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 | ||
| − | + | [[Photometry overview]] -- Dr. Luisa Rebull (2010?) | |
| − | [[Photometry overview]] | ||
Revision as of 02:22, 31 July 2020
Photometry is the quantitative measure of brightness of an object in an astronomical images
Most coherent, developed, tested materials
Movie (10:50) on Photometry, part of the "Filters, Magnitudes, Colors, Oh My!" playlist -- -- Dr. Luisa Rebull, 2020
Photometry overview -- Dr. Luisa Rebull (2010?)
Somewhat less coherent (or less standalone) materials
Other sources of interest
- Your local astronomy textbook or (if neccessary) the Wikipedia entry for photometry is probably a good place to go for a longer general introduction.
- The IRAF manuals are old but still very, very valid. If you can pay attention to the concepts and ignore the IRAF-specific instructions, you can learn an awful lot from these manuals. Oldies but goodies.
- https://www.aavso.org/
- http://gtn.sonoma.edu/members/basic.php
- http://lcogt.net/en/book/introduction-photometry
- http://www.minorplanet.info/ObsGuides/Misc/photometryguide.htm
