Showing results 1 - 8 of 8.
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| Title | Authors | Year | Publication Type | Full Text | Peer Reviewed |
|---|---|---|---|---|---|
| The 2dF Galaxy Redshift Survey: constraints on cosmic star formation history from the cosmic spectrum | Baldry, Ivan K.; Glazebrook, Karl; Baugh, Carlton; Bland-Hawthorn, Joss; Bridges, Terry J.... More | 2002 | Journal article | ||
| The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing | Lahav, Ofer; Bridle, Sarah; Percival, Will J.; Peacock, John A.; Efstathiou, George P.... More | 2002 | Journal article | ||
| The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe | Verde, Licia; Heavens, Alan F.; Percival, Will J.; Matarrese, Sabino; Baugh, Carlton... More | 2002 | Journal article | ||
| The 2dF Galaxy Redshift Survey: the bJ-band galaxy luminosity function and survey selection function | Norberg, Peder; Cole, Shaun; Baugh, Carlton; Frenk, Carlos S.; Baldry, Ivan K.... More | 2002 | Journal article | ||
| The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type | Norberg, Peder; Baugh, Carlton; Hawkins, Edward; Maddox, Stephen J.; Madgwick, Darren... More | 2002 | Journal article | ||
| The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters | Lewis, Ian; Balogh, Michael L.; De Propris, Roberto; Couch, Warrick J.; Bower, Richard G.... More | 2002 | Journal article | ||
| Evidence for a non-zero Lambda and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and cosmic microwave background anisotropies | Efstathiou, George P.; Moody, Stephen J.; Peacock, John A.; Percival, Will J.; Baugh, Carlton... More | 2002 | Journal article | ||
| Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra | Percival, Will J.; Sutherland, William J.; Peacock, John A.; Baugh, Carlton; Bland-Hawthorn, Joss... More | 2002 | Journal article |
