Cavendish Astrophysics Publications for topic : Cosmic microwave background

  1. Mortlock, D., Challinor, A., Hobson, M., 2001. Analysis of cosmic microwave background data on an incomplete sky. MNRAS, 330, 405. Link

  2. Challinor, A., Fosalba, P., Mortlock, D., Ashdown, M., Wandelt, B., Gorski, K., 2000. All-sky convolution for polarimetry experiments. Phys. Rev. D, 62, 123002. Link

  3. Lewis, A., Challinor, A., Lasenby, A., 2000. Efficient computation of CMB anisotropies in closed FRW models. ApJ, 538, 473. Link

  4. Challinor, A., 2000. Microwave background polarization in cosmological models. Phys. Rev. D, 62, 043004. Link

  5. Challinor, A., 2000. Microwave background anisotropies from gravitational waves: the 1+3 covariant approach. Class. Quantum. Grav., 17, 871. Link

  6. Challinor, A., Ford, M., Lasenby, A., 2000. Thermal and kinematic corrections to the microwave background polarization induced by galaxy clusters along the line of sight. MNRAS, 312, 159. Link

  7. Challinor, A., 2000. The covariant perturbative approach to cosmic microwave background anisotropies. Gen. Rel. Grav., 32, 1059. Link

  8. Saunders, R., 1993. Correlators for cosmic microwave background astronomy. New Generation Digital Correlators, D. Emerson, NRAO, 59.

  9. Grainge, K., Jones, M., Saunders, R., Pooley, G., Edge, A., Kneissl, R., 2002. Measuring the Hubble Constant from Ryle Telescope and X-ray observations, with application to A1413. MNRAS, 333, 318.

  10. Kneissl, R., Sunyaev, R.A., White, S.D.M., 1998. A deep ROSAT PSPC observation towards the CMB decrement close to PC1643+4631 A & B: no cluster X-ray emission. MNRAS, 297, L29-L33. Link

[ Previous page | Next page ]

[ Astrophysics Home | Publications | Subject List ]


Last modified Friday 28 March 2003
Webpage Administrator.