Paper
21 July 2010 The effects of atmospheric calibration errors on source model parameters
Author Affiliations +
Abstract
Optical long-baseline interferometric data is commonly calibrated with respect to an external calibrator, which is either an unresolved source or a star with a known angular diameter. A typical observational strategy involves acquiring data in a sequence of calibrator-target pairs, where the observation of each source is obtained separately. Therefore, the atmospheric variations that have time scales shorter than the cadence between the target-calibrator pairs are not always fully removed from the data even after calibration. This results in calibrated observations of a target star that contain unknown quantities of residual atmospheric variations. We describe how Monte Carlo simulations can be used to assess quantitatively the impact of atmospheric variations on fitted model parameters, such as angular diameters of uniform-disk models representing semi- and fully-resolved single stars.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christopher Tycner, D. J. Hutter, and R. T. Zavala "The effects of atmospheric calibration errors on source model parameters", Proc. SPIE 7734, Optical and Infrared Interferometry II, 773439 (21 July 2010); https://doi.org/10.1117/12.857345
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Cited by 3 scholarly publications.
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KEYWORDS
Atmospheric modeling

Calibration

Stars

Interferometry

Current controlled current source

Infrared radiation

Monte Carlo methods

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