When the image is loaded into memory, it is also displayed in an X
window. Before or after loading you can choose either grey level or
color coded intensity display. You choose the pallete by pressing
either Grey or Color button in the image window. If
you want to save this setting as a default mode for the next time when
you invoke fitsblink
, go to the Astrometry menu and
press the Settings button. Although white stars on black
background are ``natural'', you may prefer to set the inverse mode
(black stars on white background) or color mode in which you spot
nebulosities more easily. If you have only an 8-bit display and you
already run some colorful program when you invoke fitsblink
,
the color pallete may be limited and you may see stars displayed in
some funny colors.
If you are not happy with the color or grey level settings which were set automatically when the image was loaded, you may want to adjust them manually. You can do this by holding the left mouse button on one of the points in the Grey level correction window and dragging it to a desired position. Typically, the two points between which the curve jumps from zero to the maximum value are very close together. For fine adjustment you should zoom the curve by clicking on arrow buttons below the window. Press the right mouse button for quick zoom, middle mouse button for moderately quick zoom and left mouse button for slow zoom. Pressing the right mouse button on the third arrow is what you usually need.
You can resize the blinker window to some limit in the usual way as it
is done in X-Windows. If you want to set the new window size as a
default value for the future invocations of fitsblink
, just open
the Settings window and press Save. Note that you
also save all other parameters when you do this.