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Detecting First‐Star Lyα Spheres through Gravitational Telescopes

  • Authors: Guoliang Li, Pengjie Zhang, and Xuelei Chen

Li, Zhang, & Chen 2007 The Astrophysical Journal 666 45.

  • Provider: AAS Journals

Caption: Fig. 2.

Optical depth as a function of magnification. Different colors correspond to different source sizes. The optical depth for μ ≥ 2 is virtually independent of source size. This is because the region with μ ≥ 2 in the source plane is much larger than the size of the caustics or the source. Hence, the cross section for μ ≥ 2 is dominated by the low‐magnification region, and the optical depth is almost the same for point sources and finite sources.

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