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/10.1088/0264-9381/28/9/094010

Additional 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