QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at z∼0.7
| Autor: | Federico Bianchini, Mattia Negrello, Laura Bonavera, Jesús Daniel Santos, F. J. de Cos Juez, Sergio Luis Suárez Gómez, Andrea Lapi, E. Díez Alonso, J. González-Nuevo |
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| Jazyk: | angličtina |
| Rok vydání: | 2019 |
| Předmět: |
Physics
QSOS Cosmology and Nongalactic Astrophysics (astro-ph.CO) 010308 nuclear & particles physics gravitational lensing FOS: Physical sciences Magnification Astronomy and Astrophysics Astrophysics weak gravitational lensing 01 natural sciences Measure (mathematics) Galaxy Gravitation weak gravitational lensing galaxy surveys gravitational lensing Gravitational lens Settore FIS/05 - Astronomia e Astrofisica 0103 physical sciences Cluster (physics) Halo galaxy surveys 010303 astronomy & astrophysics Astrophysics - Cosmology and Nongalactic Astrophysics |
| Popis: | Magnification bias is a gravitational lensing effect that is normally overlooked because it is considered sub-optimal in comparison with the lensing shear. Thanks to the demonstrated optimal characteristics of the sub-millimetre galaxies (SMGs) for lensing analysis, in this work we were able to measure the magnification bias produced by a sample of QSOs acting as lenses, $0.2 13.6_{-0.4}^{+0.9}$, also confirmed by the mass density profile analysis ($M_{200c}\sim 10^{14} M_\odot$). These mass values indicate that we are observing the lensing effect of a cluster size halo signposted by the QSOs, as in previous studies of the magnification bias. Moreover, we were able to estimate the lensing convergence, $\kappa(\theta)$, for our magnification bias measurements down to a few kpcs. The derived mass density profile is in good agreement with a Navarro-Frank-White (NFW) profile. We also attempt an estimation of the halo mass and the concentration parameters, obtaining $M_{NFW}=1.0^{+0.4}_{-0.2}\times10^{14} M_\odot$ and $C=3.5_{-0.3}^{+0.5}$. This concentration value is rather low and it would indicate that the cluster halos around these QSOs are unrelaxed. However, higher concentration values still provides a compatible fit to the data. Comment: 30 pages, 8 figures, JCAP accepted |
| Databáze: | OpenAIRE |
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