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Cas-A remnant with horizontal cut at position 4158, 4398. You should notice as you move your mouse around the image that data represented by this graph remains unchanged as long as your mouse remains in the same horizontal row of pixels. See for yourself by using the arrow left, right, up and down buttons on the keyboard. |
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Cas-A remnant with vertical cut at position 4158, 4398. You should notice as you move your mouse around the image that data represented by this graph remains unchanged as long as your mouse remains in the same vertical column of pixels. |
To remove the pixel
value table, close the window using the button in the upper left
corner.
Display
contours
Iso-intensity contours are connected lines drawn on the image
through pixels of equal value. (The root "iso" comes
from the Greek meaning "equal". We are talking here
about marking out lines of equal pixel intensity on an image,
just as a topographical map marks out lines of equal elevation.)
These are useful for indicating large-scale features of an image.
The analysis menu has an option to overlay iso-intensity contours
on the image. You can choose the number of contours to generate,
as well as the smoothness of the contour lines. If you select
the display contours option first, it will display whatever setting
has been left on the contours parameters menu. To chose the contour
parameters click on that line and the menu will appear. Change
the values as you wish and push both the generate and apply buttons,
in that order, and wait for the new contour parameters to be
drawn on the image.

To remove contours,
deselect the "Display contours" option on the analysis
menu.
Display
coordinate grid
Pull down the analysis menu and click on display coordinate grid
menu option. A grid of astronomical sky coordinates will be displayed
over the image. This is useful for reminding yourself where in
the sky your object is located. This feature is especially useful
when looking at areas of the sky with multiple sources, like
the deep surveys, or areas where it is important to be able to
pick out a particular source in an area where sources are close
together.

Summary
There are, of course, other features in ds9 that will help you
get a "qualitative" feel for your x-ray data so that
you can begin to notice interesting features that you will want
to analyze quantitatively. Don't be afraid to try things out!
A detailed manual of ds9 features is on-line at the ds9 homepage.
Part 3: Learning ds9, Starting Quantitative Analysis
[next] [back]
Last updated: 7/20/04
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Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA 02138 USA Phone: 617.496.7941 Fax: 617.495.7356 |
Comments
& Questions? cxcedu@cfa.harvard.edu |
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This site was developed with funding from NASA under Contract NAS8-39073. |
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