The 2dF galaxy redshift survey: Hierarchical galaxy clustering by Baugh, C, Croton, D, Gaztañaga, E, Norberg, P, Colless, M, Baldry, I, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D

The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering by Baugh, C, Croton, D, Gaztanaga, E, Norberg, P, Colless, M, Baldry, I, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D

The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering by Norberg, P, Baugh, C, Hawkins, E, Maddox, S, Peacock, J, Cole, S, Frenk, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Madgwick, D, Peterson, B

The 2dF galaxy redshift survey: Luminosity dependence of galaxy clustering by Norberg, P, Baugh, C, Hawkins, E, Maddox, S, Peacock, J, Cole, S, Frenk, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Madgwick, D, Peterson, B

“…We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). …”

The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type by Madgwick, D, Hawkins, E, Lahav, O, Maddox, S, Norberg, P, Peacock, J, Baldry, I, Baugh, C, Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lewis, I, Lumsden, S

The 2dF Galaxy Redshift Survey: Galaxy clustering per spectral type by Madgwick, D, Hawkins, E, Lahav, O, Maddox, S, Norberg, P, Peacock, J, Baldry, I, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lewis, I, Lumsden, S

The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type by Norberg, P, Baugh, C, Hawkins, E, Maddox, S, Madgwick, D, Lahav, O, Cole, S, Frenk, C, Baldry, I, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Glazebrook, K, Jackson, C, Lewis, I, Lumsden, S, Peacock, J

The 2dF galaxy redshift survey: Correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey by Hilton, M, Collins, C, De Propris, R, Baldry, I, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Couch, W, Dalton, G, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D, Norberg, P, Peacock, J

“…The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and the Two-degree Field Galaxy Redshift Survey (2dFGRS), respectively, comprise the largest, homogeneous X-ray selected cluster catalogue and completed galaxy redshift survey. …”

The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey by Hilton, M, Collins, C, De Propris, R, Baldry, I, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Couch, W, Dalton, G, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D, Norberg, P, Peacock, J

KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering by Joudaki, S, Blake, C, Johnson, A, Amon, A, Asgari, M, Choi, A, Erben, T, Glazebrook, K, Harnois-Déraps, J, Heymans, C, Hildebrandt, H, Hoekstra, H, Klaes, D, Kuijken, K, Lidman, C, Mead, A, Miller, L, Parkinson, D, Poole, G, Schneider, P, Viola, M, Wolf, C

The 2dF galaxy redshift survey: Voids and hierarchical scaling models by Croton, D, Colless, M, Gaztañaga, E, Baugh, C, Norberg, P, Baldry, I, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D

“…The reduced VPF measured from the 2dFGRS is in excellent agreement with the paradigm of hierarchical scaling of the galaxy clustering moments. The accuracy of our measurement is such that we can rule out, at a very high significance, popular models for galaxy clustering, including the lognormal distribution. …”

The science case for PILOT II: The distant universe by Lawrence, J, Ashley, M, Burton, MG, Storey, J, Bunker, A, Saunders, W, Bouwens, R, Burgarella, D, Gehrels, N, Glazebrook, K, Pimbble, K, Quimby, R, Wheeler, J

“…Two projects are proposed to examine the assembly and evolution of structure in the Universe: an infrared survey searching for the first evolved galaxies at high redshift, and an optical survey aimed at characterising moderate-redshift galaxy clusters. Finally, a large-area weak-lensing survey and a program to obtain supernova infrared light-curves are proposed to examine the nature and evolution of dark energy and dark matter. © Astronomical Society of Australia 2009.…”

KiDS+2dFLenS+GAMA: testing the cosmological model with the E-G statistic by Amon, A, Blake, C, Heymans, C, Leonard, C, Asgari, M, Bilicki, M, Choi, A, Erben, T, Glazebrook, K, Harnois-Deraps, J, Hildebrandt, H, Hoekstra, H, Joachimi, B, Joudaki, S, Kuijken, K, Lidman, C, Loveday, J, Parkinson, D, Valentijn, E, Wolf, C

“…We present a new measurement of EG, which combines measurements of weak gravitational lensing, galaxy clustering, and redshift-space distortions. This statistic was proposed as a consistency test of General Relativity (GR) that is insensitive to linear, deterministic galaxy bias, and the matter clustering amplitude. …”

The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters by Lewis, I, Balogh, M, De Propris, R, Couch, W, Bower, R, Offer, A, Bland-Hawthorn, J, Baldry, I, Baugh, C, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Cross, N, Dalton, G, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Hawkins, E, Jackson, C, Lahav, O, Lumsden, S

“…We have measured the equivalent width of the Ha emission line for 11 006 galaxies brighter than Mb, = -19 (ΩΛ = 0.7, Ωm = 0.3, H0 = 70 km s-1 Mpc-1) at 0.05 < z < 0.1 in the 2dF Galaxy Redshift Survey (2dFGRS), in the fields of 17 known galaxy clusters. The limited redshift range ensures that our results are insensitive to aperture bias, and to residuals from night sky emission lines. …”

The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe by Hawkins, E, Maddox, S, Cole, S, Lahav, O, Madgwick, D, Norberg, P, Peacock, J, Baldry, I, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Jones, B, Lewis, I

“…The large size of the catalogue, which contains ∼220 000 redshifts, allows us to make high-precision measurements of various properties of the galaxy clustering pattern. The effective redshift at which our estimates are made is z s ≈ 0.15, and similarly the effective luminosity, L s ≈ 1.4L*. …”