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Observations of the Sunyaev–Zel'dovich effect in the z=0.78 cluster MS 1137.5+6625
Authors:Garret Cotter  Helen J Buttery  Rhiju Das†  Michael E Jones  Keith Grainge  G G Pooley  Richard Saunders
Institution:Astrophysics, Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE
Abstract:We have observed the   z =0.78  cluster MS 1137.5+6625 with the Ryle Telescope (RT) at 15 GHz. After subtraction of contaminating radio sources in the field, we find a Sunyaev–Zel'dovich flux decrement of  -421±60 μJy  on the ≈0.65 k λ baseline of the RT, spatially coincident with the optical and X-ray positions for the cluster core.
For a spherical King-profile cluster model, the best fit to our flux measurement has a core radius   θ C=20 arcsec  , consistent with previous X-ray observations, and a central temperature decrement  Δ T =650±92 μK  .
Using this model, we calculate that the cluster has a gas mass inside a     radius of  2.9×1013 M  for an  Ω M =1  universe and  1.6×1013 M  for  Ω M =0.3  ,  ΩΛ=0.7  . We compare this model with existing measurements of the total mass of the cluster, based on gravitational lensing, and estimate a gas fraction for MS 1137.5+6625 of ≈8 per cent.
Keywords:galaxies: clusters: individual: MS 1137  5+6625  cosmology: observations
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