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Weak gravitational lensing is considered to be one of the most powerful tools to study the mass and the mass distribution of galaxy clusters. However, weak lensing mass reconstructions are plagued by the so-called mass-sheet degeneracy--the…

天体物理学 · 物理学 2010-12-16 M. Bradac , M. Lombardi , P. Schneider

Weak gravitational lensing is considered to be one of the most powerful tools to study the mass and the mass distribution of galaxy clusters. However, weak lensing mass reconstructions are plagued by the so-called mass-sheet degeneracy--the…

天体物理学 · 物理学 2007-05-23 M. Bradac , M. Lombardi , P. Schneider

Gravitational lensing has long been considered as a valuable tool to determine the total mass of galaxy clusters. The shear profile as inferred from the statistics of ellipticity of background galaxies allows to probe the cluster…

宇宙学与河外天体物理 · 物理学 2016-09-21 Vincenzo F. Cardone , Martina Vicinanza , Xinzhong Er , Roberto Maoli , Roberto Scaramella

The mass-sheet degeneracy is a well-known problem in gravitational lensing which limits our capability to infer astrophysical lens properties or cosmological parameters from observations. As the number of gravitational wave observations…

宇宙学与河外天体物理 · 物理学 2021-07-07 Paolo Cremonese , Jose María Ezquiaga , Vincenzo Salzano

We make a number of comments regarding modeling degeneracies in strong lensing measurements of the Hubble parameter $H_0$. The first point concerns the impact of weak lensing associated with different segments of the line of sight. We show…

宇宙学与河外天体物理 · 物理学 2022-10-25 Luca Teodori , Kfir Blum , Emanuele Castorina , Marko Simonović , Yotam Soreq

Weak gravitational lensing is considered to be one of the most powerful tools to study the mass and the mass distribution of galaxy clusters. However, the mass-sheet degeneracy transformation has limited its success. We present a novel…

天体物理学 · 物理学 2007-05-23 M. Bradac , P. Schneider , M. Lombardi , T. Erben

The Hubble constant ($H_0$), a crucial parameter in cosmology, quantifies the expansion rate of the universe so its precise measurement is important to understand the fundamental dynamics of our evolving universe. One of the major…

宇宙学与河外天体物理 · 物理学 2024-07-29 Narayan Khadka , Simon Birrer , Alexie Leauthaud , Holden Nix

Strong gravitational lensing is regarded as the most precise technique to measure the mass in the inner region of galaxies or galaxy clusters. In particular, the mass within one Einstein radius can be determined with an accuracy of order of…

宇宙学与河外天体物理 · 物理学 2017-05-10 Sandra Unruh , Peter Schneider , Dominique Sluse

Strong gravitational lensing has to deal with many modeling degeneracies, the most notable being the Mass Sheet Degeneracy (MSD). We review the MSD when one needs to model more lens planes, each one with an internal mass sheet. We take into…

星系天体物理 · 物理学 2026-04-03 Luca Teodori

The inversion of a gravitational lens system is, as is well known, plagued by the so-called mass-sheet degeneracy: one can always rescale the density distribution of the lens and add a constant-density mass-sheet such that the, also…

天体物理学 · 物理学 2009-11-13 J. Liesenborgs , S. De Rijcke , H. Dejonghe , P. Bekaert

The inversion of gravitational lens systems is hindered by the fact that multiple mass distributions are often equally compatible with the observed properties of the images. Besides using clear examples to illustrate the effect of the…

宇宙学与河外天体物理 · 物理学 2015-06-05 J. Liesenborgs , S. De Rijcke

The light travel time differences in strong gravitational lensing systems allows an independent determination of the Hubble constant. This method has been successfully applied to several lens systems. The formally most precise measurements…

宇宙学与河外天体物理 · 物理学 2015-06-16 Peter Schneider , Dominique Sluse

Time-delay cosmography with gravitationally lensed quasars plays an important role in anchoring the absolute distance scale and hence measuring the Hubble constant, $H_{0}$, independent of traditional distance ladder methodology. A current…

宇宙学与河外天体物理 · 物理学 2021-08-04 Geoff C. -F. Chen , Christopher D. Fassnacht , Sherry H. Suyu , Akın Yıldırım , Eiichiro Komatsu , Jose Luis Bernal

Gravitational lensing offers a competitive method to measure $H_0$ with the goal of 1% precision. A major obstacle comes in the form of lensing degeneracies, such as the mass sheet degeneracy (MSD), which make it possible for a family of…

宇宙学与河外天体物理 · 物理学 2020-12-01 Matthew R. Gomer , Liliya L. R. Williams

In strong gravitational lens systems, the light bending is usually dominated by one main galaxy, but may be affected by other mass along the line of sight (LOS). Shear and convergence can be used to approximate the contributions from less…

宇宙学与河外天体物理 · 物理学 2014-09-09 Curtis McCully , Charles R. Keeton , Kenneth C. Wong , Ann I. Zabludoff

This paper shows that the mass-sheet degeneracy and other degeneracies in lensing have simple geometrical interpretations: they are mostly rescalings of the arrival-time surface. Different degeneracies appear in Local Group lensing and in…

天体物理学 · 物理学 2009-10-31 Prasenjit Saha

This study introduces an innovative framework aimed at overcoming the ongoing issue of mass-sheet degeneracy (MSD) in time-delay cosmography by incorporating observations of both gravitationally lensed and unlensed Type Ia supernovae (SNe…

宇宙学与河外天体物理 · 物理学 2026-03-27 Xiaolei Li , Kai Liao , Xuheng Ding

In gravitational lensing, the Mass-Sheet Transformation (MST)-or mass-sheet degeneracy-leaves image positions unchanged while scaling magnifications and time delays. The transformation scales the lens mass distribution and superposes a…

宇宙学与河外天体物理 · 物理学 2026-01-06 Marc V. Gorenstein

The unprecedented amount and the excellent quality of lensing data that the upcoming ground- and space-based surveys will produce represent a great opportunity to shed light on the questions that still remain unanswered concerning our…

宇宙学与河外天体物理 · 物理学 2021-01-27 Carolina Parroni , Edouard Tollet , Vincenzo F. Cardone , Roberto Maoli , Roberto Scaramella

Attempts to constrain the Hubble constant using the strong gravitational lens system Q0957+561 are limited by systematic uncertainties in the mass model, since the time delay is known very precisely. One important systematic effect is the…

宇宙学与河外天体物理 · 物理学 2011-02-11 R. Nakajima , G. M. Bernstein , R. Fadely , C. R. Keeton , T. Schrabback
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