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Statements

Subject Item
n2:RIV%2F68407700%3A21230%2F07%3A03132199%21RIV08-GA0-21230___
rdf:type
skos:Concept n21:Vysledek
dcterms:description
This paper deals with evaluation and processing of astronomical image data, which are obtained by WFC (Wide-Field Camera) or UWFC (Ultra Wide-Field Camera) systems. Precision of astronomical image data post-processing and analyzing is very important. Large amount of different kinds of optical aberrations and distortions is included in these systems. The amplitude of wavefront aberration error increases towards margins of the FOV (Field of View). Relation between amount of high order optical aberrations and astrometry measurement precision is discussed in this paper. There are descriptions of the transfer characteristics of astronomical optical systems presented in this paper. Spatially variant (SV) optical aberrations negatively affect the transfer characteristics of all system and make it spatially variant as well. SV model of optical system is presented in this paper. Partially invariant model of optical systems allows using Fourier methods for deconvolution. This paper deals with evaluation and processing of astronomical image data, which are obtained by WFC (Wide-Field Camera) or UWFC (Ultra Wide-Field Camera) systems. Precision of astronomical image data post-processing and analyzing is very important. Large amount of different kinds of optical aberrations and distortions is included in these systems. The amplitude of wavefront aberration error increases towards margins of the FOV (Field of View). Relation between amount of high order optical aberrations and astrometry measurement precision is discussed in this paper. There are descriptions of the transfer characteristics of astronomical optical systems presented in this paper. Spatially variant (SV) optical aberrations negatively affect the transfer characteristics of all system and make it spatially variant as well. SV model of optical system is presented in this paper. Partially invariant model of optical systems allows using Fourier methods for deconvolution. This paper deals with evaluation and processing of astronomical image data, which are obtained by WFC (Wide-Field Camera) or UWFC (Ultra Wide-Field Camera) systems. Precision of astronomical image data post-processing and analyzing is very important. Large amount of different kinds of optical aberrations and distortions is included in these systems. The amplitude of wavefront aberration error increases towards margins of the FOV (Field of View). Relation between amount of high order optical aberrations and astrometry measurement precision is discussed in this paper. There are descriptions of the transfer characteristics of astronomical optical systems presented in this paper. Spatially variant (SV) optical aberrations negatively affect the transfer characteristics of all system and make it spatially variant as well. SV model of optical system is presented in this paper. Partially invariant model of optical systems allows using Fourier methods for deconvolution.
dcterms:title
Space Variant Point Spread Function Modeling for Astronomical Image Data Processing Space Variant Point Spread Function Modeling for Astronomical Image Data Processing Space Variant Point Spread Function Modeling for Astronomical Image Data Processing
skos:prefLabel
Space Variant Point Spread Function Modeling for Astronomical Image Data Processing Space Variant Point Spread Function Modeling for Astronomical Image Data Processing Space Variant Point Spread Function Modeling for Astronomical Image Data Processing
skos:notation
RIV/68407700:21230/07:03132199!RIV08-GA0-21230___
n3:strany
66910T-01;66910T-10
n3:aktivita
n18:P
n3:aktivity
P(GA102/05/2054)
n3:dodaniDat
n17:2008
n3:domaciTvurceVysledku
n5:7204698 n5:8983763 n5:8430578 n5:7605099
n3:druhVysledku
n15:D
n3:duvernostUdaju
n7:S
n3:entitaPredkladatele
n20:predkladatel
n3:idSjednocenehoVysledku
451370
n3:idVysledku
RIV/68407700:21230/07:03132199
n3:jazykVysledku
n12:eng
n3:klicovaSlova
Image processing; PSF; Spatially variant systems; UWFC; deconvolution
n3:klicoveSlovo
n9:Spatially%20variant%20systems n9:PSF n9:UWFC n9:Image%20processing n9:deconvolution
n3:kontrolniKodProRIV
[7EAF4A8C71AF]
n3:mistoKonaniAkce
San Diego
n3:mistoVydani
Bellingham
n3:nazevZdroje
Astronomical Adaptive Optics Systems and Applications III
n3:obor
n19:JA
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
5
n3:projekt
n16:GA102%2F05%2F2054
n3:rokUplatneniVysledku
n17:2007
n3:tvurceVysledku
Páta, Petr Fliegel, Karel Koten, P. Řeřábek, Martin Švihlík, Jan
n3:typAkce
n11:WRD
n3:zahajeniAkce
2007-08-26+02:00
s:numberOfPages
10
n13:hasPublisher
SPIE
n10:isbn
978-0-8194-6839-0
n6:organizacniJednotka
21230