667 research outputs found
Color Intensity Projections: A simple way to display changes in astronomical images
To detect changes in repeated astronomical images of the same field of view
(FOV), a common practice is to stroboscopically switch between the images.
Using this method, objects that are changing in location or intensity between
images are easier to see because they are constantly changing. A novel display
method, called arrival time color intensity projections (CIPs), is presented
that combines any number of grayscale images into a single color image on a
pixel by pixel basis. Any values that are unchanged over the grayscale images
look the same in the color image. However, pixels that change over the
grayscale image have a color saturation that increases with the amount of
change and a hue that corresponds to the timing of the changes. Thus objects
moving in the grayscale images change from red to green to blue as they move
across the color image. Consequently, moving objects are easier to detect and
assess on the color image than on the grayscale images. A sequence of images of
a comet plunging into the sun taken by the SOHO satellite (NASA/ESA) and Hubble
Space Telescope images of a trans-Neptunian object (TNO) are used to
demonstrate the method.Comment: 9 pages, 2 figures. Accepted for publication in Publications of the
Astronomical Society of the Pacific. The quality of figure 1 been improved
from the previous posted versio
Following illicit finance across distance and difference:The coordination and practices of financial intelligence units
Following illicit finance across distance and difference:The coordination and practices of financial intelligence units
Following Suspicious Transactions in Europe:Comparing the Operations of European Financial Intelligence Units (FIUs)
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