We compare cosmic microwave background lensing convergence maps derived from South Pole Telescope (SPT) data with galaxy survey data from the Blanco Cosmology Survey, WISE, and a new large Spitzer/IRAC field designed to overlap with the SPT survey. Using optical and infrared catalogs covering between 17 and 68deg2 of sky, we detect a correlation between the SPT convergence maps and each of the galaxy density maps at >4σ, with zero correlation robustly ruled out in all cases. The amplitude and shape of the cross-power spectra are in good agreement with theoretical expectations and the measured galaxy bias is consistent with previous work. The detections reported here utilize a small fraction of the full 2500deg2 SPT survey data and serve as both a proof of principle of the technique and an illustration of the potential of this emerging cosmological probe. © 2012. The American Astronomical Society. All rights reserved..
CITATION STYLE
Bleem, L. E., Van Engelen, A., Holder, G. P., Aird, K. A., Armstrong, R., Ashby, M. L. N., … Zahn, O. (2012). A measurement of the correlation of galaxy surveys with CMB lensing convergence maps from the south pole telescope. Astrophysical Journal Letters, 753(1). https://doi.org/10.1088/2041-8205/753/1/L9
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