Paper
21 February 2003 Catalog of reference stars for long baseline stellar interferometry
Author Affiliations +
Abstract
The calibration process of long baseline stellar interferometers requires the use of reference stars with accurately determined angular diameters. We present a catalog of 374 carefully chosen stars among the all-sky network of infrared sources provided by Ref. 1. The catalog benefits from a very good sky coverage and a median formal error on the angular diameters of only 1.2%. Besides, its groups together in a homogeneous handy set stellar coordinates, uniform and limb-darkened angular diameters, photometric measurements, and other parameters relevant to optical interferometry. In this paper, we describe the selection criteria applied to qualify stars as reference sources. Then, we discuss the catalog's statistical properties such as the sky coverage or the distributions of magnitudes and angular diameters. We study the number of available reference stars as a function of the baseline and the precision needed on the visibility measurements. Finally, we compare the angular diameters predicted in Ref. 1 with existing determinations in the literature, and find a very good agreement.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Pascal J. Borde, Vincent Coude du Foresto, Gilles Chagnon, and Guy S. Perrin "Catalog of reference stars for long baseline stellar interferometry", Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); https://doi.org/10.1117/12.457191
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Visibility

Calibration

Interferometers

K band

Interferometry

Scanning probe microscopy

RELATED CONTENT

A catalog of calibrator stars for 200 meter baseline near...
Proceedings of SPIE (October 20 2004)
Infrared interferometric observations of T Tauri stars
Proceedings of SPIE (February 21 2003)
Main sequence stars as calibrators for interferometry
Proceedings of SPIE (October 20 2004)
FLUOR fibered beam combiner at the CHARA array
Proceedings of SPIE (February 21 2003)

Back to Top