196 citations · 1.8k across the 42 of their papers we have counts for
42 papers
The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
Metin Ata, Francisco-Shu Kitaura, Chia-Hsun Chuang +31
We present a Bayesian phase-space reconstruction of the cosmic large-scale matter density and velocity fields from the SDSS-III Baryon Oscillations Spectroscopic Survey Data Releas…
Exploring 21cm - Lyman Alpha emitter synergies for SKA
Anne Hutter, Pratika Dayal, Volker Müller +1
We study the signatures of reionization and ionizing properties of the early galaxies in the cross-correlations between the 21cm emission from the spin-flip transition of neutral h…
4MOST - 4m Multi Object Spectroscopic Telescope
Eric Depagne, the 4MOST consortium
4MOST (4m Multi Object Spectroscopic Telescope) is a spectroscopic facility that will be installed on ESO's VISTA around 2020. The science rationale of this facility are to be foun…
Bayesian inference of cosmic density fields from non-linear, scale-dependent, and stochastic biased tracers
Metin Ata, Francisco-Shu Kitaura, Volker Müller
We present a Bayesian reconstruction algorithm to generate unbiased samples of the underlying dark matter field from halo catalogues. Our new contribution consists of implementing…
Non-Gaussian inference from non-linear and non-Poisson biased distributed data
Metin Ata, Francisco-Shu Kitaura, Volker Müller
We study the statistical inference of the cosmological dark matter density field from non-Gaussian, non-linear and non-Poisson biased distributed tracers. We have implemented a Bay…
The cosmic web of the Local Universe: cosmic variance, matter content and its relation to galaxy morphology
Sebastian E. Nuza, Francisco-Shu Kitaura, Steffen Hess +2
We present, for the first time, a Local Universe (LU) characterization using high precision constrained -body simulations based on self-consistent phase-space reconstructions of…
The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
A. Hutter, P. Dayal, A. M. Partl +1
We build a physical model for high-redshift Lyman Alpha emitters (LAEs) by coupling state of the art cosmological simulations (GADGET-2) with a dust model and a radiative transfer…
Simulating extremely metal-poor gas and DLA metal content at redshift z=7
Umberto Maio, Benedetta Ciardi, Volker Mueller
We present the first theoretical study of metals in damped Ly-alpha (DLA) systems at redshift z=7. The features of cold, primordial gas are studied by means of N-body, hydro, chemi…
The evolution of HI and CIV quasar absorption line systems at 1.9 < z < 3.2
Tae-Sun Kim, Adrian M. Partl, Robert F. Carswell +1
We have investigated the distribution and evolution of ~3100 intergalactic HI absorbers with HI column densities log N(HI) = [12.75, 17.0] at 1.9 < z < 3.2, using 18 high resolutio…
4MOST - 4-metre Multi-Object Spectroscopic Telescope
Roelof S. de Jong, Olga Bellido-Tirado, Cristina Chiappini +82
The 4MOST consortium is currently halfway through a Conceptual Design study for ESO with the aim to develop a wide-field (>3 square degree, goal >5 square degree), high-multiplex (…
Measuring the Cosmic Web
Volker Mueller, Kai Hoffmann, Sebastian E. Nuza
A quantitative study of the clustering properties of the cosmic web as a function of absolute magnitude and colour is presented using the SDSS Data Release 7 galaxy survey. Mark co…
Large scale environmental bias of the QSO line of sight proximity effect
Adrian M. Partl, Volker Müller, Gustavo Yepes +1
We analyse the proximity zone of the intergalactic matter around high-redshift quasars in a cosmological environment. In a box of 64 h-1 Mpc base length we employ dark matter only…
Enabling parallel computing in CRASH
Adrian M. Partl, Antonella Maselli, Benedetta Ciardi +2
We present the new parallel version (pCRASH2) of the cosmological radiative transfer code CRASH2 for distributed memory supercomputing facilities. The code is based on a static dom…
Wavelet analysis of the formation of the cosmic web
J. Einasto, G. Hütsi, E. Saar +6
According to the modern cosmological paradigm galaxies and galaxy systems form from tiny density perturbations generated during the very early phase of the evolution of the Univers…
Cosmological radiative transfer for the line-of-sight proximity effect
Adrian M. Partl, Aldo Dall'Aglio, Volker Müller +1
We study the proximity effect in the Ly-a forest around high redshift quasars as a function of redshift and environment employing a set of 3D radiative transfer simulations. The an…
Toward understanding rich superclusters
M. Einasto, E. Saar, V. J. Martinez +10
We present a morphological study of the two richest superclusters from the 2dF Galaxy Redshift Survey (SCL126, the Sloan Great Wall, and SCL9, the Sculptor supercluster). We use Mi…
Luminosity function and density field of the Sloan and Las Campanas Redshift Survey
G. Hütsi, J. Einasto, D. L. Tucker +5
The luminosity function of galaxies of the Early Data Release of the Sloan Digital Sky Survey (SDSS) and the Las Campanas Redshift Survey (LCRS) is calculated. The luminosity funct…
Clusters and Superclusters in the Sloan Digital Sky Survey
J. Einasto, G. H"utsi, M. Einasto +5
Two-dimensional high-resolution density field of galaxies of the Early Data Release of the Sloan Digital Sky Survey with a smoothing lengths 0.8 h^{-1} Mpc is applied to extract cl…
Correlations in the orientations of galaxy clusters
Andreas Faltenbacher, Martin Kerscher, Stefan Gottloeber +1
The relative orientation of clusters' major elongation axes and clusters' angular momentum is studied using a large N-body simulation in a box of 500 Mpc/h base length for a standa…
Spatial distribution of galactic halos and their merger histories
Stefan Gottloeber, Martin Kerscher, Andrey V. Kravtsov +3
We use a novel statistical tool, the mark correlation functions (MCFs), to study clustering of galaxy-size halos as a function of their properties and environment in a high-resolut…
Numerical simulations of the cosmic star formation history
Y. Ascasibar, G. Yepes, S. Gottloeber +1
The cosmic star formation history in Cold Dark Matter dominated cosmological scenarios is studied by means of hydrodynamical numerical simulations. In particular, we explore a low…
The mass function of the Las Campanas loose groups of galaxies
P. Heinamki, J. Einasto, M. Einasto +3
We have determined the mass function of loose groups of galaxies in the Las Campanas Redshift Survey. Loose groups of galaxies in the LCRS range in mass from $M \sim 10^{12} {\rm M…
Void Scaling and Void Profiles in CDM Models
S. Arbabi-Bidgoli, V. Mueller
An analysis of voids using cosmological N-body simulations of cold dark matter models is presented. It employs a robust statistics of voids, that was recently applied to discrimina…
Optical and X-ray clusters as tracers of the supercluster-void network. III Distribution of Abell and APM clusters
M. Einasto, J. Einasto, E. Tago +3
We present a comparison of Abell and APM clusters of galaxies as tracers of the large scale structure of the Universe. We investigate selection functions of both cluster catalogs.…