Article (Scientific journals)
SEAGLE - I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
Mukherjee, Sampath; Koopmans, Léon V. E.; Metcalf, R. Benton et al.
2018In Monthly Notices of the Royal Astronomical Society, 479 (3), p. 4108
Peer Reviewed verified by ORBi
 

Files


Full Text
1802.06629 (1).pdf
Author preprint (3.29 MB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
gravitational lensing: strong; methods: numerical; galaxies: evolution; galaxies: formation; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies
Abstract :
[en] In this paper we introduce the SEAGLE (i.e. Simulating EAGLE LEnses) programme, which approaches the study of galaxy formation through strong gravitational lensing, using a suite of high-resolution hydrodynamic simulations, Evolution and Assembly of GaLaxies and their Environments (EAGLE) project. We introduce the simulation and analysis pipeline and present the first set of results from our analysis of early-type galaxies. We identify and extract an ensemble of simulated lens galaxies and use the GLAMER ray-tracing lensing code to create mock lenses similar to those observed in the Sloan Lens ACS Survey (SLACS) and SL2S surveys, using a range of source parameters and galaxy orientations, including observational effects such as the point spread function, pixelization, and noise levels, representative of single-orbit observations with the Hubble Space Telescope (HST) using the ACS-F814W filter. We subsequently model these mock lenses using the code LENSED, treating them in the same way as observed lenses. We also estimate the mass model parameters directly from the projected surface mass density of the simulated galaxy, using an identical mass model family. We perform a three-way comparison of all the measured quantities with real lenses. We find the average total density slope of EAGLE lenses, t=2.26 (0.25 rms) to be higher than SL2S, t = 2.16 or SLACS, t = 2.08. We find a very strong correlation between the external shear (γ) and the complex ellipticity (∊), with γ ∼ ∊/4. This correlation indicates a degeneracy in the lens mass modelling. We also see a dispersion between lens modelling and direct fitting results, indicating systematical biases.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Mukherjee, Sampath ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Origines Cosmologiques et Astrophysiques (OrCa)
Koopmans, Léon V. E.;  Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands
Metcalf, R. Benton;  Dipartimento di Fisica e Astronomia, Università di Bologna, via Gobetti 93/2, I-40129 Bologna, Italy ; Istituto Nazionale di Astrofisica (INAF) - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, via Gobetti 93/3, I-40129 Bologna, Italy
Tessore, Nicolas;  Jodrell Bank Centre for Astrophysics, University of Manchester, Alan Turing Building, Manchester M13 9PL, UK
Tortora, Crescenzo;  Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands
Schaller, Matthieu;  Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands
Schaye, Joop;  Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands
Crain, Robert A.;  Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK
Vernardos, Georgios;  Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands
Bellagamba, Fabio;  Dipartimento di Fisica e Astronomia, Università di Bologna, via Gobetti 93/2, I-40129 Bologna, Italy ; Istituto Nazionale di Astrofisica (INAF) - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, via Gobetti 93/3, I-40129 Bologna, Italy
Theuns, Tom;  Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK)
Language :
English
Title :
SEAGLE - I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
Publication date :
01 September 2018
Journal title :
Monthly Notices of the Royal Astronomical Society
ISSN :
0035-8711
eISSN :
1365-2966
Publisher :
Oxford University Press, Oxford, United Kingdom
Volume :
479
Issue :
3
Pages :
4108
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 20 January 2021

Statistics


Number of views
29 (3 by ULiège)
Number of downloads
29 (1 by ULiège)

Scopus citations®
 
24
Scopus citations®
without self-citations
9
OpenCitations
 
20

Bibliography


Similar publications



Contact ORBi