Cavendish Astrophysics Publications for topic : Cosmology & large-scale star formation

  1. Cotter, G., Das, R., Buttery, H.J., Jones, M., Grainge, K., Grainger, W.F., Pooley, G.G., Saunders, R., 2002. Observations of the Sunyaev--Zel'dovich effect in the z = 0.78 cluster MS1137.5+6625. MNRAS, 334, 323-326. Link

  2. Cotter, G., 1998. The cosmic evolution of giant radiosources. Observational Cosmology with the new radio surveys, M.N. Bremer, N. Jackson, I. Perez-Fourno, Kluwer, ASSL, 226, 233-238.

  3. Magliochetti, M., Maddox, S.J., Wall, J.V., Benn, C.R., Cotter, G., 2000. The redshift distribution of FIRST radio sources at 1mJy. MNRAS, 318, 1047-1067. Link

  4. Cotter, G., Haynes, T., Baker, J.C., Jones, M.E., Saunders, R., 1999. Completeness and confusion in the identification of Lyman-break galaxies. The Hy-redshift Universe: Galaxy Formation and Evolution at High Redshift, Andrew J. Bunker and Wil M. van Breugel, ASP, 193, 513.

  5. Kneissl, R., Jones, M.E., Saunders, R., Eke, V.R., Lasenby, A.N., Grainge, K., Cotter, G., 2001. Surveying the Sky with the Arcminute Micro-Kelvin Imager: Expected Constraints on Galaxy Cluster Evolution and Cosmology. MNRAS, 328, 783-794.

  6. Grainge, K., 2003. The Very Small Array. Ninth Marcel Grossman Meeting, Vahe Gurzadyan , Robert Jantzen, Remo Ru, World Scientific.

  7. Grainge, K., 2000. Foreground Sources and the VSA. Rencontres de Morionde, Energy densities in the Universe.

  8. Bridle, S.L., Hobson, M.P., Saunders, R., Lasenby, A., 2003. Maximum-entropy reconstruction of gravitational lenses using shear and/or magnification data. MNRAS, in press.

  9. Jarvis, M.J., Rawlings, S., Lacy, M., Blundell, K.M., Bunker, A.J., Eales, S., Saunders, R., Spinrad, H., Stern, D., Willott, C.J., 2001. A sample of 6C radio sources designed to find objects at redshift > 4: II -spectroscopy and emission-line properties. MNRAS, 326, 1563-1584.

  10. Longair, M.S., 2001. The Technology of Cosmology. Historical Development of Modern Cosmology, V. Martinez and V. Trimble, ASP, 252, 55.

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