z-logo
open-access-imgOpen Access
Intermediate Strength Gravitational Lensing
Author(s) -
John B. Irwin
Publication year - 2005
Language(s) - English
Resource type - Reports
DOI - 10.2172/839937
Subject(s) - weak gravitational lensing , physics , strong gravitational lensing , gravitational lens , distortion (music) , gravitational lensing formalism , galaxy , astrophysics , curvature , quadrupole , optics , redshift , geometry , mathematics , amplifier , optoelectronics , cmos , atomic physics
Weak lensing is found in the correlations of shear in 104 galaxy images, strong lensing is detected by the obvious distortion of a single galaxy image, whereas intermediate lensing requires detection of less obvious curvature in several neighboring galaxies. Small impact-parameter lensing causes a sextupole distortion whose orientation is correlated with the quadrupole distortion (shear). By looking within a field for the spatial correlation of this sextupole-quadrupole correlation, an intermediate lensing regime is observed. This technique requires correction for the sextupole as well as the quadrupole content of the PSF. We remove the HST PSF and uncover intermediate lensing in the Hubble deep fields. Correlations of the type expected are found.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom