Difference between revisions of "Spectral Energy Distributions (SEDs)"

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Spectral energy distributions (SEDs) show the amount of energy emitted by an object as a function of wavelength. SEDs are not the same thing as blackbodies! But stars can be approximated by blackbodies, so blackbodies come up a lot in the context of SEDs.
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Spectral energy distributions (SEDs) show the amount of energy emitted by an object as a function of wavelength. SEDs are not the same thing as blackbodies! But stars can be approximated by blackbodies, so blackbodies come up a lot in the context of SEDs. This page covers concepts; there is [[Making SEDs | another page on how to make SEDs]].
  
 
=Most coherent, developed, tested materials=
 
=Most coherent, developed, tested materials=
  
[https://www.youtube.com/watch?v=BUdKXY4JDMk&list=PLjCjDYabTFm9b9jQd4hcZPAnFWYsIjs2D&index=6&t=0s Movie (12:46) on Temperatures and Blackbodies], part of the "Filters, Magnitudes, Colors, Oh My!" playlist -- Dr. Luisa Rebull, 2020  
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*[https://www.youtube.com/watch?v=BUdKXY4JDMk&list=PLjCjDYabTFm9b9jQd4hcZPAnFWYsIjs2D&index=6&t=0s Movie (12:46) on Temperatures and Blackbodies], part of the "Filters, Magnitudes, Colors, Oh My!" playlist -- Dr. Luisa Rebull, 2020  
 
 
 
*[https://www.youtube.com/watch?v=VHMTB95b5us Movie (0:30, soundless)] that shows blackbodies as a function of temperature (T)  -- Dr. Luisa Rebull, 2017
 
*[https://www.youtube.com/watch?v=VHMTB95b5us Movie (0:30, soundless)] that shows blackbodies as a function of temperature (T)  -- Dr. Luisa Rebull, 2017
 
*[https://www.youtube.com/watch?v=HoQ_Ew4loFg Movie (0.31, soundless)] that shows a blackbody with varying reddening (Av)  -- Dr. Luisa Rebull, 2017
 
*[https://www.youtube.com/watch?v=HoQ_Ew4loFg Movie (0.31, soundless)] that shows a blackbody with varying reddening (Av)  -- Dr. Luisa Rebull, 2017
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=Other important CoolWiki pages=
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*[[Filters]]
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*[[Photometry (concept)]]
  
 
=Somewhat less coherent (or less standalone) materials=
 
=Somewhat less coherent (or less standalone) materials=

Latest revision as of 19:04, 11 August 2020

Spectral energy distributions (SEDs) show the amount of energy emitted by an object as a function of wavelength. SEDs are not the same thing as blackbodies! But stars can be approximated by blackbodies, so blackbodies come up a lot in the context of SEDs. This page covers concepts; there is another page on how to make SEDs.

Most coherent, developed, tested materials

Other important CoolWiki pages

Somewhat less coherent (or less standalone) materials

Other sources of interest