Imaging the Sunyaev-Zeldovich Effect in the High Redshift Galaxy Cluster MS1137+66

Details Imaging the Sunyaev-Zeldovich Effect in the High Redshift Galaxy Cluster MS1137+66 Imaging the Sunyaev-Zeldovich Effect in the High Redshift Galaxy Cluster MS1137+66

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.1005j&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #10.05; Bulletin of the American Astronomical Society, Vol. 31, p.1388

Astronomy and Astrophysics

Astronomy

Scientific paper

We present interferometric measurements of the Sunyaev-Zel'dovich Effect (SZE) in MS1137+66, a distant galaxy cluster at a redshift of 0.78. The data were obtained in 1997 and 1998 at the Berkeley-Illinois-Maryland millimeter array using sensitive 28.5 GHz receivers optimized for imaging of the SZE, with a total on-source integration time of 87.8 hours. We discuss constraints derived from spherical β model fits to the SZE data, place an upper limit on the strength of any possible radio point sources in the field, and compare the results with the x-ray data published by Donahue et al. in 1999.

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