App/program that allows you to adjust spectrums of light?

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Discussion Overview

The discussion centers around the possibility of accessing or creating images of galaxies and nebulae that allow users to adjust the spectra of light portrayed. Participants explore the nature of how telescopes capture images and the availability of spectral data from various sources.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant inquires about a website or program that allows for the adjustment of light spectra in images of galaxies and nebulae.
  • Another participant mentions a site where users can process raw Hubble data to create images, noting that telescopes typically capture greyscale images through different filters rather than color images.
  • A participant points out the availability of spectral data on stars, galaxies, and quasars at the SDSS website, explaining the process of selecting objects for spectral analysis.
  • There is a discussion about the nature of the data from SDSS, with one participant questioning whether it represents the total light of an object or allows for images made of different wavelengths.
  • Another participant explains that it is common practice to use filters to block undesired frequencies and mentions that modern computers can deselect photons based on frequency.
  • Clarifications are made regarding the definition of a spectrum, emphasizing that it represents light intensity versus wavelength but lacks spatial information.
  • It is noted that the SDSS site provides multiple images taken through different filters, which can be downloaded as fits files.

Areas of Agreement / Disagreement

Participants express varying levels of understanding about the imaging process and the nature of spectral data. There is no consensus on the existence of a specific application that meets the original inquiry, and multiple viewpoints regarding the capabilities of existing data sources remain.

Contextual Notes

Participants highlight limitations in accessing spatially resolved images at different wavelengths and the need for further learning to navigate the spectral data available at SDSS.

questioner1
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Hey!

I'm looking for a web-site or something with images from galaxy's and nebulae that allows you to adjust which spectra of light the image portrays.
I know that the images shown of galaxys usually are "translated" into our visible spectrum of light, but I'd like to be able to adjust which spectra I see myself. Is that possible?

is it true that when telescopes make these images, that they actually record all the spectra? or is the data not even available? (i.e. do they choose which spectra to record before the image is taken?)

This would be really awesome, if such a website/program exists!
 
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I don't know of an app that does what you want but I found this site where people can process the raw image data from Hubble to produce a stunning picture. You might further references there.

http://hubblesite.org/get_involved/hubble_image_processors/
 
jedishrfu said:
I don't know of an app that does what you want but I found this site where people can process the raw image data from Hubble to produce a stunning picture. You might further references there.

http://hubblesite.org/get_involved/hubble_image_processors/

Thanks! I see now that the telescopes don't actually take color images, but greyscale images at different filters. I didn't know that!
 
There's a wealth of spectral data on stars, galaxies and quasars available at the SDSS website at http://mirror.sdss3.org/ I attached an image of the type of spectrum you can get. It will take a little bit of learning to learn how to find the spectra (they are under "Optical Spectra"), but it is well worth it. At SDSS, they run a preliminary imaging run, then select which objects they want spectra on, and then take the spectra. SDSS is able to get spectra on about 500-1000 objects at a time for each exposure.
 

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phyzguy said:
There's a wealth of spectral data on stars, galaxies and quasars available at the SDSS website at http://mirror.sdss3.org/ I attached an image of the type of spectrum you can get. It will take a little bit of learning to learn how to find the spectra (they are under "Optical Spectra"), but it is well worth it. At SDSS, they run a preliminary imaging run, then select which objects they want spectra on, and then take the spectra. SDSS is able to get spectra on about 500-1000 objects at a time for each exposure.

Thats cool! but this data contains only the total light of the entire object, right? So you can't see an image made of different wavelengths
 
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It is common practice to use filters to block undesired frequencies. With modern computers photons can be deselected based on frequency, which is often more efficient.
 
questioner1 said:
Thats cool! but this data contains only the total light of the entire object, right? So you can't see an image made of different wavelengths

A spectrum is a plot where the light is broken up into different wavelengths. The plot I uploaded shows the light intensity on the Y-axis vs wavelength on the X-axis.
 
To be overly explicit, a spectrum is exactly an image of the different wavelenghts from some source. It does however not make a picture in the sense that you have any spatial information.
 
Tobychev said:
To be overly explicit, a spectrum is exactly an image of the different wavelenghts from some source. It does however not make a picture in the sense that you have any spatial information.

Right. If you want images at different wavelengths, the SDSS site has 5 different images taken through 5 different filters, called ugriz. You can download the fits files for these images.
 

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