Astrometry and Photometry with HST WFC3. II. Improved Geometric-Distortion Corrections for 10 Filters of the UVIS Channel

We present an improved geometric-distortion solution for the Hubble Space Telescope UVIS channel of Wide Field Camera 3 for 10 broadband filters. The solution is made up of three parts: (1) a third-order polynomial to deal with the general optical distortion, (2) a table of residuals that accounts f...

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Veröffentlicht in:	Publications of the Astronomical Society of the Pacific 2011-05, Vol.123 (903), p.622-637
Hauptverfasser:	BELLIN, A, ANDERSON, J, BEDIN, L. R
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Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology
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description	We present an improved geometric-distortion solution for the Hubble Space Telescope UVIS channel of Wide Field Camera 3 for 10 broadband filters. The solution is made up of three parts: (1) a third-order polynomial to deal with the general optical distortion, (2) a table of residuals that accounts for both chip-related anomalies and fine-structure introduced by the filter, and (3) a linear transformation to put the two chips into a convenient master frame. The final correction is better than 0.008 pixel ( [approx]0.3 mas ) in each coordinate. We provide the solution in two different forms: a FORTRAN subroutine and a set of FITS files, one for each filter/chip/coordinate.
doi_str_mv	10.1086/659878
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source	Jstor Complete Legacy; IOP Publishing Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection
subjects	Astronomy Earth, ocean, space Exact sciences and technology
title	Astrometry and Photometry with HST WFC3. II. Improved Geometric-Distortion Corrections for 10 Filters of the UVIS Channel
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