Please use this identifier to cite or link to this item: https://hdl.handle.net/20.500.12104/68021
Title: Diffracto-astrometry measurements: Accuracy of the measuring algorithm
Author: Ruelas-Mayorga, A.
Sanchez, L.J.
Olivares, J.
Allen, C.
Poveda, A.
Costero, R.
Nigoche-Netro, A.
Issue Date: 2014
Abstract: We present a theoretical analysis of the Diffracto-Astrometry measuring algorithm. We generated Tiny-Tim Theoretical Point Spread Functions (PSFs) for the CCDs in the HST Wide Field Planetary Camera 2 (WFPC2). These images were then measured using only their diffraction pattern, and positions for the simulated PSFs were obtained. The measuring algorithm recovers the original positions reasonably well (±0.1 to ±0.4 pixels). However, slight deviations from the original values are observed. We adjust the differences between the real and the measured position with a quadratic function of the coordinates. Application of these transformations allows determination of the position of a stellar image within a few hundredths of a pixel.
URI: http://hdl.handle.net/20.500.12104/68021
Appears in Collections:Producción científica UdeG (prueba)

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