Edward L. Wright

TL;DR: The results of the DIRBE search were presented in this paper, showing that only the 140 and 240 μm data provided candidate detections of the CIB. But no plausible solar system or Galactic source of the observed 140 and 120 μm residuals can be identified, leading to the conclusion that the C IB has been detected at levels of νIν = 25 ± 7 and 14 ± 3 nW m-2 sr-1 at 140 and240 μm, respectively.

TL;DR: In this paper, the authors carried out a survey of the north and south ecliptic poles, EP-N and EP-S, respectively, with the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer (WISE).

TL;DR: In this article, the authors examined the properties of the power spectrum data with respect to the six-parameter CDM model and found no significant anomalies, and concluded that there is no compelling evidence for deviations from the?CDM model, which is generally an acceptable statistical fit to WMAP and other cosmological data.

TL;DR: In this article, a simple mid-infrared color criterion, W1-W2 \geq 0.8 (i.e., [3.4]-[4.6], was presented, which identifies 61.9 \pm 5.4 AGN candidates per deg2 to a depth of W2 = 15.0.

TL;DR: In this article, the authors presented the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29-month full-mission data.