Paper
16 November 1982 Methods Of Photoelectric Astrometry
Laurence W. Fredrick, Charles D. Smith
Author Affiliations +
Abstract
The idea of a photoelectric technique applied to differential astrometry has been around for about a decade. When developed such instruments promise increased accuracy and speed. Using linear detectors they can determine relative magnitudes and colors of all stars in the field at the same time that the relative positions are measured. Three such instruments have been proposed and have been developed to various degrees. These instruments and several variants will be reviewed. The current status of one instrument employing a rotating Ronchi linear grid, called the AMAS, will be discussed in detail. An accuracy of 5 μm in position is achieved routinely and proposed improvements project an improvement of a factor of ten to 0.5 μm. At this point the accuracy will be "seeing" limited and further improvement will be at the expense of observing time. The present instrument is sky limited at a magnitude of 11.5(V). A very minor change will increase this limit to 15.5(V) using two minute integration periods.
© (1982) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Laurence W. Fredrick and Charles D. Smith "Methods Of Photoelectric Astrometry", Proc. SPIE 0331, Instrumentation in Astronomy IV, (16 November 1982); https://doi.org/10.1117/12.933487
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Astronomy

Sensors

Ronchi rulings

Modulation

Stellar astronomy

Microchannel plates

RELATED CONTENT

Status of the STUDIO UV balloon mission and platform
Proceedings of SPIE (December 13 2020)
Angular Resolution Requirements For Orbital Astronomy
Proceedings of SPIE (March 24 1970)
Six years in orbit the MCP detectors aboard the...
Proceedings of SPIE (August 28 1998)
Photoelastic-Modulator Polarimeters In Astronomy
Proceedings of SPIE (May 17 1982)
Very High Resolution Camera For The 3.6m On Mauna Kea
Proceedings of SPIE (January 09 1984)

Back to Top