On the relative bias of void tracers in the Dark Energy Survey

Pollina, G.; Hamaus, N.; Paech, K.; Dolag, K.; Weller, J.; Sánchez, C.; Rykoff, E. S.; Jain, B.; Abbott, T. M. C.; Allam, S.; Avila, S.; Bernstein, R. A.; Bertin, E.; Brooks, D.; Burke, D. L.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Cunha, C. E.; D’Andrea, C. B.; da Costa, L. N.; De Vicente, J.; DePoy, D. L.; Desai, S.; Diehl, H. T.; Doel, P.; Evrard, A. E.; Flaugher, B.; Fosalba, P.; Frieman, J.; García-Bellido, J.; Gerdes, D. W.; Giannantonio, T.; Gruen, D.; Gschwend, J.; Gutierrez, G.; Hartley, W. G.; Hollowood, D. L.; Honscheid, K.; Hoyle, B.; James, D. J.; Jeltema, T.; Kuehn, K.; Kuropatkin, N.; Lima, M.; March, M.; Marshall, J. L.; Melchior, P.; Menanteau, F.; Miquel, R.; Plazas, A. A.; Romer, A. K.; Sanchez, E.; Scarpine, V.; Schindler, R.; Schubnell, M.; Sevilla-Noarbe, I.; Smith, M.; Soares-Santos, M.; Sobreira, F.; Suchyta, E.; Tarle, G.; Walker, A. R.; Wester, W.

doi:10.1093/mnras/stz1470

Title: On the relative bias of void tracers in the Dark Energy Survey

Abstract

Luminous tracers of large-scale structure are not entirely representative of the distribution of mass in our Universe. As they arise from the highest peaks in the matter density field, the spatial distribution of luminous objects is biased towards those peaks. On large scales, where density fluctuations are mild, this bias simply amounts to a constant offset in the clustering amplitude of the tracer, known as linear bias. In this work we focus on the relative bias between galaxies and galaxy clusters that are located inside and in the vicinity of cosmic voids, extended regions of relatively low density in the large-scale structure of the Universe. With the help of mock data we verify that the relation between galaxy and cluster overdensity around voids remains linear. Hence, the void-centric density profiles of different tracers can be linked by a single multiplicative constant. This amounts to the same value as the relative linear bias between tracers for the largest voids in the sample. For voids of small sizes, which typically arise in higher density regions, this constant has a higher value, possibly showing an environmental dependence similar to that observed for the linear bias itself. We confirm our findings by analysing datamore »« less

Authors:

Pollina, G. ^[1]; Hamaus, N. ^[2];

^[1]; Dolag, K. ^[3]; Weller, J. ^[4]; Sánchez, C. ^[5]; Rykoff, E. S. ^[6]; Jain, B. ^[7]; Abbott, T. M. C. ^[8]; Allam, S. ^[9];

^[10]; Bernstein, R. A. ^[11]; Bertin, E. ^[12]; Brooks, D. ^[13]; Burke, D. L. ^[6];

^[14]; Carrasco Kind, M. ^[15]; Carretero, J. ^[16]; Cunha, C. E. ^[17]; D’Andrea, C. B. ^[7] more »

Excellence Cluster Universe, Boltzmannstrasse 2, D-85748 Garching, Germany, Fakultät für Physik, Universitäts-Sternwarte, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany
Fakultät für Physik, Universitäts-Sternwarte, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany
Fakultät für Physik, Universitäts-Sternwarte, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany, Max-Planck-Institute for Astrophysics, Karl-Schwarzschild Strasse 1, D-85748 Garching, Germany
Excellence Cluster Universe, Boltzmannstrasse 2, D-85748 Garching, Germany, Fakultät für Physik, Universitäts-Sternwarte, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, D-85748 Garching, Germany
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
Kavli Institute for Particle Astrophysics & Cosmology, Stanford University, PO Box 2450, Stanford, CA 94305, USA, SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA
Institute of Cosmology & Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
Observatories of the Carnegie Institution of Washington, 813 Santa Barbara St, Pasadena, CA 91101, USA
CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, France, Institut d’Astrophysique de Paris, Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, F-75014 Paris, France
Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil, Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA, National Center for Supercomputing Applications, 1205 West Clark St, Urbana, IL 61801, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
Kavli Institute for Particle Astrophysics & Cosmology, Stanford University, PO Box 2450, Stanford, CA 94305, USA
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA, Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
Institut d’Estudis Espacials de Catalunya (IEEC), E-08193 Barcelona, Spain, Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA, Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
Fakultät für Physik, Universitäts-Sternwarte, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany, Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA, Department of Physics, The Ohio State University, Columbus, OH 43210, USA
Fakultät für Physik, Universitäts-Sternwarte, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, D-85748 Garching, Germany
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Australian Astronomical Observatory, North Ryde, NSW 2113, Australia
Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil, Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, Brazil
Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain, Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA
Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, UK
SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA
Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil, Instituto de Física Gleb Wataghin, Universidade Estadual de Campinas, 13083-859 Campinas, SP, Brazil
Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
(

