Discovery of the Largest Known Lensed Images Formed by a Critically Convergent Lensing Cluster

We identify the largest known lensed images of a single spiral galaxy, lying close to the centre of the distant cluster MACS J1149.5+2223 (z = 0.544). These images cover a total area of ≃ 150 2 and are magnified ≃ 200 times. Unusually, there is very little image distortion implying the central mass distribution is almost uniform over a wide area (r ≃ 200 kpc) with a surface density equal to the critical density for lensing, corresponding to maximal lens magnification. Many fainter multiply-lensed galaxies are also uncovered by our model, outlining a very large tangential critical curve, of radius r ≃ 170 kpc, posing a potential challenge for the standard LCDM-Cosmology. Because of the uniform central mass distribution a particularly clean measurement of the mass of the brightest cluster galaxy is possible here, for which we infer stars contribute most of the mass within a limiting radius of ≃ 30 kpc, with a mass-to-light ratio of M/LB ≃ 4.5(M/L)⊙. This cluster with its uniform and central mass distribution acts analogously to a regular magnifying glass, converging light without distorting the images, resulting in the most powerful lens yet discovered for accessing the faint high-z Universe. Subject headings: gravitational lensing , galaxies: clusters: individual: MACS J1149.5+2223 , dark matter