Anomaly distribution in quasar magnitudes: a test of lensing by an hypothetic Supergiant Molecular Cloud in the Galactic halo
Edmond Giraud

TL;DR
This paper investigates whether a hypothetical Supergiant Molecular Cloud in the Galactic halo could cause the observed quasar magnitude anomaly through gravitational lensing, using detailed modeling of the cloud's structure and mass.
Contribution
It introduces a fractal and clumpy lens model of a Supergiant Molecular Cloud to explain the quasar magnitude anomaly via gravitational lensing effects.
Findings
A plausible lens model requires a mass of (1.5-4.1) x 10^{10} solar masses.
The model involves a fractal cloud structure with a dimension of 1.8-2.
Complex caustic networks are formed by the clumpy cloud structure.
Abstract
An anomaly in the distribution of quasar magnitudes based on the SDSS survey, has been recently reported by Longo (2012). The angular size of this anomaly is of the order of on the sky. A low surface brightness smooth structure in -rays, coincides with the sky location and extent of the quasar anomaly, and is close to the Northern component of a pair of -ray bubbles discovered in the \sl Fermi Gamma-ray Space Telescope \rm survey. Molecular clouds are thought to be illuminated by cosmic rays. I test the hypothesis that the magnitude anomaly in the quasar distribution, is due to a lensing effect by an hypothetic Supergiant Molecular Cloud (SGMC) in the Galactic halo.A series of grid lens models are built by assuming firstly that a SGMC is a lattice with clumps of , 10 AU in size, and assuming various filling factors of the cloud, and…
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