Published May 7, 2011
| Version v1
Journal article
Characterization of photoreceivers for LISA
- 1. NASA Goddard Space Flight Center, Code 663, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States)
Description
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.
Availability note (English)
Available from http://dx.doi.org/10.1088/0264-9381/28/9/094010Additional details
Identifiers
- DOI
- 10.1088/0264-9381/28/9/094010;
- PII
- S0264-9381(11)74472-0;
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 28
- Journal Issue
- 9
- Journal Page Range
- [9 p.]
- ISSN
- 0264-9381
- CODEN
- CQGRDG
Conference
- Title
- 8. international LISA symposium
- Dates
- 28 Jun - 2 Jul 2010
- Place
- Stanford, CA (United States)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43031609
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANTENNAS; INTERFEROMETERS; MASS; MHZ RANGE; NOISE; PHASE OSCILLATIONS; PHOTODETECTORS
- Descriptors DEC
- BEAM DYNAMICS; DYNAMICS; ELECTRICAL EQUIPMENT; EQUIPMENT; FREQUENCY RANGE; MEASURING INSTRUMENTS; MECHANICS; OSCILLATIONS