Share Email Print
cover

Proceedings Paper

Near-infrared astrometry of star clusters with different flavors of adaptive optics and HST
Author(s): Jessica R. Lu; Benoit Neichel; Jay Anderson; Evan Sinukoff; Matthew W. Hosek; Andrea M. Ghez; Francois Rigaut
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

High-precision infrared astrometry is a powerful tool for the study of resolved stellar populations throughout our Galaxy. We highlight two particular science cases that require precise infrared astrometry: (1) measuring the initial mass function in massive young clusters throughout the MilkyWay and (2) finding isolated black holes that photometrically and astrometrically lens background bulge stars. Using astrometric results from these science cases, we perform a comparative analysis of the infrared astrometric capabilities from the Keck single-conjugate adaptive optics (AO) system, the Gemini multi-conjugate AO system, and the Hubble WFC3IR instrument. For the most crowded fields and a small region of interest, we show that Keck's single-conjugate AO system and the well-characterized NIRC2 instrument produce the highest astrometric precision at ~150 μas. However, for targets that cover a wider field of view, both the Gemini South AO Imager (GSAOI) and HST WFC3IR should be considered carefully. GSAOI currently delivers lower astrometric precision than HST WFC3IR for a given integration time; but, programs that require more frequent astrometric measurements over longer periods of time may benefit from the higher availability and possibly longer lifetime of GSAOI.

Paper Details

Date Published: 21 July 2014
PDF: 13 pages
Proc. SPIE 9148, Adaptive Optics Systems IV, 91480B (21 July 2014); doi: 10.1117/12.2057241
Show Author Affiliations
Jessica R. Lu, Institute for Astronomy, Univ. of Hawai'i (United States)
Benoit Neichel, Lab. d'Astrophysique de Marseille, CNRS, Aix Marseille Univ. (France)
Jay Anderson, Space Telescope Science Institute (United States)
Evan Sinukoff, Institute for Astronomy, Univ. of Hawai'i (United States)
Matthew W. Hosek, Institute for Astronomy, Univ. of Hawai'i (United States)
Andrea M. Ghez, Univ. of California, Los Angeles (United States)
Francois Rigaut, The Australian National Univ. (Australia)


Published in SPIE Proceedings Vol. 9148:
Adaptive Optics Systems IV
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

© SPIE. Terms of Use
Back to Top