The commissioning of LIGO required the mitigation of technical noise couplings to the Gravitational Wave readout. Of particular interest were RF oscillator Phase Noise and Thermal Compensation Laser Intensity Noise. Both couplings were larger than anticipated.
© 2007 APS
You do not have subscription access to this journal. Citation lists with outbound citation links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.
Contact your librarian or system administrator
Login to access OSA Member Subscription