The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity
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Scott Croom | Karl Glazebrook | Gregory Poole | Karl Forster | Rob Sharp | David Gilbank | Lister Staveley-Smith | Darren Croton | Chris Blake | Sarah Brough | Michael J. Drinkwater | Russell J. Jurek | Warrick Couch | Tamara Davis | S. Brough | T. Davis | B. Madore | J. B. James | C. Blake | C. Contreras | K. Glazebrook | W. Couch | R. Sharp | S. Croom | M. Pracy | D. Croton | M. Drinkwater | M. Colless | R. Jurek | L. Staveley-Smith | K. Pimbblet | M. Gladders | H. Yee | K. Forster | T. Wyder | D. Gilbank | G. Poole | David Woods | Carlos Contreras | Matthew Colless | Howard Yee | Barry Madore | Chris Martin | Michael Pracy | Ben Jelliffe | I. Li | E. Wisnioski | D. Woods | Ben Jelliffe | I-hui Li | Emily Wisnioski | Ted Wyder | Morag Scrimgeour | J. Berian James | Mike Gladders | Kevin Pimbblet | Morag I. Scrimgeour | M. Gladders | C. Martin
[1] Scott Croom,et al. The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations , 2011, 1108.2635.
[2] A. Heavens,et al. Testing homogeneity with the fossil record of galaxies , 2011, 1107.5910.
[3] M. Bruni,et al. Redshift and distances in a ΛCDM cosmology with non-linear inhomogeneities , 2011, 1107.4433.
[4] Matthew Colless,et al. The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant , 2011, 1106.3366.
[5] Scott Croom,et al. The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9 , 2011, 1104.2948.
[6] S. Räsänen. Backreaction: directions of progress , 2011 .
[7] M. Sullivan,et al. SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY , 2011, 1104.1443.
[8] R. Nichol,et al. THE EFFECT OF PECULIAR VELOCITIES ON SUPERNOVA COSMOLOGY , 2010, 1012.2912.
[9] Matthew Colless,et al. The WiggleZ Dark Energy Survey: the selection function and z = 0.6 galaxy power spectrum , 2010, 1003.5721.
[10] Nishikanta Khandai,et al. Fractal dimension as a measure of the scale of homogeneity , 2010, 1001.0617.
[11] A. Shafieloo,et al. Model independent tests of the standard cosmological model , 2009, 0911.4858.
[12] Alexander S. Szalay,et al. Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample , 2009, 0907.1660.
[13] Karl Glazebrook,et al. The WiggleZ Dark Energy Survey: survey design and first data release , 2009, 0911.4246.
[14] D. Wiltshire. Average observational quantities in the timescape cosmology , 2009, 0909.0749.
[15] Y. Baryshev,et al. Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey – Data release six , 2009, 0909.0132.
[16] J. Yadav,et al. The scale of homogeneity of the galaxy distribution in SDSS DR6 , 2009, 0906.3431.
[17] S. Brough,et al. The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 , 2009, 0901.2587.
[18] K. Land,et al. Living in a void: testing the Copernican principle with distant supernovae. , 2008, Physical review letters.
[19] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[20] T. R. Seshadri,et al. Fractal dimensions of a weakly clustered distribution and the scale of homogeneity , 2007, 0712.2905.
[21] G. Robbers,et al. Cosmological backreaction from perturbations , 2007, 0710.4964.
[22] D. Wiltshire. Exact solution to the averaging problem in cosmology. , 2007, Physical review letters.
[23] T. Buchert. Dark Energy from structure: a status report , 2007, 0707.2153.
[24] D. Wiltshire. Cosmic clocks, cosmic variance and cosmic averages , 2007, gr-qc/0702082.
[25] D. Schwarz,et al. Onset of cosmological backreaction , 2007, gr-qc/0702043.
[26] N. Tetradis,et al. The effect of large scale inhomogeneities on the luminosity distance , 2006, astro-ph/0612179.
[27] S. Rasanen. Accelerated expansion from structure formation , 2006, astro-ph/0607626.
[28] G. Ellis,et al. The universe seen at different scales , 2005, gr-qc/0506106.
[29] India.,et al. Testing homogeneity on large scales in the Sloan Digital Sky Survey Data Release One , 2005, Monthly Notices of the Royal Astronomical Society.
[30] R. Nichol,et al. Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies , 2005, astro-ph/0501171.
[31] Neta A. Bahcall,et al. Cosmic Homogeneity Demonstrated with Luminous Red Galaxies , 2004, astro-ph/0411197.
[32] S. Matarrese,et al. Effect of inhomogeneities on the expansion rate of the universe , 2004, Physical Review D.
[33] J. Frieman,et al. The Luminosity and Color Dependence of the Galaxy Correlation Function , 2004, astro-ph/0408569.
[34] I. Hook,et al. A high abundance of massive galaxies 3–6 billion years after the Big Bang , 2004, Nature.
[35] N. Afshordi. Integrated Sachs-Wolfe effect in cross-correlation: The observer's manual , 2004, astro-ph/0401166.
[36] J. Brinkmann,et al. A Map of the Universe , 2003, astro-ph/0310571.
[37] R. Ellis,et al. The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe , 2002, astro-ph/0212375.
