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Drizzle (image processing)

Known as: Drizzle (disambiguation), Drizzle (photometry) 
Drizzle (or DRIZZLE) is a digital image processing method for the linear reconstruction of undersampled images. It is normally used for the… 
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Related topics

Related topics

4 relations
Digital image processingLucy–Hook coaddition methodUndersampling

Broader (1)

Image processing

Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2016
2016
Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V 1094 Tau ⋆
Context. V1094 Tau is a bright eclipsing binary star with an orbital period close to nine days that contains two stars similar to… 
2014
2014
Circadian Characteristics of Special Glazing
The window provides the natural daylight for the indoor environment. Recent discoveries in photobiology found, that light… 
2014
2014
Athens Institute for Education and Research ATINER ATINER ' s Conference Paper Series PHY 2014-1259
The window provides the natural daylight for the indoor environment. Recent discoveries in photobiology found, that light… 
Review
2012
Review
2012
Searching for the Perseus arm in the anticenter direction
Here we propose a two step approach to provide new insights on the outer spiral arm pattern of the Milky Way: 1) a Stromgren… 
2010
2010
A study of the massive star forming region M8 using Spitzer IRAC images
Spitzer IRAC images (3.6, 4.5, 5.8 and 8.0$\mu$m) and photometry of the star forming region M8 are presented. IRAC photometry… 
2006
2006
MPIfR Near-infrared speckle imaging and AO polarimetry of the bipolar protoplanetary nebula Frosty
IRAS 09371+1212 is an oxygen-rich post-asymptotic giant branch (postAGB) star with an hourglass-like bipolar proto-planetary… 
2002
2002
Photoelectric photometry of eclipsing contact binaries: U Peg, YY CrB, OU Ser and EQ Tau
New photoelectricUBV observations of the eclipsing contact binary systems U Peg, YY CrB, OU Ser and EQ Tau obtained from August… 
Review
2002
Review
2002
Detection and study of variable sources with wide field imagers
In recent years massive CCD photometry has dramatically increased the number of known variable stars in the Milky Way and nearby… 
2000
2000
A detailed spectroscopic analysis of epsilon Per I. Determination of the orbital parameters and of the frequencies
We present the analysis of 445 high signal-to-noise spectra of the Si III triplet at 4553̊ A, 4568Å, 4575Å of the lineprofile… 
2000
2000
Strömgren Photometry from Z = 0 to Z ≈ 1. I. the Method
We use rest-frame Strömgren photometry to observe clusters of galaxies in a self-consistent manner from z =0 to z =0.8. Strömgren… 
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