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  Characterization of photoreceivers for LISA

Guzman Cervantes, F., Livas, J., Silverberg, R., Buchanan, E., & Stebbins, R. (2011). Characterization of photoreceivers for LISA. Classical and quantum gravity, 28(9): 094010. doi:10.1088/0264-9381/28/9/094010.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-4174-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-4175-3
Genre: Journal Article

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Guzman Cervantes, F.1, Author              
Livas, J., Author
Silverberg, R., Author
Buchanan, E., Author
Stebbins, R., Author
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              

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 Abstract: 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.

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 Dates: 2011
 Publication Status: Published in print
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 Identifiers: DOI: 10.1088/0264-9381/28/9/094010
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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 28 (9) Sequence Number: 094010 Start / End Page: - Identifier: ISSN: 0264-9381
CoNE: /journals/resource/954925513480_1