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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. 4.

The 95% lower limit on the discriminatory power, ﹩D_{95}﹩, of current surveys (solid line) and the proposed next‐generation survey, "SuperMACHO," of Stubbs (1998) as a function of observation epoch. We assume a starting date of 1992.5 for the current surveys and 2001 for SuperMACHO. The limits shown are for the halo model with ﹩f_{h}=0.1﹩ and ﹩m_{\mathrm{dark}\,}=0.5\,M_{\odot }﹩.

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