Search for gravitational radiation from the Crab pulsar

Katsunobu Oide, Hiromasa Hirakawa, and Masa-Katsu Fujimoto
Phys. Rev. D 20, 2480 – Published 15 November 1979
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Abstract

The result of a revised search for the gravitational radiation from the Crab pulsar at 60.2 Hz is presented. Cold damping was applied to a 1400-kg aluminum quadrupole antenna at room temperature. The resulting antenna system had a bandwidth increased to 0.012 Hz and a noise temperature reduced to 24 K. From the taped record of 621 h of observation, we have obtained an upper limit for the energy flux of the radiation in one of the polarization components: SG+<0.08 W/m2.

  • Received 3 July 1979

DOI:https://doi.org/10.1103/PhysRevD.20.2480

©1979 American Physical Society

Authors & Affiliations

Katsunobu Oide and Hiromasa Hirakawa

  • Department of Physics, University of Tokyo, Bunkyo, Tokyo 113, Japan

Masa-Katsu Fujimoto

  • Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan

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Issue

Vol. 20, Iss. 10 — 15 November 1979

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