8,084 research outputs found
Image enhancement from a stabilised video sequence
The aim of video stabilisation is to create a new video sequence where the motions (i.e. rotations, translations) and scale differences between frames (or parts of a frame) have effectively been removed. These stabilisation effects can be obtained via digital video processing techniques which use the information extracted from the video sequence itself, with no need for additional hardware or knowledge about camera physical motion.
A video sequence usually contains a large overlap between successive frames, and regions of the same scene are sampled at different positions. In this paper, this multiple sampling is combined to achieve images with a higher spatial resolution. Higher resolution imagery play an important role in assisting in the identification of people, vehicles, structures or objects of interest captured by surveillance cameras or by video cameras used in face recognition, traffic monitoring, traffic law reinforcement, driver assistance and automatic vehicle guidance systems
The WFPC2 Archival Parallels Project
We describe the methods and procedures developed to obtain a near-automatic
combination of WFPC2 images obtained as part of the WFPC2 Archival Pure
Parallels program. Several techniques have been developed or refined to ensure
proper alignment, registration, and combination of overlapping images that can
be obtained at different times and with different orientations. We quantify the
success rate and the accuracy of the registration of images of different types,
and we develop techniques suitable to equalize the sky background without
unduly affecting extended emission. About 600 combined images of the 1,500
eventually planned have already been publicly released through the STScI
Archive. The images released to date are especially suited to study star
formation in the Magellanic Clouds, the stellar population in the halo of
nearby galaxies, and the properties of star-forming galaxies at .Comment: 12 pages, 7 figures, to appear in the PAS
Difference Image Analysis of Galactic Microlensing I. Data Analysis
This is a preliminary report on the application of Difference Image Analysis
(DIA) to galactic bulge images. The aim of this analysis is to increase the
sensitivity to the detection of gravitational microlensing. We discuss how the
DIA technique simplifies the process of discovering microlensing events by
detecting only objects which have variable flux. We illustrate how the DIA
technique is not limited to detection of so called ``pixel lensing'' events,
but can also be used to improve photometry for classical microlensing events by
removing the effects of blending. We will present a method whereby DIA can be
used to reveal the true unblended colours, positions and light curves of
microlensing events. We discuss the need for a technique to obtain the accurate
microlensing time scales from blended sources, and present a possible solution
to this problem using the existing HST colour magnitude diagrams of the
galactic bulge and LMC. The use of such a solution with both classical and
pixel microlensing searches is discussed. We show that one of the major causes
of systematic noise in DIA is differential refraction. A technique for removing
this systematic by effectively registering images to a common airmass is
presented. Improvements to commonly used image differencing techniques are
discussed.Comment: 18 pages, 8 figures, uses AAS LaTEX 4.0, To appear in Astrophysical
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