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Title: Lensing is low: cosmology, galaxy formation or new physics?

Abstract

Here, we introduce high signal-to-noise galaxy-galaxy lensing measurements of the Baryon Oscillation Spectroscopic Survey constant mass (CMASS) sample using 250 deg2 of weak-lensing data from Canada-France-Hawaii Telescope Lensing Survey and Canada-France-Hawaii Telescope Stripe 82 Survey. We compare this signal with predictions from mock catalogues trained to match observables including the stellar mass function and the projected and two-dimensional clustering of CMASS. We show that the clustering of CMASS, together with standard models of the galaxy-halo connection, robustly predicts a lensing signal that is 20-40 per cent larger than observed. Detailed tests show that our results are robust to a variety of systematic effects. Lowering the value of S8 = σ 8√{Ωm/0.3 compared to Planck Collaboration XIII reconciles the lensing with clustering. However, given the scale of our measurement (r < 10 h-1 Mpc), other effects may also be at play and need to be taken into consideration. We explore the impact of baryon physics, assembly bias, massive neutrinos and modifications to general relativity on ΔΣ and show that several of these effects may be non-negligible given the precision of our measurement. Disentangling cosmological effects from the details of the galaxy-halo connection, the effect of baryons, and massive neutrinos, is themore » next challenge facing joint lensing and clustering analyses. This is particularly true in the context of large galaxy samples from Baryon Acoustic Oscillation surveys with precise measurements but complex selection functions.« less

Authors:
 [1];  [2];  [3];  [2];  [4];  [5];  [6];  [5];  [1];  [7];  [8];  [9];  [8];  [10];  [11];  [12];  [13];  [14];  [2];  [15] more »;  [16];  [17] « less
+ Show Author Affiliations
  1. Univ. of California, Santa Cruz, CA (United States); Univ. of Tokyo (Japan)
  2. Max Planck Society, Garching (Germany). Max Planck Inst. for Astrophysics
  3. Exzellenzcluster Origins, Garching (Germany); Ludwig Maximilian Univ., Munich (Germany)
  4. Univ. of Tokyo (Japan)
  5. Univ. of California, Berkeley, CA (United States)
  6. Carnegie Mellon Univ., Pittsburgh, PA (United States); Univ. of Edinburgh, Scotland (United Kingdom)
  7. Univ. of Geneva (Switzerland). Astronomical Observatory
  8. Univ. of Bonn (Germany). Argelander Inst. for Astronomy (AIfA)
  9. Univ. of Edinburgh, Scotland (United Kingdom)
  10. Carnegie Mellon Univ., Pittsburgh, PA (United States)
  11. Univ. of Oxford (United Kingdom)
  12. Univ. College London, Bloomsbury (United Kingdom)
  13. Brazilian Center for Research in Physics, Rio de Janeiro (Brazil)
  14. Autonomous Univ. of Madrid (Spain); Consejo Superior de Investigaciones Cientificas (CSIC), Madrid (Spain)
  15. Ecole Polytechnique Federale Lausanne (Switzlerland). Lab. of Astrophysics (LASTRO)
  16. Istituto Nazionale di Astrofisica (INAF) (Italy). Astronomical Observatory of Trieste; National Inst. of Nuclear Physics (INFN), Trieste (Italy)
  17. Istituto Nazionale di Astrofisica (INAF) (Italy). Astronomical Observatory of Trieste; National Inst. of Nuclear Physics (INFN), Trieste (Italy); Center for Computational Astrophysics, New York, NY (United States)
Publication Date:
Research Org.:
University of California, Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Aeronautics and Space Administration (NASA); National Natural Science Foundation of China (NSFC); European Research Council (ERC)
OSTI Identifier:
1594740
Grant/Contract Number:  
SC0017860; NAS5-26555
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 467; Journal Issue: 3; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; gravitational lensing: weak; cosmology: observations; large-scale structure of Universe