Publication Date:: Fri May 31 00:00:00 EDT 2019

Research Org.:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Org.:: USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)

Contributing Org.:: DES Collaboration

OSTI Identifier:: 1526094

Alternate Identifier(s):: OSTI ID: 1471731; OSTI ID: 1531212; OSTI ID: 1709101

Report Number(s):: arXiv:1806.06860; FERMILAB-PUB-18-220
Journal ID: ISSN 0035-8711

Grant/Contract Number:: AC02-07CH11359; AC05-00OR22725; SC0019193

Resource Type:: Published Article

Journal Name:: Monthly Notices of the Royal Astronomical Society

Additional Journal Information:: Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 487 Journal Issue: 2; Journal ID: ISSN 0035-8711

Publisher:: Royal Astronomical Society

Country of Publication:: United Kingdom

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: general; large-scale structure of Universe; cosmology: observations

Citation Formats


                    Pollina, G., Hamaus, N., Paech, K., Dolag, K., Weller, J., Sánchez, C., Rykoff, E. S., Jain, B., Abbott, T. M. C., Allam, S., Avila, S., Bernstein, R. A., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., De Vicente, J., DePoy, D. L., Desai, S., Diehl, H. T., Doel, P., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruen, D., Gschwend, J., Gutierrez, G., Hartley, W. G., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Sobreira, F., Suchyta, E., Tarle, G., Walker, A. R., Wester, W., and DES Collaboration). On the relative bias of void tracers in the Dark Energy Survey.  United Kingdom: N. p., 2019. 
Web.  doi:10.1093/mnras/stz1470.

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                    Pollina, G., Hamaus, N., Paech, K., Dolag, K., Weller, J., Sánchez, C., Rykoff, E. S., Jain, B., Abbott, T. M. C., Allam, S., Avila, S., Bernstein, R. A., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., De Vicente, J., DePoy, D. L., Desai, S., Diehl, H. T., Doel, P., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruen, D., Gschwend, J., Gutierrez, G., Hartley, W. G., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Sobreira, F., Suchyta, E., Tarle, G., Walker, A. R., Wester, W., & DES Collaboration). On the relative bias of void tracers in the Dark Energy Survey.  United Kingdom.  https://doi.org/10.1093/mnras/stz1470

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                    Pollina, G., Hamaus, N., Paech, K., Dolag, K., Weller, J., Sánchez, C., Rykoff, E. S., Jain, B., Abbott, T. M. C., Allam, S., Avila, S., Bernstein, R. A., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., De Vicente, J., DePoy, D. L., Desai, S., Diehl, H. T., Doel, P., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruen, D., Gschwend, J., Gutierrez, G., Hartley, W. G., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Sobreira, F., Suchyta, E., Tarle, G., Walker, A. R., Wester, W., and DES Collaboration). Fri .  
"On the relative bias of void tracers in the Dark Energy Survey".  United Kingdom.  https://doi.org/10.1093/mnras/stz1470.

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@article{osti_1526094,

  title        = {On the relative bias of void tracers in the Dark Energy Survey},

  author       = {Pollina, G. and Hamaus, N. and Paech, K. and Dolag, K. and Weller, J. and Sánchez, C. and Rykoff, E. S. and Jain, B. and Abbott, T. M. C. and Allam, S. and Avila, S. and Bernstein, R. A. and Bertin, E. and Brooks, D. and Burke, D. L. and Carnero Rosell, A. and Carrasco Kind, M. and Carretero, J. and Cunha, C. E. and D’Andrea, C. B. and da Costa, L. N. and De Vicente, J. and DePoy, D. L. and Desai, S. and Diehl, H. T. and Doel, P. and Evrard, A. E. and Flaugher, B. and Fosalba, P. and Frieman, J. and García-Bellido, J. and Gerdes, D. W. and Giannantonio, T. and Gruen, D. and Gschwend, J. and Gutierrez, G. and Hartley, W. G. and Hollowood, D. L. and Honscheid, K. and Hoyle, B. and James, D. J. and Jeltema, T. and Kuehn, K. and Kuropatkin, N. and Lima, M. and March, M. and Marshall, J. L. and Melchior, P. and Menanteau, F. and Miquel, R. and Plazas, A. A. and Romer, A. K. and Sanchez, E. and Scarpine, V. and Schindler, R. and Schubnell, M. and Sevilla-Noarbe, I. and Smith, M. and Soares-Santos, M. and Sobreira, F. and Suchyta, E. and Tarle, G. and Walker, A. R. and Wester, W. and DES Collaboration)},

