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The number of low-mass X-ray binaries in NGC 4365 that are within 0.5" of a globular cluster and considered to be matches is 18, not 23 as mistakenly reported in the first paragraph of § 3. The correct number is used elsewhere in the above Letter. The fraction of low-mass X-ray binaries that are associated with globular clusters in NGC 4365 is indeed 40% as noted later in the same paragraph. We thank W. Lewin for alerting us to this error

Erratum: “Some Constraints on the Effect of Age and Metallicity on the Low-Mass X-Ray Binary Formation Rate” (ApJ, 589, L81 [2003])