That bath of ancient and young photons suffusing the Universe today is called
the extragalactic background light (EBL).
The attached figure illustrates how energetic gamma rays (dashed lines) from a distant blazar strike photons of
extragalactic background light (wavy lines) and produce pairs of electrons and positrons.
In addition to Bock, Zemcov, and Cooray, other coauthors of the paper, «On the Origin of Near - Infrared
Extragalactic Background Light Anisotropy,» are Joseph Smidt of Los Alamos National Laboratory; Toshiaki Arai, Toshio Matsumoto, Shuji Matsuura, and Takehiko Wada of the Japan Aerospace Exploration Agency; Yan Gong of UC Irvine; Min Gyu Kim of Seoul National University; Phillip Korngut, a postdoctoral scholar at Caltech; Anson Lam of UCLA; Dae Hee Lee and Uk Won Nam of the Korea Astronomy and Space Science Institute (KASI); Gael Roudier of JPL; and Kohji Tsumura of Tohoku University.
Not exact matches
The
extragalactic infrared
background represents all of the infrared
light from all of the sources in the universe, «and there were some hints we didn't know where it was all coming from.»
Since astronomers don't know much about how strongly galactic dust polarizes
light, researchers involved in the
Background Imaging of Cosmic
Extragalactic Polarization, or BICEP, experiment relied on whatever information they could get their hands on.
The nature of this
light, called the
extragalactic gamma - ray
background (EGB) has been debated since it was first measured by NASA's Small Astronomy Satellite 2 in the early 1970s.