“…This was followed recently by the Balloon‐borne Large Aperture Submillimeter Telescope (BLAST), 2 which measured the clustering power near the energetic peak of the CIB at 600, 860 and 1200 GHz (500, 350 and 250 μm, respectively; Viero et al 2009). Hall et al (2010) reported the first detection of clustered CIB power at millimetre wavelengths, in South Pole Telescope (SPT) 3 data, soon followed by Dunkley et al (2011) in Atacama Cosmology Telescope (ACT) 4 data, and Shirokoff et al (2011) with additional SPT data. Most recently, measurements of the CIB fluctuation power, extending over a broad range in frequencies and angular scales, have been reported in Planck Collaboration (2011) and Amblard et al (2011), inferred from Planck and Herschel data, respectively 5 .…”