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Joint analysis of galaxy-galaxy lensing and galaxy clustering: Methodology and forecasts for Dark Energy Survey

机译:银河银行透镜和银河集群的联合分析:黑暗能源调查的方法论和预测

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摘要

The joint analysis of galaxy-galaxy lensing and galaxy clustering is a promising method for inferring the growth function of large-scale structure. Anticipating a near future application of this analysis to Dark Energy Survey (DES) measurements of galaxy positions and shapes, we develop a practical approach to modeling the assumptions and systematic effects affecting the joint analysis of small-scale galaxy-galaxy lensing and large-scale galaxy clustering. Introducing parameters that characterize the halo occupation distribution (HOD), photometric redshift uncertainties, and shear measurement errors, we study how external priors on different subsets of these parameters affect our growth constraints. Degeneracies within the HOD model, as well as between the HOD and the growth function, are identified as the dominant source of complication, with other systematic effects being subdominant. The impact of HOD parameters and their degeneracies necessitate the detailed joint modeling of the galaxy sample that we employ. We conclude that DES data will provide powerful constraints on the evolution of structure growth in the Universe, conservatively/optimistically constraining the growth function to 7.9%/4.8% with its first-year data that cover over 1000 square degrees, and to 3.9%/2.3% with its full five-year data that will survey 5000 square degrees, including both statistical and systematic uncertainties.
机译:Galaxy-Galaxy透镜和Galaxy Clustering的联合分析是推断大规模结构的生长功能的有希望的方法。预测该分析的近期应用对黑暗能量调查(DES)的Galaxy位置和形状的测量,我们开发了建模影响影响小型Galaxy-Galaxy镜头和大规模的共同分析的假设和系统效果的实用方法Galaxy Clustering。引入表征光晕职业分布(HOD),光度红移不确定度和剪切测量误差的参数,我们研究这些参数的不同子集上的外部前置如何影响我们的生长约束。 HOD模型中的退化性,以及HOD和生长功能,被鉴定为显着的并发症源,其它系统效应是亚纳米。 HOD参数及其退化的影响需要我们采用的星系样本的详细联合建模。我们得出结论,DES数据将对宇宙结构增长的演变提供强大的限制,保守/乐观地将增长函数与其第一年数据覆盖超过1000平方度的7.9%/ 4.8%,以及3.9%/ 2.3%,其完整的五年数据将调查5000平方度,包括统计和系统的不确定性。

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  • 来源
    《Physical review, D》 |2016年第1期|共22页
  • 作者单位

    Univ Chicago Kavli Inst Cosmol Phys Chicago IL 60637 USA;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol POB 2450 Stanford CA 94305 USA;

    Univ Chicago Kavli Inst Cosmol Phys Chicago IL 60637 USA;

    Univ Penn Dept Phys &

    Astron Philadelphia PA 19104 USA;

    Swiss Fed Inst Technol Dept Phys Wolfgang Pauli Str 16 CH-8093 Zurich Switzerland;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol POB 2450 Stanford CA 94305 USA;

    Univ Manchester Jodrell Bank Ctr Astrophys Sch Phys &

    Astron Oxford Rd Manchester M13 9PL Lancs England;

    Univ Penn Dept Phys &

    Astron Philadelphia PA 19104 USA;

    IEEC CSIC Inst Ciencies Espai Campus UAB Carrer Can Magrans S-N Barcelona 08193 Spain;

    IEEC CSIC Inst Ciencies Espai Campus UAB Carrer Can Magrans S-N Barcelona 08193 Spain;

    IEEC CSIC Inst Ciencies Espai Campus UAB Carrer Can Magrans S-N Barcelona 08193 Spain;

    Ohio State Univ Ctr Cosmol &

    Astroparticle Phys Columbus OH 43210 USA;

    Univ Arizona Dept Phys Tucson AZ 85721 USA;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Univ Autonoma Barcelona Inst Fis Altes Energies E-08193 Barcelona Spain;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol POB 2450 Stanford CA 94305 USA;

    Natl Opt Astron Observ Cerro Tololo Interamer Observ Casilla 603 La Serena Chile;

    UCL Dept Phys &

    Astron Gower St London WC1E 6BT England;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    UCL Dept Phys &

    Astron Gower St London WC1E 6BT England;

