The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations

We present the online MultiDark Database -- a Virtual Observatory-oriented, relational database for hosting various cosmological simulations. The data is accessible via an SQL (Structured Query Language) query interface, which also allows users to directly pose scientific questions, as shown in a number of examples in this paper. Further examples for the usage of the database are given in its extensive online documentation (www.multidark.org). The database is based on the same technology as the Millennium Database, a fact that will greatly facilitate the usage of both suites of cosmological simulations. The first release of the MultiDark Database hosts two 8.6 billion particle cosmological N-body simulations: the Bolshoi (250/h Mpc simulation box, 1/h kpc resolution) and MultiDark Run1 simulation (MDR1, or BigBolshoi, 1000/h Mpc simulation box, 7/h kpc resolution). The extraction methods for halos/subhalos from the raw simulation data, and how this data is structured in the database are explained in this paper. With the first data release, users get full access to halo/subhalo catalogs, various profiles of the halos at redshifts z=0-15, and raw dark matter data for one time-step of the Bolshoi and four time-steps of the MultiDark simulation. Later releases will also include galaxy mock catalogs and additional merging trees for both simulations as well as new large volume simulations with high resolution. This project is further proof of the viability to store and present complex data using relational database technology. We encourage other simulators to publish their results in a similar manner.

[1]  Volker Springel,et al.  Resolving cosmic structure formation with the Millennium-II simulation , 2009, 0903.3041.

[2]  Edinburgh,et al.  Simulating the joint evolution of quasars, galaxies and their large-scale distribution , 2005, astro-ph/0504097.

[3]  Yipeng Jing,et al.  The growth and structure of dark matter haloes , 2003 .

[4]  Stefan Gottloeber,et al.  The ART of Cosmological Simulations , 2008, 0803.4343.

[5]  J. C. Muñoz-Cuartas,et al.  The Redshift Evolution of LCDM Halo Parameters: Concentration, Spin, and Shape , 2010, 1007.0438.

[6]  V. Springel The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.

[7]  Potsdam,et al.  The Dark Side of the Halo Occupation Distribution , 2003, astro-ph/0308519.

[8]  R. Wechsler,et al.  Modeling Luminosity-dependent Galaxy Clustering through Cosmic Time , 2005, astro-ph/0512234.

[9]  S. More,et al.  Towards a concordant model of halo occupation statistics , 2006, astro-ph/0610686.

[10]  Joel R. Primack,et al.  Dynamical effects of the cosmological constant. , 1991 .

[11]  John Dubinski,et al.  The structure of cold dark matter halos , 1991 .

[12]  Frank C. van den Bosch,et al.  Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP1, WMAP3 and WMAP5 results , 2008, 0805.1926.

[13]  Martin White,et al.  What determines satellite galaxy disruption , 2009, 0907.0702.

[14]  M. Halpern,et al.  SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP ) OBSERVATIONS: ARE THERE COSMIC MICROWAVE BACKGROUND ANOMALIES? , 2010, 1001.4758.

[15]  G. Efstathiou,et al.  The evolution of large-scale structure in a universe dominated by cold dark matter , 1985 .

[16]  J. Ostriker,et al.  Linking halo mass to galaxy luminosity , 2004, astro-ph/0402500.

[17]  Durham,et al.  The Aquarius Project: the subhaloes of galactic haloes , 2008, 0809.0898.

[18]  J. Peacock,et al.  Simulations of the formation, evolution and clustering of galaxies and quasars , 2005, Nature.

[19]  Simon Prunet,et al.  Full-sky weak-lensing simulation with 70 billion particles , 2008, 0807.3651.

[20]  Michael S. Warren,et al.  Precision Determination of the Mass Function of Dark Matter Halos , 2005, astro-ph/0506395.

[21]  A. Klypin,et al.  Adaptive Refinement Tree: A New High-Resolution N-Body Code for Cosmological Simulations , 1997, astro-ph/9701195.

[22]  G. Kauffmann,et al.  The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colour , 2005, astro-ph/0508046.

[23]  U. Chicago,et al.  The Astrophysical Journal, in press Preprint typeset using L ATEX style emulateapj v. 6/22/04 THE DEPENDENCE OF HALO CLUSTERING ON HALO FORMATION HISTORY, CONCENTRATION, AND OCCUPATION , 2005 .

[24]  U. California,et al.  Semi-analytic modelling of galaxy formation: The local Universe , 1998, astro-ph/9802268.

[25]  Joel Primack,et al.  GALAXIES IN ΛCDM WITH HALO ABUNDANCE MATCHING: LUMINOSITY–VELOCITY RELATION, BARYONIC MASS–VELOCITY RELATION, VELOCITY FUNCTION, AND CLUSTERING , 2010, 1005.1289.

[26]  Anatoly Klypin,et al.  The Origin and Evolution of Halo Bias in Linear and Nonlinear Regimes , 1999 .

[27]  S. J. Aarseth,et al.  Dynamical Evolution of Clusters Of Galaxies, II , 1963 .

[28]  Guinevere Kauffmann,et al.  Clustering of galaxies in a hierarchical universe - I. Methods and results at z=0 , 1999 .

[29]  S. J. Aarseth Dynamical Evolution of Clusters of Galaxies—III , 1969 .

[30]  G. Bryan,et al.  Statistical Properties of X-Ray Clusters: Analytic and Numerical Comparisons , 1997, astro-ph/9710107.

[31]  A. Knebe,et al.  Ahf: AMIGA'S HALO FINDER , 2009, 0904.3662.

