CIB power spectra in Sections \[sec:tszinterp\], \[sec:kszinterp\], \[sec:tszcibinterp\], and \[sec:cibinterp\] respectively. We conclude in Section \[sec:conclusions\].

Data and analysis {#sec:dataanalysis}
=================

We present power spectra from 2540 square degrees of SPT data at 95, 150, and 220GHz. Power spectra are estimated using a pseudo-${\it C}_\ell$ cross-spectrum method [@hivon02; @polenta05; @tristram05]. We calibrate the data by comparing the power spectrum to *Planck* 1-year CMB power spectrum [@planck13-15].

Data {#subsec:data}
----

The 2540 [deg$^2$]{} of sky analyzed in this work were observed with the [SPT-SZ]{} camera on the SPT from 2008 to 2011. The full survey was divided into 19 contiguous sub-patches, referred to as fields, for observations. The specific field locations and extents can be found in Table 1 of @story13, hereafter S13. The [SPT-SZ]{} camera consists of 960 horn-coupled spiderweb bolometers with superconducting transition edge sensors and was installed on the 10-meter SPT from 2007-2011. The telescope, receiver, and detectors are discussed in more detail in @ruhl04, @padin08, @shirokoff09, and @carlstrom11.

Seventeen of the 19 fields were observed to an approximate depth of 18 $\mu$K-arcmin at 150GHz. The noise levels at 95 and 220GHz vary significantly between 2008 and subsequent years as the focal plane was refurbished to maximize sensitivity 