    Inst Astrophys Paris CNRS UMR 7095 F-75014 Paris France;

    UCL Dept Phys &

    Astron Gower St London WC1E 6BT England;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol POB 2450 Stanford CA 94305 USA;

    Lab Interinst E Astron LIneA Rua Gal Jose Cristino 77 BR-20921400 Rio De Janeiro RJ Brazil;

    Univ Illinois Dept Astron 1002 West Green St Urbana IL 61801 USA;

    IEEC CSIC Inst Ciencies Espai Campus UAB Carrer Can Magrans S-N Barcelona 08193 Spain;

    IEEC CSIC Inst Ciencies Espai Campus UAB Carrer Can Magrans S-N Barcelona 08193 Spain;

    Lab Interinst E Astron LIneA Rua Gal Jose Cristino 77 BR-20921400 Rio De Janeiro RJ Brazil;

    Texas A&

    M Univ George P &

    Cynthia Woods Mitchell Inst Fundamenta College Stn TX 77843 USA;

    Univ Munich Dept Phys Scheinerstr 1 D-81679 Munich Germany;

    Excellence Cluster Universe Boltzmannstr 2 D-85748 Garching Germany;

    UCL Dept Phys &

    Astron Gower St London WC1E 6BT England;

    Univ Penn Dept Phys &

    Astron Philadelphia PA 19104 USA;

    Lab Interinst E Astron LIneA Rua Gal Jose Cristino 77 BR-20921400 Rio De Janeiro RJ Brazil;

    Univ Autonoma Barcelona Inst Fis Altes Energies E-08193 Barcelona Spain;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Munich Univ Sternwarte Fak Phys Scheinerstr 1 D-81679 Munich Germany;

    Univ Illinois Dept Astron 1002 West Green St Urbana IL 61801 USA;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Natl Opt Astron Observ Cerro Tololo Interamer Observ Casilla 603 La Serena Chile;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Australian Astron Observ N Ryde NSW 2113 Australia;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Lab Interinst E Astron LIneA Rua Gal Jose Cristino 77 BR-20921400 Rio De Janeiro RJ Brazil;

    Lab Interinst E Astron LIneA Rua Gal Jose Cristino 77 BR-20921400 Rio De Janeiro RJ Brazil;

    Texas A&

    M Univ George P &

    Cynthia Woods Mitchell Inst Fundamenta College Stn TX 77843 USA;

    Ohio State Univ Ctr Cosmol &

    Astroparticle Phys Columbus OH 43210 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Autonoma Barcelona Inst Fis Altes Energies E-08193 Barcelona Spain;

    Univ Portsmouth Inst Cosmol &

    Gravitat Portsmouth PO1 3FX Hants England;

    Lab Interinst E Astron LIneA Rua Gal Jose Cristino 77 BR-20921400 Rio De Janeiro RJ Brazil;

    CALTECH Jet Prop Lab 4800 Oak Grove Dr Pasadena CA 91109 USA;

    Lawrence Berkeley Natl Lab 1 Cyclotron Rd Berkeley CA 94720 USA;

    Univ Sussex Dept Phys &

    Astron Pevensey Bldg Brighton BN1 9QH E Sussex England;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol POB 2450 Stanford CA 94305 USA;

    Ctr Invest Energet Medioambientales &

    Tecnol CIEM Madrid Spain;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Illinois Dept Astron 1002 West Green St Urbana IL 61801 USA;

    Fermilab Natl Accelerator Lab POB 500 Batavia IL 60510 USA;

    Ohio State Univ Ctr Cosmol &

    Astroparticle Phys Columbus OH 43210 USA;

    Natl Ctr Supercomp Applicat 1205 West Clark St Urbana IL 61801 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Illinois Dept Phys 1110 West Green St Urbana IL 61801 USA;

    Argonne Natl Lab 9700 South Cass Ave Lemont IL 60439 USA;

    Natl Opt Astron Observ Cerro Tololo Interamer Observ Casilla 603 La Serena Chile;

    Excellence Cluster Universe Boltzmannstr 2 D-85748 Garching Germany;

    Univ Manchester Jodrell Bank Ctr Astrophys Sch Phys &

    Astron Oxford Rd Manchester M13 9PL Lancs England;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 粒子物理学;场论;
  • 关键词

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