[32]  Joel R. Primack,et al.  LCDM Correctly Predicts Basic Statistics of Galaxies: Luminosity-Velocity Relation, Baryonic Mass-Velocity Relation, and Velocity Function , 2010 .

[33]  Alexander S. Szalay,et al.  Implementing a General Spatial Indexing Library for Relational Databases of Large Numerical Simulations , 2011, SSDBM.

[34]  Joel R. Primack,et al.  Halo concentrations in the standard LCDM cosmology , 2011, 1104.5130.

[35]  G. Lemson,et al.  Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony , 2006, astro-ph/0608019.

[36]  Oxford,et al.  Breaking the hierarchy of galaxy formation , 2005, astro-ph/0511338.

[37]  John Dubinski,et al.  THE HORIZON RUN N-BODY SIMULATION: BARYON ACOUSTIC OSCILLATIONS AND TOPOLOGY OF LARGE-SCALE STRUCTURE OF THE UNIVERSE , 2008, 0812.1392.

[38]  G. Lucia,et al.  The hierarchical formation of the brightest cluster galaxies , 2006, astro-ph/0606519.

[39]  Arndt Bode,et al.  High Performance Computing in Science and Engineering, Garching/Munich 2007: Transactions of the Third Joint HLRB and KONWIHR Status and Result Workshop, ... Centre, Garching/Munich, Germany , 2008 .

[40]  F. Prada,et al.  How Far Do They Go? The Outer Structure of Galactic Dark Matter Halos , 2005, astro-ph/0506432.

[41]  R. Somerville,et al.  Profiles of dark haloes: evolution, scatter and environment , 1999, astro-ph/9908159.

[42]  Joel R. Primack,et al.  Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations , 2011, 1104.0669.

[43]  Joachim Stadel,et al.  Quantifying the heart of darkness with GHALO – a multibillion particle simulation of a galactic halo , 2008, 0808.2981.

[44]  Anatoly Klypin,et al.  Particle mesh code for cosmological simulations , 1997, astro-ph/9712217.

[45]  Gerard Lemson,et al.  Cosmological simulations in a relational database: modelling and storing merger trees , 2006 .

[46]  Michael S. Warren,et al.  THE LARGE-SCALE BIAS OF DARK MATTER HALOS: NUMERICAL CALIBRATION AND MODEL TESTS , 2010, 1001.3162.

[47]  S. J. Aarseth,et al.  N-body simulations of galaxy clustering. III. The covariance function , 1979 .

[48]  Michael Kuhlen,et al.  The Dark Matter Annihilation Signal from Galactic Substructure: Predictions for GLAST , 2008, 0805.4416.

[49]  Shaun Cole,et al.  The shapes and alignments of dark matter halos , 2011, 1111.5616.

[50]  H. Schnopper,et al.  X-Ray and Radio Observations of the Structure of Abell 478. , 1977 .

[51]  S. White,et al.  The age dependence of halo clustering , 2005, astro-ph/0506510.

[52]  G. Kauffmann,et al.  Clustering of galaxies in a hierarchical universe — III. Mock redshift surveys , 1998, astro-ph/9812009.

[53]  Simon D. M. White,et al.  The Dynamics of Rich Clusters of Galaxies , 1976 .

[54]  Shaun Cole,et al.  The statistics of ΛCDM halo concentrations , 2007 .

[55]  Astronomy,et al.  The statistics of lambda CDM Halo Concentrations , 2007, 0706.2919.

[56]  A. Klypin,et al.  DARK MATTER HALOS IN THE STANDARD COSMOLOGICAL MODEL: RESULTS FROM THE BOLSHOI SIMULATION , 2010, 1002.3660.

[57]  Volker Springel,et al.  The Many lives of AGN: Cooling flows, black holes and the luminosities and colours of galaxies , 2006, astro-ph/0602065.

[58]  H. M. P. Couchman,et al.  The mass function of dark matter haloes , 2000, astro-ph/0005260.

[59]  Risa H. Wechsler,et al.  The Physics of Galaxy Clustering. I. A Model for Subhalo Populations , 2005 .

[60]  R. Sheth,et al.  An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier , 2001, astro-ph/0105113.

[61]  Francisco Prada,et al.  Where Are the Missing Galactic Satellites? , 1999, astro-ph/9901240.

[62]  S. White,et al.  A Universal Density Profile from Hierarchical Clustering , 1996, astro-ph/9611107.

[63]  Ue-Li Pen,et al.  Can 21-cm observations discriminate between high-mass and low-mass galaxies as reionization sources? , 2011, 1107.4772.

[64]  Michael S. Warren,et al.  Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality , 2008, 0803.2706.

[65]  Bernard J. T. Jones,et al.  The rotation of galaxies: numerical investigations of the tidal torque theory , 1979 .

[66]  Risa H. Wechsler,et al.  The shape of dark matter haloes : dependence on mass, redshift, radius and formation , 2005, astro-ph/0508497.

[67]  Y. Jing,et al.  Accurate Fitting Formula for the Two-Point Correlation Function of Dark Matter Halos , 1998, astro-ph/9805202.

[68]  S. More,et al.  THE OVERDENSITY AND MASSES OF THE FRIENDS-OF-FRIENDS HALOS AND UNIVERSALITY OF HALO MASS FUNCTION , 2011, 1103.0005.

[69]  Phillip James Edwin Peebles,et al.  STRUCTURE OF THE COMA CLUSTER OF GALAXIES. , 1970 .

[70]  George Lake,et al.  Dark Matter Substructure within Galactic Halos , 1999, astro-ph/9907411.