Observations with a low-temperature, resonant mass, gravitational radiation detector

Details Observations with a low-temperature, resonant mass, gravitational radiation detector Observations with a low-temperature, resonant mass, gravitational radiation detector

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...261l..19b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 261, Oct. 1, 1982, p. L19-L22.

Statistics

34

Gravitational Wave Antennas, Low Temperature, Radiation Detectors, Brownian Movements, Calibrating, Magnetic Flux, Maxima, Signal To Noise Ratios

Scientific paper

A highly sensitive antenna's output noise level is used to establish a new observational upper limit on the flux of 1 kHz gravity wave bursts. The data employed were from 74 days of operation, and they demonstrate that the detector was being excited by pulses with non-Gaussian statistics. The absence of corresponding veto signals shows that the pulses contained only modest power at the second harmonic frequency of 1680 Hz.

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