A Full Resolution of the 450 μm Extragalactic Background Light

Abstract

The extragalactic background light (EBL) is the cumulative radiation outside the Milky Way. The determination of its corresponding primary emitting sources as well as its total energy level across the entire electromagnetic spectrum has profound implications for both cosmology and galaxy formation. However, the detailed origin of the EBL at far-infrared wavelengths, particularly those close to the peak of the cosmic infrared background, remains unclear. Here we report the results of our ongoing SCUBA-2 450 μ m survey of 10 massive galaxy cluster fields. By exploiting the strong gravitational lensing offered by these clusters, we obtain significant counts down to an unprecedented depth of ∼0.1 mJy at this wavelength, about 10 times deeper than that reached by any other previous survey. The cumulative energy density based on the counts is 138.1 ${}_{-19.3}^{+23.9}$ Jy deg ^−2 or 0.45 ${}_{-0.06}^{+0.08}$ MJy sr ^−1 . Comparing our measurements to those made by the COBE and Planck satellites, we find that at this flux density level, the 450 μ m EBL is entirely resolved by our SCUBA-2 observations. Thus, we find for the first time that discrete sources produce fully to the 450 μ m EBL, and that about half of it comes from sources with sub-mJy flux densities. Our deep number counts provide strong constraints on galaxy formation models.

Keywords

• Submillimeter astronomy
• Galaxy counts
• Extragalactic astronomy
• Cosmic background radiation