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The Pulkovo Compilation of Radial Velocities (PCRV) has been made to studythe stellar kinematics in the local spiral arm. The PCRV contains weighted meanabsolute radial velocities for 35 495 Hipparcos stars of various spectral typesand luminosity classes over the entire celestial sphere mainly within 500 pc ofthe Sun. The median accuracy of the radial velocities obtained is 0.7 kms$^{-1}$. Results from 203 publications were used in the catalogue. Four ofthem were used to improve the radial velocities of standard stars from the IAUlist. The radial velocities of 155 standard stars turned out to be constantwithin 0.3 km s$^{-1}$. These stars were used to analyze 47 768 mean radialvelocities for 37 200 stars from 12 major publications ($\sim80\%$ of all thedata used). Zero-point discrepancies and systematic dependences on radialvelocity, $(B-V)$ color index, right ascension, and declination were found inradial velocity differences of the form "publication minus IAU list ofstandards". These discrepancies and dependences were approximated and takeninto account when calculating the weighted mean radial velocities. 1128 starswhose independent radial-velocity determinations were available at least inthree of these publications and agreed within 3 km s$^{-1}$ were chosen as thework list of secondary standards. Radial-velocity differences of the form"publication minus list of secondary standards" were used by analogy to correctthe zero points and systematic dependences in the radial velocities from 33more publications (~13\% of the data used). In addition, the radial velocitiesfrom 154 minor publications ($\sim7\%$ of the data used) pertaining towell-known instruments were used without any corrections.

Pulkovo Compilation of Radial Velocities for 35495 Hipparcos Stars in a Common System