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TIME AND SPACE
Reproducing the large-scale Universe
by Staff Writers
Potsdam, Germany (SPX) Feb 17, 2016


Pie plot of the BOSS DR12 observations (upper-left region) and one mock realization (lower-right region). Image courtesy F. Kitaura. For a larger version of this image please go here.

The BOSS survey has scanned the sky measuring the redshifts of more than 1 million galaxies, yielding a three dimensional picture of luminous sources in our Universe covering about 4.5 billion years. An international team of astronomers has now reproduced the observed galaxy clustering and determined the uncertainties in the measurement of observed quantities by generating thousands of simulated galaxy catalogues.

For the first time, the separation between pairs of galaxies, and the separation between triplets of galaxies has been explicitly constrained to reproduce the observations. Hence, the cosmic web in particular the empty regions between galaxies are described.

The distribution of galaxies on very large scales encodes valuable information about the origin and fate of the Universe. To study this, the Baryon Oscillation Spectroscopic Survey (BOSS), a branch of the Sloan Digital Sky Survey (SDSS-III), has measured the redshift distribution of galaxies with unprecedented accuracy.

One important question arises in the analysis of the data provided by such surveys: if the Universe is comparable to a huge unique experiment, how can we determine the uncertainties in the measurement of quantities derived from observing it?

While common experiments can be repeated an arbitrary number of times in the laboratory, the cosmic Universe is only reproducible in super-computing facilities. One needs to consider the statistical fluctuations caused by the so-called cosmic variance, having its origin in the primordial seed fluctuations.

However, reconstructing the large-scale structure covering the volumes of a survey like BOSS from the fluctuations generated after the Big Bang until the formation of the observed galaxies after about 14 billion years of cosmic evolution is an extremely expensive task, requiring millions of super-computing hours.

Francisco Kitaura from the Leibniz Institute for Astrophysics Potsdam (AIP) states: "We have developed the necessary techniques to generate thousands of simulated galaxy catalogues, reproducing the statistical properties of the observations."

The production of the catalogues followed three steps: first, thousands of Dark Matter fields were generated with different seed perturbations at different cosmic epochs. Second, the galaxies were distributed in a nonlinear, stochastic way matching the statistical properties of the observations.

Third, the mass of each galaxy - determined by its environment - was reconstructed. Finally, the catalogues of different cosmic times were combined into light cones reproducing the observational properties of the BOSS data, such as the survey geometry, and galaxy number density at different distances and lookback times.

Chia-Hsun Chuang from the AIP explains: "With this novel approach we are able to reliably constrain the errors to the cosmological parameters we extract from the data".

"The MareNostrum super-computing facility at the Barcelona Supercomputing Center (BSC) was used to produce the largest number of synthetic galaxy catalogues to date covering a volume more than ten times larger than the sum of all the large volume simulations carried out so far", reports Gustavo Yepes from the Autonomous University of Madrid (UAM).

The statistical properties extracted from the data and compared to the models have helped gain new insights: "Now we understand better the relation between the galaxy distribution and the underlying large-scale Dark Matter field. We will continue refining our methods to further understand the structures we observe in the Universe", concludes Kitaura.

Publication: Kitaura, Francisco-Shu et al. 2016: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release, in Monthly Notices of the Royal Astronomical Society, Vol. 456.

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