138, United States
[5] Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, United States
[6] Instituto de Astrofisica de Andalucía (CSIC). Camino Bajo de Huítor, 24, Granada, Spain
[7] School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel - Source
Monthly Notices of the Royal Astronomical Society. 2005, Vol 362, Num 4, pp 1247-1258, 12 p ; ref : 35 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- galaxies: clusters: general methods: numerical
- Keyword (fr)
- Amas galaxies Cercle Distribution masse Dégénérescence Déplacement vers le rouge Galaxies elliptiques Incertitude Matière sombre Modèle Méthode numérique Perturbation Sous structure
- Keyword (en)
- Galaxy clusters Circle Mass distribution Degeneration Red shift Elliptical galaxies Uncertainty Dark matter Models Numerical method Disturbances Substructure
- Keyword (es)
- Circulo Incertidumbre Modelo Método numérico Subestructura
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17116379
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1111/j.1365-2966.2005.09372.x 
https://dx.doi.org/10.1111/j.1365-2966.2005.09372.x
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