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Event Rate and Einstein Time Evaluation in Pixel Microlensing

  • Authors: Edward A. Baltz and Joseph Silk

Baltz & Silk 2000 The Astrophysical Journal 530 578.

  • Provider: AAS Journals

Caption: Fig. 6.

Contours of constant optical depth to the disk of M31. These are given in (dimensionless) units of ﹩10^{-6}﹩. The isophotes (thick lines) are taken from Hodge & Kennicutt (1982), and are 19, 20, 21, 22, 23, 24, and 25 B mag arcsec−2. The rectangular boxes show the field of view of the CFHT 12k CCD, centered on M31 and aligned along both the major and minor axes.

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