Imaging the Thermal and Kinematic Sunyaev–Zel’dovich Effect Signals in a Sample of 10 Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities

@article{Sayers2019ImagingTT,
  title={Imaging the Thermal and Kinematic Sunyaev–Zel’dovich Effect Signals in a Sample of 10 Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities},
  author={Jack Sayers and Alfredo Monta{\~n}a and Tony Mroczkowski and Grant W. Wilson and Michael Zemcov and Adi Zitrin and Nath'alia Cibirka and Sunil Golwala and David Hughes and Daisuke Nagai and Erik D. Reese and David S'anchez and John A. Zuhone},
  journal={The Astrophysical Journal},
  year={2019},
  volume={880}
}
We have imaged the Sunyaev–Zel’dovich (SZ) effect signals at 140 and 270 GHz toward 10 galaxy clusters with Bolocam and AzTEC/ASTE. We also used Planck data to constrain the signal at large angular scales, Herschel–SPIRE images to subtract the brightest galaxies that comprise the cosmic infrared background (CIB), Chandra imaging to map the electron temperature of the intra-cluster medium, and Hubble Space Telescope imaging to derive models of each galaxy cluster’s mass density. The galaxy… 
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