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Is the Large Magellanic Cloud a Large Microlensing Cloud?

  • Authors: N. Wyn Evans and Eamonn Kerins

Evans & Kerins 2000 The Astrophysical Journal 529 917.

  • Provider: AAS Journals

Caption: Fig. 2.

Assumed evolution of detection efficiency toward the LMC with experiment lifetime T for ﹩T=2.1﹩, 6, 20, and 60 years (dashed lines). The efficiency is assumed to increase with T for longer Einstein diameter crossing times ﹩\hat{t}﹩ up to a maximum efficiency level of 0.5. The actual detection efficiency of Alcock et al. (1997a) after 2.1 years observation is shown by the solid line.

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