Nominal frequency allocation plan for LISA
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Engineering topics
Publications and source records attributed to Tinto, M..
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We present a procedure for computing LISA's sensitivity to gravitational radiation.
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Doppler tracking experiments using the earth and a distant spacecraft as separated test masses have been used for gravitational wave searches in the low-frequency band. Here we describe the experiment, including the transfer functions of the signals and noises to the Doppler observable, and present the noise statistics and compare them with the pre-experiment noise budget.
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The first in-flight Doppler tracking measurements performed by LISA will be used to assess its detector performance.
LISA can be considered as six proof masses, pairwise Doppler tracked with one-way optical links.
The detection of gravitational radiation is one of the most challenging efforts in the physics of this century. A successful observation will not only represent a great triumph in experimental physics, but will also provide a new observational tool for obtaining better and deeper understanding about its sources, as well as a unique test of the proposed relativistic theories of gravity.
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LISA is a proposed space mission which will use coherent laser beams exchanged between three remote spacecraft, to detect and study low-frequency cosmic gravitational radiation.
LISA (Laser Interferometer Space Antenna) is a proposed mission which will use coherent laser beams exchanged between three remote spacecraft to detect and study low-frequency cosmic gravitational radiation.