Aperture Tool
Astronomy Module Specific
The Aperture Tool is a small floating Tool Window used to adjust the shape of the markers used in the Aperture Photometry package.
Open the Aperture Tool by clicking on the Aperture Photometry Toolbar.
The Aperture Tool Window makes it easy to change the marker parameters. Doing so changes the amount of signal being measured through the inner aperture ad affects the measurement of the local sky background between the 2 outer apertures. In the description below, the term "marker" refers to the set of 3 apertures used to mark and measure each object.
The top-most control is the Mode selection box. Mira provides two ways to express the size of the measuring apertures: directly in radius or as a scale factor that multiplies the FWHM of the image. Select Radius or Scale, and the values in the aperture size fields will change to the appropriate values.
The upper 3 edit fields show the size of the measuring apertures. The units displayed depends upon the mode setting:
Radius, specifies the radius directly in units of [pixels].
Scale, specifies the radius indirectly in terms of scale factors that multiply the image FWHM as measured in [pixels]. The FWHM must have been previously measured for the image and the value stored in the image header as the PSF-FWHM keyword.
All aperture measurements equate to radius, in dimensions of [pixels].
The mode, Radius or Scale, is specified on the Other Preferences page opened from the button on the Aperture Photometry Toolbar. Values can be set for each of the aperture rings. Actually, these settings control the semimajor axis of each aperture, since Mira considers apertures to be elliptical (Note: for a circular aperture, the semimajor axis equals the radius). From the top control downward, these 3 fields show 1) the inner aperture that measures the object, 2) the inner sky aperture, and 3) the outer sky aperture. Needless to say, these three apertures should have radii in increasing order.
The control above the large round dial, changes the Ellipticity of the markers. Ellipticity is defined as E = 1 - b/a, in which b is the semiminor axis and a is the semimajor axis length. All 3 apertures have the same ellipticity, so they also change together. Setting a value of 0 makes the apertures circular.
The Angle dial orients the direction of the major axis of the marker. This is only useful if the Ellipticity is greater than 0, meaning that the apertures are not circular. The angle is always measured so that it increases from positive x through positive y (see Angle Measurement Definition), except that the astronomical 0 angle is taken along the y axis, which is north (up) if the image is a FITS format image displayed in the normal way.
The [Apply] button applies your settings if the Auto option is not checked. Since Mira updates all the measurements when the settings are applied, it is sometimes desirable to uncheck the Auto option and make all your changes before clicking [Apply] to force everything to be re-measured.
If the Auto check box at the bottom of the window is checked, releasing the mouse on any control causes Mira to recalculate all magnitudes for all images in the Image Window and then update the Photometry Measurements window. If this check box is unchecked, Mira does no recalculation until you click [Apply].
The Aperture Tool Window is a shared resource, meaning that there is only one of them and therefore, if you have more than 1 Photometry Toolbar Command going, it will have to be shared between them.
The Aperture Tool communicates with the top-most Image Window where an Aperture Photometry Toolbar is active.
If you have more than one Aperture Photometry process active, you can see the values in the Tool Window change when you click on the different windows. One useful result of this is that you can easily compare the effect of different aperture parameters by opening the same image(s) for aperture photometry in a number of separate Image Windows. Simply click on each window in turn to connect it with the Aperture Tool and then change the settings. This also shows why each Image Window is connected to a different Photometry Measurements Report window.
Aperture Photometry, Photometry Measurements, Aperture Photometry Example, Other Preferences