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The Diffuse Radiation Field at High Galactic Latitudes

  • Authors: M. S. Akshaya, Jayant Murthy, S. Ravichandran, R. C. Henry, and James Overduin

2018 The Astrophysical Journal 858 101.

  • Provider: AAS Journals

Caption: Figure 5.

FUV surface brightness plotted against IR surface brightness for the NGP. The black line shows a linear fit over all the data points and the blue line shows the best fit with the inflection point at 1.08 MJy sr−1.

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