Figure 3 from UNVEILING THE GAMMA-RAY SOURCE COUNT DISTRIBUTION BELOW THE FERMI DETECTION LIMIT WITH PHOTON STATISTICS

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

UNVEILING THE GAMMA-RAY SOURCE COUNT DISTRIBUTION BELOW THE FERMI DETECTION LIMIT WITH PHOTON STATISTICS

Authors: Hannes-S. Zechlin, Alessandro Cuoco, Fiorenza Donato, Nicolao Fornengo, and Andrea Vittino

2016 The Astrophysical Journal Supplement Series 225 18.

Provider: AAS Journals

Caption: Figure 3.

Photon counts map between 1 and 10 GeV as derived from the Fermi-LAT data covering the time period of 6 yr. The Mollweide projection of the celestial sphere is shown in Galactic coordinates ﹩(l,b),﹩ centered on the position of the Galactic center. The Galactic plane has been omitted within ﹩| b| \lt 30﹩° (gray area). The color scale is log-linear.

Other Images in This Article

Copyright and Terms & Conditions