http://skynet.unc.edu/
To use images already requested and imaged on Skynet, use this site and the passcodes Mrs Ramseyer gave you in class.
Directions for Imaging with the Skynet Telescopes (we will need to wait for Yerkes to reopen)
Use of AfterGlow
Once the images are returned and you would like to create a light curve with them use:
http://skynet.unc.edu/afterglow
First go to
Process - Align
Add files and WAIT
then My Images (This area matches what is currently in your Skynet account.)
then filter area type what image you are looking for NOT the color filter:)
select images (button on lower right...Use the shift button on the keypad or control to choose.))
then next.
A split screen is returned; an image screen and an align screen.
FIT the first of your images on the screen then
using the ALIGN screen that is open on the right make sure each image is visible and that
one star manual is selected.
Click on one bright star in the center of each images. The program will automatically advance to the next image. Click on this same star in every image until complete. (You will see a Red x.)
Choose Select Target Directory on the align screen. A new screen appears where you make a new folder, select the new folder and select. (This is at the bottom of the new folder screen!!!)
This new folder will appear under the Select Target Directory. Hit NEXT and you get a happy message. OK. Return to Afterglow screen.
Next
Process - Batch Photometry
load the folder (previously created in the work area) Select and NEXT.
A split screen is returned; an image screen and a batch photometry screen.
Using the batch photometry screen
select the variable star and 1-2 reference star in one of the images and name them on the batch photometry screen.
Click on Find Source in All Images.
Check to see if these stars were labeled on every image get a spreadsheet of data. NEXT
A Spreadsheet appears. To make a light curve you need to export - data analyzer - Variable Source
Two new screen appear (one is hidden behind the graph). List the variable and the reference and the magnitude of the reference star and check out your graph!