Difference between revisions of "Photometry (concept)"

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=Most coherent, developed, tested materials=
 
=Most coherent, developed, tested materials=
  
[https://www.youtube.com/watch?v=gpq6xVmosx8&list=PLjCjDYabTFm9b9jQd4hcZPAnFWYsIjs2D&index=3&t=0s Movie (10:50) on Photometry], part of the "Filters, Magnitudes, Colors, Oh My!" playlist -- Dr. Luisa Rebull, 2020  
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*[https://www.youtube.com/watch?v=gpq6xVmosx8&list=PLjCjDYabTFm9b9jQd4hcZPAnFWYsIjs2D&index=3&t=0s Movie (10:50) on Photometry], part of the "Filters, Magnitudes, Colors, Oh My!" playlist -- Dr. Luisa Rebull, 2020  
 
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*[https://www.youtube.com/watch?v=8Um3p0QScQ0&list=PLjCjDYabTFm9b9jQd4hcZPAnFWYsIjs2D&index=4&t=0s Movie (3:01) on Detections and Limits], part of the "Filters, Magnitudes, Colors, Oh My!" playlist -- Dr. Luisa Rebull, 2020
[[Photometry overview]] -- Dr. Luisa Rebull (2010?)
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*[[Photometry overview]] -- Dr. Luisa Rebull (2010?)
  
  

Revision as of 17:10, 31 July 2020

Photometry is the quantitative measure of brightness of an object in an astronomical images.

Most coherent, developed, tested materials


Somewhat less coherent (or less standalone) materials

Aperture Photometry Overview -- Dr. Luisa Rebull (2010?)

PSF photometry - To come. Basic steps are essentially the same (detect objects, center up, determine what is background/source, sum up light for the source, check your results). More complicated than aperture photometry because you have many more free parameters than for aperture photometry.

need to add document i made for olivia and tom 2019

Other sources of interest