Paul L. Schechter

The Las Campanas Redshift Survey

The Las Campanas Redshift Survey (LCRS) consists of 26418 redshifts of galaxies selected from a CCD-based catalog obtained in the

The Velocity Dispersion Function of Early‐Type Galaxies

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The Quadruple Gravitational Lens PG 1115+080: Time Delays and Models

band. The survey covers over 700 square degrees in 6 strips, each 1.5

X-Ray and Optical Flux Ratio Anomalies in Quadruply Lensed Quasars. I. Zooming in on Quasar Emission Regions

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Sizes and Temperature Profiles of Quasar Accretion Disks from Chromatic Microlensing

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The Power Spectrum of Galaxy Clustering in the Las Campanas Redshift Survey

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On the universality of microlensing in quadruple gravitational lenses

, three each in the North and South galactic caps. The median redshift in the survey is about 30000 km~s

The Las Campanas Redshift Survey galaxy—galaxy autocorrelation function

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Differential Microlensing of the Continuum and Broad Emission Lines in SDSS J0924+0219, the Most Anomalous Lensed Quasar*

. Essential features of the galaxy selection and redshift measurement methods are described and tabulated here. These details are important for subsequent analysis of the LCRS data. Two dimensional representations of the redshift distributions reveal many repetitions of voids, on the scale of about 5000 km~s

HE 0435-1223: A wide separation quadruple QSO and gravitational lens

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