Characterization of photoreceivers for LISA

F. Guzmán Cervantes, J. Livas, R. Silverberg, E. Buchanan, R. Stebbins

Research output: Contribution to journalArticlepeer-review

26 Scopus citations


LISA will use quadrant photoreceivers as front-end devices for the phasemeter measuring the motion of drag-free test masses in both angular orientation and separation. We have set up a laboratory testbed for the characterization of photoreceivers. Some of the limiting noise sources have been identified and their contribution has been either measured or derived from the measured data. We have built a photoreceiver with a 0.5 mm diameter quadrant photodiode with an equivalent input current noise of better than 1.8 pA Hz -1/2 below 20 MHz and a 3 dB bandwidth of 34 MHz.

Original languageEnglish (US)
Article number094010
JournalClassical and Quantum Gravity
Issue number9
StatePublished - May 7 2011
Externally publishedYes

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)


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