Cavendish Astrophysics Publications for topic : Cosmic microwave background

1. Chon, G., Challinor, A., Prunet, S., Hivon, E., Szapudi, I., 1900. Fast estimation of polarization power spectra using correlation functions. MNRAS, submitted.

2. Kneissl, R., 2002. Cosmological constraints from SZ. The Cosmological Model.

3. Kneissl, R., 2001. H_0 from X-ray and Ryle Telescope observations and prospects for the Arcminute MicroKelvin Imager. Clusters of galaxies and the high redshift universe observed in X-rays, Neumann D.M., Tranh Thanh Van J., CEA. Link

4. Kneissl, R., Jones, M.E., 2002. SZ Surveys with the Arcminute MicroKelvin Imager. Tracing the Cosmic Evolution with Galaxy Clusters, Borgani S., Mezzetti M., Valdarnini R., ASP, 268, 113.

5. Kneissl, R., 2003. High redshift Sunyaev-Zel'dovich clusters and XEUS. XEUS - studying the evolution of the hot universe, Hasinger G., Boller Th., Parmer A.N., MPE Report, 281, 49.

6. Weller, J., Battye, R.A., Kneissl, R., 2002. Constraining Dark Energy with Sunyaev-Zel'dovich Cluster Surveys. Physical Review Letters, 88, 231301.

7. Taylor, A.C., 2001. The radio source population at 15 GHz. XXXIIIrd Recontres de Moriond, Editions Frontiers.

8. Taylor, A.C., 2001. Radio source counts at 15 GHz: Implications for CMB experiments. IAU Symposium no. 201, ASP, in press.

9. Taylor, A.C., 2001. The Very Small Array. NAM 2001.

10. Taylor, A.C., 2002. The Very Small Array. 2K1BC Workshop: "Experimental Cosmology at millimetre wavelengths", 72.

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