Gravitational lensing model degeneracies: Is steepness all-important?
arXiv:astro-ph/0608496 · doi:10.1086/508798
Abstract
In gravitational lensing, steeper mass profiles generically produce longer time delays but smaller magnifications, without necessarily changing the image positions or magnification ratios between different images. This is well known. We find in this paper, however, that even if steepness is fixed, time delays can still have significant model dependence, which we attribute to shape modeling degeneracies. This conclusion follows from numerical experiments with models of 35 galaxy lenses. We suggest that varying and twisting ellipticities, features that are explored by pixelated lens models but not so far by parametric models, have an important effect on time delays.
To appear in ApJ
References in corpus (20)
- The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the fundamental plane of elliptical and lenticular galaxies
- Massive Dark-matter halos and Evolution of Early-type Galaxies to z=1
- HST STIS spectroscopy of the triple nucleus of M31: two nested disks in Keplerian rotation around a Supermassive Black Hole
- What Do Gravitational Lens Time Delays Measure?
- The Time Delays of Gravitational Lens HE0435-1223: An Early-Type Galaxy With a Rising Rotation Curve
- Lensing Degeneracies Revisited
- A portable modeler of lensed quasars
- Non-parametric reconstruction of the galaxy-lens in PG1115+080
- Pixelated Lenses and H_0 from Time-delay QSOs
- Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant
- Parameter degeneracy in models of the quadruple lens system Q2237+0305
- The Hubble time inferred from 10 time-delay lenses
- Degeneracies and scaling relations in general power-law models for gravitational lenses
- A multipole-Taylor expansion for the potential of gravitational lens MG J0414+0534
- Qualitative Theory for Lensed QSOs
- An optical time delay for the double gravitational lens system FBQ 0951+2635
- Mass-sheet degeneracy: Fundamental limit on the cluster mass reconstruction from statistical (weak) lensing
- Intrinsic Degeneracy of Gravitational Lens Time Delays: the case for a simple quadruple system in CDM cosmology
- Gravitational Lensing and the Mass Distribution of Clusters
- Time-delay quasars: scales and orders of magnitudes
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- Strong Lensing by Galaxies
- TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
- TDCOSMO. I. An exploration of systematic uncertainties in the inference of from time-delay cosmography
- Gravitational Lens Time Delays: A Statistical Assessment of Lens Model Dependences and Implications for the Global Hubble Constant
- Source-position transformation -- an approximate invariance in strong gravitational lensing
- The mass-sheet degeneracy and time-delay cosmography: Analysis of the strong lens RXJ1131-1231
- Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
- LensPerfect: Gravitational Lens Massmap Reconstructions Yielding Exact Reproduction of All Multiple Images
- A New Estimate of the Hubble Time with Improved Modeling of Gravitational Lenses
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- A Unifying Framework for Self-consistent Gravitational Lensing and Stellar Dynamics Analyses of Early-Type Galaxies
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- The Hubble constant inferred from 18 time-delay lenses
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- A generalisation of the mass-sheet degeneracy producing ring-like artefacts in the lens mass distribution
- Meso-structure in three strong-lensing systems
- Large-Scale Gravitational Lens Modeling with Bayesian Neural Networks for Accurate and Precise Inference of the Hubble Constant
- Gravitational Lens Recovery with GLASS: Measuring the mass profile and shape of a lens
- Steepened inner density profiles of group galaxies via interactions: An N-body analysis
- Golden gravitational lensing systems from the Sloan Lens ACS Survey. I. SDSS J1538+5817: one lens for two sources
- Estimating cosmological parameters from future gravitational lens surveys
- Galaxy-lens determination of : constraining density slope in the context of the mass sheet degeneracy
- The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: The Elliot Arc
- Extended lens reconstructions with Grale: exploiting time domain, substructural and weak-lensing information
- Lensing time delays as a substructure constraint: a case study with the cluster SDSS~J1004+4112
- Lensed Image Angles: New Statistical Evidence for Substructure
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- TDCOSMO VIII: A key test of systematics in the hierarchical method of time-delay cosmography
- Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
- Lessons from a blind study of simulated lenses: image reconstructions do not always reproduce true convergence
- Unveiling the Universe with Emerging Cosmological Probes
- Separating inner and outer contributions in gravitational lenses using the perturbative method
- The Hubble constant from galaxy lenses: impacts of triaxiality and model degeneracies
- TDCOSMO: XX. WFI2033--4723, the First Quadruply-Imaged Quasar Modeled with JWST Imaging
- What Multiple Images Say About the Large-Scale Mass Maps of Galaxy Clusters
- Along the Primary Curve: Simultaneous Source and Lens Reconstruction of Bright Arcs in Cluster Lenses
- Which gravitational lensing degeneracies are broken in wave-optics?
- Minimal lensing solutions in the singular perturbative approach
- A Taxonomy for the Configurations of Quadruply Lensed Quasars
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- A Fuzzy Situation Eased: Cold Dark Matter with Multipoles Can Explain The Double Radio Quad Lens HS 0810+2554