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• W3125040452 abstract "We have made the largest-volume measurement to date of the transition to large-scale homogeneity in the distribution of galaxies. We use the WiggleZ survey, a spectroscopic survey of over 200,000 blue galaxies in a cosmic volume of ~1 (Gpc/h)^3. A new method of defining the 'homogeneity scale' is presented, which is more robust than methods previously used in the literature, and which can be easily compared between different surveys. Due to the large cosmic depth of WiggleZ (up to z=1) we are able to make the first measurement of the transition to homogeneity over a range of cosmic epochs. The mean number of galaxies N(<r) in spheres of comoving radius r is proportional to r^3 within 1%, or equivalently the fractal dimension of the sample is within 1% of D_2=3, at radii larger than 71 pm 8 Mpc/h at z~0.2, 70 pm 5 Mpc/h at z~0.4, 81 pm 5 Mpc/h at z~0.6, and 75 pm 4 Mpc/h at z~0.8. We demonstrate the robustness of our results against selection function effects, using a LCDM N-body simulation and a suite of inhomogeneous fractal distributions. The results are in excellent agreement with both the LCDM N-body simulation and an analytical LCDM prediction. We can exclude a fractal distribution with fractal dimension below D_2=2.97 on scales from ~80 Mpc/h up to the largest scales probed by our measurement, ~300 Mpc/h, at 99.99% confidence." @default.
• W3125040452 created "2021-02-01" @default.
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• W3125040452 date "2012-07-26" @default.
• W3125040452 modified "2023-10-17" @default.
• W3125040452 title "The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity" @default.
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• W3125040452 cites W1871723080 @default.
• W3125040452 cites W1939864003 @default.
• W3125040452 cites W1944901286 @default.
• W3125040452 cites W1963611021 @default.
• W3125040452 cites W1963802336 @default.
• W3125040452 cites W1965973439 @default.
• W3125040452 cites W1969221502 @default.
• W3125040452 cites W1973240083 @default.
• W3125040452 cites W1976907621 @default.
• W3125040452 cites W1980276813 @default.
• W3125040452 cites W1980647430 @default.
• W3125040452 cites W1982364216 @default.
• W3125040452 cites W2001290456 @default.
• W3125040452 cites W2002185357 @default.
• W3125040452 cites W2004491479 @default.
• W3125040452 cites W2007173662 @default.
• W3125040452 cites W2015920480 @default.
• W3125040452 cites W2025634246 @default.
• W3125040452 cites W2027337393 @default.
• W3125040452 cites W2029109287 @default.
• W3125040452 cites W2029789017 @default.
• W3125040452 cites W2029965202 @default.
• W3125040452 cites W2031497590 @default.
• W3125040452 cites W2035399222 @default.
• W3125040452 cites W2040405503 @default.
• W3125040452 cites W2043913300 @default.
• W3125040452 cites W2047082467 @default.
• W3125040452 cites W2049741749 @default.
• W3125040452 cites W2051869499 @default.
• W3125040452 cites W2053057887 @default.
• W3125040452 cites W2056454413 @default.
• W3125040452 cites W2061357238 @default.
• W3125040452 cites W2066929508 @default.
• W3125040452 cites W2080645793 @default.
• W3125040452 cites W2087470333 @default.
• W3125040452 cites W2093612453 @default.
• W3125040452 cites W2095511138 @default.
• W3125040452 cites W2109204822 @default.
• W3125040452 cites W2113513599 @default.
• W3125040452 cites W2113869105 @default.
• W3125040452 cites W2117363750 @default.
• W3125040452 cites W2121951791 @default.
• W3125040452 cites W2128759530 @default.
• W3125040452 cites W2129119343 @default.
• W3125040452 cites W2147875900 @default.
• W3125040452 cites W2154376620 @default.
• W3125040452 cites W2155148078 @default.
• W3125040452 cites W2155711232 @default.
• W3125040452 cites W2157544440 @default.
• W3125040452 cites W2166967850 @default.
• W3125040452 cites W2171023349 @default.
• W3125040452 cites W2208922821 @default.
• W3125040452 cites W2903919837 @default.
• W3125040452 cites W3004198491 @default.
• W3125040452 cites W3099172066 @default.
• W3125040452 cites W3099582894 @default.
• W3125040452 cites W3099712500 @default.
• W3125040452 cites W3100028230 @default.
• W3125040452 cites W3100897521 @default.
• W3125040452 cites W3101274643 @default.
• W3125040452 cites W3101500842 @default.
• W3125040452 cites W3102293147 @default.

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