  abstractNote = {Luminous tracers of large-scale structure are not entirely representative of the distribution of mass in our Universe. As they arise from the highest peaks in the matter density field, the spatial distribution of luminous objects is biased towards those peaks. On large scales, where density fluctuations are mild, this bias simply amounts to a constant offset in the clustering amplitude of the tracer, known as linear bias. In this work we focus on the relative bias between galaxies and galaxy clusters that are located inside and in the vicinity of cosmic voids, extended regions of relatively low density in the large-scale structure of the Universe. With the help of mock data we verify that the relation between galaxy and cluster overdensity around voids remains linear. Hence, the void-centric density profiles of different tracers can be linked by a single multiplicative constant. This amounts to the same value as the relative linear bias between tracers for the largest voids in the sample. For voids of small sizes, which typically arise in higher density regions, this constant has a higher value, possibly showing an environmental dependence similar to that observed for the linear bias itself. We confirm our findings by analysing data obtained during the first year of observations by the Dark Energy Survey. As a side product, we present the first catalogue of three-dimensional voids extracted from a photometric survey with a controlled photo-z uncertainty. Finally, our results will be relevant in forthcoming analyses that attempt to use voids as cosmological probes.},

  doi          = {10.1093/mnras/stz1470},

  journal      = {Monthly Notices of the Royal Astronomical Society},

  number       = 2,

  volume       = 487,

  place        = {United Kingdom},

  year         = {Fri May 31 00:00:00 EDT 2019},

  month        = {Fri May 31 00:00:00 EDT 2019}

}

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Title: On the relative bias of void tracers in the Dark Energy Survey

Abstract

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Revealing the Cosmic Web-dependent Halo Bias
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The evolution of voids in the expanding universe
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Lensing measurements of the mass distribution in SDSS voids
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A halo bias function measured deeply into voids without stochasticity
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Voids in coupled scalar field cosmology: Voids in coupled scalar field cosmology
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Spatial and dynamical properties of voids in a Λ cold dark matter universe
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First results from the IllustrisTNG simulations: matter and galaxy clustering
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Weak lensing by galaxy troughs in DES Science Verification data
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Multipole analysis of redshift-space distortions around cosmic voids
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Cosmic voids in coupled dark energy cosmologies: the impact of halo bias
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Clues on void evolution – I. Large-scale galaxy distributions around voids
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Constraints on Cosmology and Gravity from the Dynamics of Voids
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redMaGiC: selecting luminous red galaxies from the DES Science Verification data
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The Redshift Evolution of the mean Temperature, Pressure, and Entropy Profiles in 80 Spt-Selected Galaxy Clusters
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Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
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Cosmological exploitation of cosmic void statistics: New numerical tools in the CosmoBolognaLib to extract cosmological constraints from the void size function⋆
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Cosmology with Void-Galaxy Correlations
journal, January 2014

The structure of cosmic voids in a ΛCDM Universe
journal, July 2013

zobov: a parameter-free void-finding algorithm
journal, June 2008

A cosmic watershed: the WVF void detection technique
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An Imprint of Superstructures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
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Cosmological simulations of black hole growth: AGN luminosities and downsizing
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Fast Cosmic Microwave Background Analyses via Correlation Functions
journal, February 2001

The dark Energy Camera
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A measurement of the Alcock–Paczyński effect using cosmic voids in the SDSS
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The cosmological simulation code gadget-2
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A Public void Catalog from the sdss dr7 Galaxy Redshift Surveys Based on the Watershed Transform
journal, November 2012

Dark Energy Survey Year 1 Results: The Photometric Data Set for Cosmology
journal, April 2018

Sparse sampling, galaxy bias, and voids
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A Detection of the Integrated Sachs–Wolfe Imprint of Cosmic Superstructures Using a Matched-Filter Approach
journal, October 2016

The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes
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Origin and properties of dual and offset active galactic nuclei in a cosmological simulation at $\boldsymbol {z=2}$
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Dependence of halo bias on mass and environment
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Constraints on the distribution and energetics of fast radio bursts using cosmological hydrodynamic simulations
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The Dark Energy Survey: Data Release 1
journal, November 2018

The Santiago–Harvard–Edinburgh–Durham void comparison – I. SHEDding light on chameleon gravity tests
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VIDE: The Void IDentification and Examination toolkit
journal, March 2015

Cosmic voids in Sloan Digital Sky Survey Data Release 7
journal, February 2012

A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
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Clustering and bias measurements of SDSS voids
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Using cosmic voids to distinguish f ( R ) gravity in future galaxy surveys
journal, June 2015

Halo mass function: baryon impact, fitting formulae, and implications for cluster cosmology
journal, December 2015

The persistent percolation of single-stream voids
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Voids in modified gravity: excursion set predictions
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SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
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Redshift-space distortions around voids
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The Difference Imaging Pipeline for the Transient Search in the dark Energy Survey
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On the universality of void density profiles
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Strong clustering of underdense regions and the environmental dependence of clustering from Gaussian initial conditions
journal, June 2007

The nature of voids – I. Watershed void finders and their connection with theoretical models
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Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
journal, December 2001

An evolution free test for non-zero cosmological constant
journal, October 1979

The Redmapper Galaxy Cluster Catalog from des Science Verification data
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The abundance of voids and the excursion set formalism
journal, July 2013

Cosmic voids and void lensing in the Dark Energy Survey Science Verification data
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Unveiling galaxy bias via the halo model, KiDS, and GAMA
journal, June 2018