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We describe the techniques used in pulsar timing observations, and show howthese observations may be applied to tests of strong-field general relativityfor double-neutron-star binary systems. We describe the tests of GR resultingfrom the PSRs B1913+16 and B1534+12 systems. For the latter pulsar, 5"Post-Keplerian" timing parameters are measurable, including the orbital periodderivative and the two Shapiro delay parameters.Comment: Talk at Marcel-Grossmann meeting IX, Rome, 2000, to be published by  World Scientific, 2 pages, no figure

PULSAR TIMING OBSERVATIONS AND TESTS OF GENERAL RELATIVITY IN DOUBLE-NEUTRON-STAR BINARIES