[38] J. Peacock,et al. Stable clustering, the halo model and non-linear cosmological power spectra , 2002, astro-ph/0207664.
[39] Jean-Luc Starck,et al. Astronomical Data Analysis II , 2002 .
[40] D. Schwarz. Accelerated expansion without dark energy , 2002, astro-ph/0209584.
[41] Vicent J. Martinez,et al. Clustering statistics in cosmology , 2002, SPIE Astronomical Telescopes + Instrumentation.
[42] C. Blake,et al. Detection of the velocity dipole in the radio galaxies of the NRAO VLA Sky Survey , 2002, astro-ph/0203385.
[43] Chris Blake,et al. A velocity dipole in the distribution of radio galaxies , 2002, Nature.
[44] P. Coles,et al. Boundary corrections in fractal analysis of galaxy surveys , 2001, astro-ph/0111234.
[45] A. Gabrielli,et al. Glass-like universe: Real-space correlation properties of standard cosmological models , 2001, astro-ph/0110451.
[46] Masahiro Morikawa,et al. Scaling analysis of galaxy distribution in the Las Campanas Redshift Survey data , 2001 .
[47] V. Springel,et al. GADGET: a code for collisionless and gasdynamical cosmological simulations , 2000, astro-ph/0003162.
[48] P. Coles,et al. Large‐scale cosmic homogeneity from a multifractal analysis of the PSCz catalogue , 2000, astro-ph/0008240.
[49] M. Montuori,et al. Fractal cosmology in an open universe , 2000, astro-ph/0002504.
[50] Cambridge,et al. The 2-10 keV X-Ray Background Dipole and Its Cosmological Implications , 1999, astro-ph/9908187.
[51] A. Lewis,et al. Efficient computation of CMB anisotropies in closed FRW models , 1999, astro-ph/9911177.
[52] T. Buchert. On Average Properties of Inhomogeneous Fluids in General Relativity: Dust Cosmologies , 1999, gr-qc/9906015.
[53] L. Amendola,et al. The Scale of Homogeneity in the Las Campanas Redshift Survey , 1999, astro-ph/9901420.
[54] M. Montuori,et al. Fractal Correlations in the CfA2-South Redshift Survey , 1999, astro-ph/9901290.
[55] O. Lahav,et al. The large-scale smoothness of the Universe , 1998, Nature.
[56] M. Graham,et al. Searching for the scale of homogeneity , 1998, astro-ph/9804073.
[57] M. Montuori,et al. Scale-invariance of galaxy clustering , 1997, astro-ph/9711073.
[58] S. Cole,et al. Modelling the redshift-space distortion of galaxy clustering , 1997, astro-ph/9707186.
[59] D. Weinberg,et al. Constraints on the Effects of Locally Biased Galaxy Formation , 1997, astro-ph/9712192.
[60] L. Guzzo,et al. Is the universe homogeneous? (On large scales) , 1997, astro-ph/9711206.
[61] N. Turok. Critical Dialogues in Cosmology , 1997 .
[62] M. Montuori,et al. On the Fractal Structure of the Visible Universe , 1996, astro-ph/9611197.
[63] L. Cowie,et al. New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields , 1996, astro-ph/9606079.
[64] E. L. Wright,et al. The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set , 1996, astro-ph/9605054.
[65] K. Fisher. On the validity of the streaming model for the redshift space correlation function in the linear regime , 1994, astro-ph/9412081.
[66] S. Borgani. Scaling in the Universe , 1994, astro-ph/9404054.
[67] P. Coles,et al. Correlations and Scaling in the QDOT Redshift Survey , 1994 .
[68] L. Guzzo,et al. Clustering properties from finite galaxy samples , 1994 .
[69] J. A. PeacockS.J. Dodds,et al. Reconstructing the linear power spectrum of cosmological mass fluctuations , 1993, astro-ph/9311057.
[70] A. Hamilton. Toward Better Ways to Measure the Galaxy Correlation Function , 1993 .
[71] A. Szalay,et al. Bias and variance of angular correlation functions , 1993 .
[72] P. Coles. Galaxy formation with a local bias , 1993 .
[73] P. Peebles. Principles of Physical Cosmology , 1993 .
[74] Luciano Pietronero,et al. The fractal structure of the universe , 1992 .
[75] A. Hamilton. Measuring Omega and the real correlation function from the redshift correlation function , 1992 .
[76] G. Lemson,et al. On the use of the conditional density as a description of galaxy clustering , 1991 .
[77] A. Kashlinsky,et al. Large-scale structure in the Universe , 1991, Nature.
[78] B. Jones,et al. A lognormal model for the cosmological mass distribution. , 1991 .
[79] J. Huchra,et al. Mapping the Universe , 1989, Science.
[80] J. Huchra,et al. The Luminosity Function for the CfA Redshift Survey Slices , 1989 .
[81] N. Kaiser. Clustering in real space and in redshift space , 1987 .
[82] N. Kaiser. On the spatial correlations of Abell clusters , 1984 .
[83] B. Ripley. Modelling Spatial Patterns , 1977 .
[84] R. Sachs,et al. Perturbations of a Cosmological Model and Angular Variations of the Microwave Background , 1967 .