Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
arXiv:0810.2300 · doi:10.1111/j.1365-2966.2009.14402.x
Abstract
We describe a method for constructing mock galaxy catalogues which are well suited for use in conjunction with large photometric surveys. We use the semi-analytic galaxy formation model of Bower et al. implemented in the Millennium simulation. We apply our method to the specific case of the surveys soon to commence with PS1, the first of 4 telescopes planned for the Pan-STARRS system. PS1 has 5 photometric bands (grizy), and will carry out an all-sky 3pi survey and a medium deep survey (MDS) over 84 sq.deg. We calculate the expected magnitude limits for extended sources in the two surveys. We find that, after 3 years, the 3pi survey will have detected over 10^8 galaxies in all 5 bands, 10 million of which will lie at redshift z>0.9, while the MDS will have detected over 10^7 galaxies with 0.5 million lying at z>2. These numbers at least double if detection in the shallowest band, y is not required. We then evaluate the accuracy of photometric redshifts estimated using an off-the-shelf photo-z code. With the grizy bands alone it is possible to achieve an accuracy in the 3pi survey of Delta z/(1+z)~0.06 for 0.25<z<0.8, which could be reduced by about 15% using near infrared photometry from the UKIDDS survey, but would increase by about 25% for the deeper sample without the y band photometry. For the MDS an accuracy of Delta z/(1+z)~0.05 is achievable for 0.02<z<1.5 using grizy. A dramatic improvement in accuracy is possible by selecting only red galaxies. In this case, Delta z/(1+z)~0.02-0.04 is achievable for ~100 million galaxies at 0.4<z<1.1 in the 3pi survey and for 30 million galaxies in the MDS at 0.4<z<2. We investigate the effect of using photo-z in the estimate of the baryonic acoustic oscillation scale. We find that PS1 will achieve a similar accuracy in this estimate as a spectroscopic survey of 20 million galaxies.
23 pages, 18 figures, accepted by MNRAS
References in corpus (66)
- Stellar population synthesis at the resolution of 2003
- The Sloan Digital Sky Survey: Technical Summary
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Cosmological parameters from SDSS and WMAP
- The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The broken hierarchy of galaxy formation
- The 2dF Galaxy Redshift Survey: Spectra and redshifts
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Hierarchical Galaxy Formation
- Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
- The size distribution of galaxies in the Sloan Digital Sky Survey
- Bayesian photometric redshift estimation
- The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
- The formation history of elliptical galaxies
- The 2dF Galaxy Redshift Survey: Near Infrared Galaxy Luminosity Functions
- The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
- Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
- Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
- The UKIRT Infrared Deep Sky Survey ZYJHK Photometric System: Passbands and Synthetic Colours
- Reconstructing the linear power spectrum of cosmological mass fluctuations
- A primer on hierarchical galaxy formation: the semi-analytical approach
- Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler
- The size evolution of galaxies since z~3: combining SDSS, GEMS and FIRES
- ANNz: estimating photometric redshifts using artificial neural networks
- The 2dF Galaxy Redshift Survey: The b_J-band galaxy luminosity function and survey selection function
- Evolution of the Hubble Sequence in Hierarchical Models for Galaxy Formation
- Slicing Through Multicolor Space: Galaxy Redshifts From Broadband Photometry
- GALICS I: A hybrid N-body semi-analytic model of hierarchical galaxy formation
- The infrared side of galaxy formation. I. The local universe in the semi-analytical framework
- Evidence for a non-zero Lambda and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and Cosmic Microwave Background Anisotropies
- Galaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data
- Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field
- Large Synoptic Survey Telescope: Overview
- Photometric Redshifts for the SDSS Early Data Release
- Semi-analytical model of galaxy formation with high-resolution N-body simulations
- Estimating photometric redshifts with artificial neural networks
- Cosmological parameters from CMB measurements and the final 2dFGRS power spectrum
- The detectability of baryonic acoustic oscillations in future galaxy surveys
- The K20 survey. V The evolution of the near-IR Luminosity Function
- Evolution and Color-Dependence of the Galaxy Angular Correlation Function: 350,000 Galaxies in 5 Square Degrees
- MoMaF : The Mock Map Facility
- The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands
- Photometric Redshifts of Galaxies in COSMOS
- Black Hole Growth in Hierarchical Galaxy Formation
- Baryon Oscillations as a Cosmological Probe
- Cosmology with photometric redshift surveys
- Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
- The Effects of Photoionization on Galaxy Formation -- III: Environmental Dependence in the Luminosity Function
- Gas cooling in simulations of the formation of the galaxy population
- The Hawaii-AAO K-band Galaxy Redshift Survey -- Paper I: The Local K-band Luminosity Function
- Photo-z for weak lensing tomography from space: the role of optical and near-IR photometry
- Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
- A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
- The Photometric Redshift Distribution and Evolutionary Properties of Galaxies up to z= 4.5 in the Field of the Quasar BR1202-0725
- Massive and Red Objects predicted by a semianalytical model of galaxy formation
- The Munich Near-Infrared Cluster Survey (MUNICS) -- II. The K-Band Luminosity Function of Field Galaxies to z ~ 1.2
- The structural and photometric properties of early-type galaxies in hierarchical models
- Baryon Oscillations and Dark-Energy Constraints from Imaging Surveys
- Models of Disk Evolution: Confrontation with Observations
- Spatial Variations of Galaxy Number Counts in the Sloan Digital Sky Survey. II. Test of Galactic Extinction in High Extinction Regions
- GalICS V : Low and high order clustering in mock SDSS's
- Evolution in the Clustering of Galaxies for Z < 1
- Spatial Variations of Galaxy Number Counts in the SDSS I.: Extinction, Large-Scale Structure and Photometric Homogeneity
Cited by in corpus (16)
- Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection
- The JWST Extragalactic Mock Catalog: Modeling galaxy populations from the UV through the near-IR over thirteen billion years of cosmic history
- What Shapes the Galaxy Mass Function? Exploring the Roles of Supernova-Driven Winds and AGN
- Redshift distributions of galaxies in the DES Science Verification shear catalogue and implications for weak lensing
- Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
- Modeling the angular correlation function and its full covariance in Photometric Galaxy Surveys
- Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
- ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
- Photo-z Performance for Precision Cosmology
- ORCA: The Overdense Red-sequence Cluster Algorithm
- The effect of photometric redshift uncertainties on galaxy clustering and baryonic acoustic oscillations
- Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
- Influence of Projection in Cluster Cosmology Studies
- Constructing mock catalogues for the REFLEX II galaxy cluster sample
- A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
- Characterising the optical properties of galaxy clusters with GMPhoRCC