Cosmic Microwave Background Temperature at Galaxy Clusters

We have deduced the cosmic microwave background temperature in the Coma Cluster (A1656, z = 0.0231) and in A2163 ( z = 0.203) from spectral measurements of the Sunyaev-Zeldovich (SZ) effect over four passbands at radio and microwave frequencies. The resulting temperatures at these redshifts are T Coma = 2.789 K and T A2163 = 3.377 K, respectively. These values confirm the expected relation T ( z ) = T 0 (1 + z ), where T 0 = 2.725 ± 0.002 K is the value measured by the COBE Far Infrared Absolute Spectrometer experiment. Alternative scaling relations that are conjectured in nonstandard cosmologies can be constrained by the data; for example, if T ( z ) = T 0 (1 + z ) 1- a or T ( z ) = T 0 [1 + (1 + d ) z ], then a = -0.16 and d = 0.17 ± 0.36 (at 95% confidence). We briefly discuss future prospects for more precise SZ measurements of T ( z ) at higher redshifts.