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Finding Asteroids

If you have done the Asteroids project, you may have learned how to identify asteroids from their movements. We are now going to learn to identify moving objects by a process called "blinking". In 1930, Clyde Tombaugh blinked images to discover Pluto. Along with asteroids and new planets, blinking can also be used to discover other objects such as supernovae, novae, and variable stars.

Blinking images means quickly switching between two images. IRIS can do this for you automatically. You will be able to see changes between the two images, such as an object moving back and forth. The moving object could be an asteroid.

You may see some objects get brighter or dimmer. If you are alternating two filters, such as the red and the green, this tells you that an object is brighter in one color than in the other. If you are looking at two different images taken through the same filter but at different times, this tells you the object is actually getting brighter or dimmer.

The procedure for blinking images is lengthy, but it's worth it!

Exercise 6. The steps you must follow to blink images are outlined below.

1. Retrieve the data from the SDSS Retrieve Images tool. You want run 125, rerun 7, camcol 5, field 178, objid 55. Enter these numbers in the textbox, separating each value by a space. For the data type, deselect Atlas Images and select Corrected Frames. Select the r and g bands (they are on opposite ends of the camera, so the most time passes between the r and g bands, making it easier to find asteroids). Return the files as a .zip file. Unzip the files into the default directory you specified earlier. Rename the files so they are easy to remember. Be sure the filename ends with the .fts extension.

2. Align the fields: Since some time passes between the two exposures, the fields are not exactly aligned. To directly compare the images, we need to shift their alignments. Open the green picture first. Adjust the max and min values to make the images clear. Select any easily identified bright star in the field. Draw a box around it with the mouse. Right click on the box and select PSF (this stands for Point Spread Function). Record the x and y coordinate of the center. Open the red picture and repeat the process to find the center of the same object.

Now, subtract the x-coordinate of the green image from the x-coordinate of the red image. Subtract the y-coordinate of the green image from the y-coordinate of the red image. Load the green image. Click on Geometry and select Shift. You will see a box as shown below:

Enter the offsets you calculated. Be sure not to drop the signs! Click OK when you have the images aligned, then save both files.

3. You are now ready to blink the images! Click on the in the toolbar. This button will bring up a small command box. Type the blink command. The blink command has the format:

blink image#1 image#2 delay

For image#1 and image#2, type the filenames for the red and green images (no .fts extension on the end, and be sure they are in your default directory). "Delay" is how long the images stay on the screen before switching, given in milliseconds. Try 200 - 300 for the delay (this will give you a 0.2 to 0.3 second delay). You can change the delay later if you like. To stop the images from blinking, type the command blinkoff.

All of the objects in the images should remain stationary, except for the asteroids. Find the asteroid(s)! Some objects may get brighter or dimmer but not move. That is all right. Some objects are brighter in the green or red filter.

Exercise 7. Go to the Navigation tool. Select any field you wish. Click on any object in the field. Click on Explore to get more information. Use the run, rerun, camcol, field, and objid to obtain another set of fields from the SDSS Retrieve Images tool. Look for asteroids in this set of fields. You may need to adjust max and min values to find dim asteroids.