Here, we report on the first detection of
weak lensing magnification with a new, independent technique using the distribution of galaxy sizes and magnitudes.
Not exact matches
Abstract: We derive an accurate mass distribution of the galaxy cluster MACS J1206.2 - 0847 (z = 0.439) from a combined
weak -
lensing distortion, magnification, and strong - lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) p
lensing distortion,
magnification, and strong -
lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) p
lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster
Lensing And Supernova survey with Hubble (CLASH) p
Lensing And Supernova survey with Hubble (CLASH) program.
We find good agreement in the regions of ove... ▽ More We derive an accurate mass distribution of the galaxy cluster MACS J1206.2 - 0847 (z = 0.439) from a combined
weak -
lensing distortion, magnification, and strong - lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) p
lensing distortion,
magnification, and strong -
lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) p
lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster
Lensing And Supernova survey with Hubble (CLASH) p
Lensing And Supernova survey with Hubble (CLASH) program.
We present the magnific... ▽ More
Weak lensing is commonly measured using shear through galaxy ellipticities, or using the effect of
magnification bias on galaxy number densities.