Abstract
The intensity of the diffuse ~1-4 μm sky emission from which solar system and Galactic foregrounds have been subtracted is in excess of that expected from energy released by galaxies and stars that formed during the z
Cite
CITATION STYLE
APA
Dwek, E., Arendt, R. G., & Krennrich, F. (2005). The Near‐Infrared Background: Interplanetary Dust or Primordial Stars? The Astrophysical Journal, 635(2), 784–794. https://doi.org/10.1086/497569
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