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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… 
2016
2016
Applications of Radiometric Measurements in Non-Contact Thermometry and Mesopic Photometry
Aalto University, P.O. Box 11000, FI-00076 Aalto www.aalto.fi Author Maksim Shpak Name of the doctoral dissertation Applications… 
2014
2014
Circadian Characteristics of Special Glazing
The window provides the natural daylight for the indoor environment. Recent discoveries in photobiology found, that light… 
Review
2011
Review
2011
Save the Lightcurves
Asteroid time-series photometry has been going on for many years and, as a result, generated enormous amounts data, much of it… 
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… 
2007
2007
Analysis of the Halo Globular Cluster M30 and its Variable Stars
Andrew C. Layden, Advisor Photometry of the metal-poor globular cluster M30 is presented in B, V, R and I bandpasses. A color… 
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… 
2002
2002
Rotation of stars in NGC 6134 ⋆ A comparison of δ Scuti stars and non-variable stars
We present results of spectroscopic observations of selected stars in the southern open cluster NGC 6134. We have determined the… 
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… 
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