Citation Formats

Leauthaud, Alexie, Saito, Shun, Hilbert, Stefan, Barreira, Alexandre, More, Surhud, White, Martin, Alam, Shadab, Behroozi, Peter, Bundy, Kevin, Coupon, Jean, Erben, Thomas, Heymans, Catherine, Hildebrandt, Hendrik, Mandelbaum, Rachel, Miller, Lance, Moraes, Bruno, Pereira, Maria E. S., Rodríguez-Torres, Sergio A., Schmidt, Fabian, Shan, Huan-Yuan, Viel, Matteo, and Villaescusa-Navarro, Francisco. Lensing is low: cosmology, galaxy formation or new physics?. United States: N. p., 2017. Web. doi:10.1093/mnras/stx258.
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Leauthaud, Alexie, Saito, Shun, Hilbert, Stefan, Barreira, Alexandre, More, Surhud, White, Martin, Alam, Shadab, Behroozi, Peter, Bundy, Kevin, Coupon, Jean, Erben, Thomas, Heymans, Catherine, Hildebrandt, Hendrik, Mandelbaum, Rachel, Miller, Lance, Moraes, Bruno, Pereira, Maria E. S., Rodríguez-Torres, Sergio A., Schmidt, Fabian, Shan, Huan-Yuan, Viel, Matteo, & Villaescusa-Navarro, Francisco. Lensing is low: cosmology, galaxy formation or new physics?. United States. https://doi.org/10.1093/mnras/stx258
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Leauthaud, Alexie, Saito, Shun, Hilbert, Stefan, Barreira, Alexandre, More, Surhud, White, Martin, Alam, Shadab, Behroozi, Peter, Bundy, Kevin, Coupon, Jean, Erben, Thomas, Heymans, Catherine, Hildebrandt, Hendrik, Mandelbaum, Rachel, Miller, Lance, Moraes, Bruno, Pereira, Maria E. S., Rodríguez-Torres, Sergio A., Schmidt, Fabian, Shan, Huan-Yuan, Viel, Matteo, and Villaescusa-Navarro, Francisco. Fri . "Lensing is low: cosmology, galaxy formation or new physics?". United States. https://doi.org/10.1093/mnras/stx258. https://www.osti.gov/servlets/purl/1594740.
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@article{osti_1594740,
title = {Lensing is low: cosmology, galaxy formation or new physics?},
author = {Leauthaud, Alexie and Saito, Shun and Hilbert, Stefan and Barreira, Alexandre and More, Surhud and White, Martin and Alam, Shadab and Behroozi, Peter and Bundy, Kevin and Coupon, Jean and Erben, Thomas and Heymans, Catherine and Hildebrandt, Hendrik and Mandelbaum, Rachel and Miller, Lance and Moraes, Bruno and Pereira, Maria E. S. and Rodríguez-Torres, Sergio A. and Schmidt, Fabian and Shan, Huan-Yuan and Viel, Matteo and Villaescusa-Navarro, Francisco},
abstractNote = {Here, we introduce high signal-to-noise galaxy-galaxy lensing measurements of the Baryon Oscillation Spectroscopic Survey constant mass (CMASS) sample using 250 deg2 of weak-lensing data from Canada-France-Hawaii Telescope Lensing Survey and Canada-France-Hawaii Telescope Stripe 82 Survey. We compare this signal with predictions from mock catalogues trained to match observables including the stellar mass function and the projected and two-dimensional clustering of CMASS. We show that the clustering of CMASS, together with standard models of the galaxy-halo connection, robustly predicts a lensing signal that is 20-40 per cent larger than observed. Detailed tests show that our results are robust to a variety of systematic effects. Lowering the value of S8 = σ 8√{Ωm/0.3 compared to Planck Collaboration XIII reconciles the lensing with clustering. However, given the scale of our measurement (r < 10 h-1 Mpc), other effects may also be at play and need to be taken into consideration. We explore the impact of baryon physics, assembly bias, massive neutrinos and modifications to general relativity on ΔΣ and show that several of these effects may be non-negligible given the precision of our measurement. Disentangling cosmological effects from the details of the galaxy-halo connection, the effect of baryons, and massive neutrinos, is the next challenge facing joint lensing and clustering analyses. This is particularly true in the context of large galaxy samples from Baryon Acoustic Oscillation surveys with precise measurements but complex selection functions.},
doi = {10.1093/mnras/stx258},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 467,
place = {United States},
year = {Fri Feb 03 00:00:00 EST 2017},
month = {Fri Feb 03 00:00:00 EST 2017}
}
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    Testing Shear Recovery with Field Distortion
    text, January 2018

    Tests of Gravity with Galaxy Clusters
    text, January 2019

    Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
    text, January 2019

    On the degeneracy between baryon feedback and massive neutrinos as probed by matter clustering and weak lensing
    journal, January 2019

    • Parimbelli, Gabriele; Viel, Matteo; Sefusatti, Emiliano
    • Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 01
    • DOI: 10.1088/1475-7516/2019/01/010

    Modeling assembly bias with machine learning and symbolic regression
    preprint, January 2020

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