Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope
F. De Bernardis, S. Aiola, E. M. Vavagiakis, N. Battaglia, M. D., Niemack, J. Beall, D. T. Becker, J. R. Bond, E. Calabrese, H. Cho, K., Coughlin, R. Datta, M. Devlin, J. Dunkley, R. Dunner, S. Ferraro, A. Fox, P., A. Gallardo, M. Halpern, N. Hand, M. Hasselfield

TL;DR
This paper measures the pairwise kinematic Sunyaev-Zel'dovich effect using ACT and BOSS data, revealing large-scale halo motions with significant statistical confidence, and compares optical depth estimates from different methods.
Contribution
First measurement of the pairwise kinematic Sunyaev-Zel'dovich effect using ACT and BOSS data, with detailed error analysis and systematic considerations.
Findings
Detected a non-zero pairwise kSZ signal with S/N between 3.6 and 4.1.
Optical depth estimates from kSZ are consistent with thermal SZ measurements.
Error estimates vary depending on the method, affecting the significance of the detection.
Abstract
We present a new measurement of the kinematic Sunyaev-Zeldovich effect using data from the Atacama Cosmology Telescope (ACT) and the Baryon Oscillation Spectroscopic Survey (BOSS). Using 600 square degrees of overlapping sky area, we evaluate the mean pairwise baryon momentum associated with the positions of 50,000 bright galaxies in the BOSS DR11 Large Scale Structure catalog. A non-zero signal arises from the large-scale motions of halos containing the sample galaxies. The data fits an analytical signal model well, with the optical depth to microwave photon scattering as a free parameter determining the overall signal amplitude. We estimate the covariance matrix of the mean pairwise momentum as a function of galaxy separation, using microwave sky simulations, jackknife evaluation, and bootstrap estimates. The most conservative simulation-based errors give signal-to-noise estimates…
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