How do I properly plot the solar spectrum and handle the flux of Arcturus?

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SUMMARY

This discussion focuses on plotting the solar spectrum using a dataset that includes Solar Flux, Arcturus Flux, and Wavelength values. The user encounters difficulties in visualizing the data due to the high number of data points (21,000) and seeks clarification on the role of Arcturus Flux, questioning if it serves as a calibration standard. Recommendations include normalizing the flux, potentially flipping the plot, and utilizing a smoothing filter to enhance clarity while preserving essential spectral features.

PREREQUISITES
  • Understanding of spectral data representation (Wavelength vs. Flux)
  • Familiarity with normalization techniques in data visualization
  • Knowledge of smoothing filters for data processing
  • Basic concepts of stellar flux and calibration standards
NEXT STEPS
  • Learn about normalization techniques for spectral data visualization
  • Research the use of smoothing filters in data analysis
  • Explore the characteristics of Ca H and K lines in stellar spectra
  • Investigate methods for effectively plotting large datasets in scientific visualization
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Astronomers, data analysts, and researchers involved in spectral analysis and visualization, particularly those working with stellar flux data and seeking to improve their plotting techniques.

AlphaCrucis
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TL;DR
I'm to plot the solar spectrum from some data files I'm given and locate and mark on my plot various types of spectral lines
I'm trying to plot the solar spectrum (Wavelength versus Flux) from a table of values I'm given. I'm given 3 columns;

Solar Flux
Arcturus Flux
Wavelength

Plotting Solar Flux versus Wavelength gives me a graph (below) that is very difficult to resolve. There are 21,000 data points as well.
If I'm plotting the solar spectrum however; I'm confused what to do with the flux of Arcturus. Is it a calibration standard?
My plot looks like what is shown below; it is difficult to resolve. Perhaps I need to normalize?

Plot.png
I would like something more like this; (it appears I need to flip my plot as well)

Screenshot (130).png


The F/Fc axis for the second image seems like the flux is normalized to a continuum(?).
 
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The data looks to be already normalised. I don't think you need do anything with the Arcturus spectra. To see what's going on better increase the length of the x-axis or plot subsections.

Given where they are they look like tha Ca H and K lines which are very complex. You would think need to research these lines and their structure.

Regards Andrew

PS I have replied to two other post of yours but never got a reply. Hint.
 
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andrew s 1905 said:
PS I have replied to two other post of yours but never got a reply. Hint.
Clicking on the user name gives "this user's profile is unavailable". I'm afraid I think that means you won't get a reply to this one either...
 
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You could pass a smoothing filter over the spectrum to smooth it a bit if it appears noisy. The features you're interested in will still be apparent and it would probably look a lot more like the examples given.
 

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