Aperture Photometry

The Aperture Photometry command opens the Aperture Photometry Toolbar. This is a standard Command Toolbar interface to functions for measuring the magnitudes of astronomical objects. Aperture photometry results are reported in a standard Mira Report Window. The Aperture Photometry package can measure the magnitudes and related parameters for one or more stars in one or more images each in one or more Windows. Both standard stars and target objects can be measured.

Getting Started with Aperture Photometry

To start or finish Aperture Photometry, use Measure > Photometry or click on the main Measurements Toolbar to open or close its toolbar.
View the tutorial Introduction to Aperture Photometry.
View the tutorial Doing Time Series Photometry.
To Measure an Object, click the mouse on each object. The result is reported in the Photometric Measurements Report window. If the ZERO-PT keyword is already present in the image header(s), the zero point value is included in the reported magnitude.
To change most photometry settings, click the button on the Toolbar to open the Aperture Photometry Preferences dialog.
Change aperture size and shape using the Aperture Tool window.
Measure an Image Set and Plot a Light Curve of targets, standards, and check stars.
If you are a member of the AAVSO, prepare an AAVSO formatted report of measurements.
Learn about setting header keywords for calculating airmass, photometric errors, and the zero point using the Photometry Keywords dialog. Note that the airmass is not calculated for an image unless you check the option on the Other preferences page.
To learn how magnitudes and errors are computed, see Magnitude Calculations.
Read about Photometric Measurement Definitions and Photometric Error Definitions.
To set or change the object name, notes, or weight, click the button on the toolbar to enter Edit Mode.
Each magnitude measurement appears in a Photometry Measurements Report Window. This window has a large amount of built-in functionality of Mira Report Windows which allow you to reorganize the table and save your results.
Object coordinates may be copied and pasted from one image to another or from one window to another using the Copy Markers and Paste Markers commands. You can also import coordinates from a text file using the Import Photometry Catalog command.
An existing marker may be moved around the image to measure other objects without adding new positions. Simply change to move mode and drag the aperture to a new position. Each time you release the mouse to drop the aperture, it will (optionally) centroid on the new position and report it magnitude in the table.
Marker parameters may be interactively adjusted using the Aperture Tool. You can adjust the shape between circular and elongated, and set the sizes and orientation of the apertures.
Select Heliocentric or Geocentric (normal) Julian Date from theOther Preferences dialog.

Aperture Photometry Toolbar

Aperture photometry commands are operated from the toolbar shown below. Some commands are also accessed from the Preferences dialog, which is opened using the button on the toolbar.

The button calculates and/or applies the photometric zero point for all images where objects are marked, then updates the results in the Photometric Measurements table. This calculation uses all specified settings and all standard stars defined in all images. It is important to recalculate everything after making certain types of changes such as changing the weights of standard stars or making adding 1 or more standard stars to an image or you make changes to the GAIN, RDNOISE, or EXPTIME keywords for an image. If in doubt, click .Mira allows some flexibility in which keywords are used for the various photometry parameters. The keywords can be specified using the Photometry Keywords dialog. The airmass is also calculated if the appropriate keywords are found in the image header. The airmass calculation uses the first 6 keywords specified in the Photometry Keywords dialog.

The results of photometric measurements are listed in the Aperture Photometry Report Window. All reported values are defined in Photometric Measurement Definitions and Photometric Error Definitions. You can copy or save the results from this window, plot a light curve, or make a scatter plot of values in two table columns. For example you might plot the Error vs. Magnitude. If doing photometry of an Image Set, then you might plot Magnitude versus Julian Date.

Overview

The Image Window below shows an image with 5 objects marked. Each marker includes 3 apertures: the inner aperture, which measures the total signal from the object + sky, and 2 outer apertures which define an annulus for measuring the local brightness of the background (the "sky"). The background is subtracted from the [object + background] measurement to obtain the net signal attributable to the object. This is converted to a magnitude and reported in the Photometry Measurements Report window. As shown below, Mira allows the photometry apertures to be ellipses. Circular apertures are used simply by setting the ellipticity to 0.

Automated Processing of Multiple Objects in Multiple Frames

Mira AP provides a semi-automation capability for measuring objects in multiple frames using the importing facility. In this case, you import the coordinates of the objects from a text file "database" and have Mira process the objects in all images of an image set. See the Import Photometry Catalog command.

Getting Started with Aperture Photometry

Aperture Photometry Toolbar

Overview

Automated Processing of Multiple Objects in Multiple Frames

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