Astrometric Interferometry
Abstract
Astrometry is a powerful technique in astrophysics to measure three-dimensional positions of stars and other astrophysical objects, including exoplanets and the gravitational influence they have on each other. Interferometric astrometry is presented here as just one in a suite of powerful astrometric techniques, which include space-based, seeing-limited and wide-angle adaptive optics techniques. Fundamental limits are discussed, demonstrating that even ground-based techniques have the capability for astrometry at the single micro-arcsecond level, should sufficiently sophisticated instrumentation be constructed for both the current generation of single telescopes and long-baseline optical interferometers.
Cite
@article{arxiv.1812.02926,
title = {Astrometric Interferometry},
author = {Michael J. Ireland and Julien Woillez},
journal= {arXiv preprint arXiv:1812.02926},
year = {2018}
}
Comments
28 pages, 10 figures. Chapter to appear in 2019 in The WSPC Handbook of Astronomical Instrumentation, Volume 3, UV, Optical & IR Instrumentation: Part 2. Edited by David N. Burrows