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Space Science Reviews

, 215:17 | Cite as

Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects

A Millimetre/Submillimetre Probe of the Warm and Hot Universe
  • Tony MroczkowskiEmail author
  • Daisuke Nagai
  • Kaustuv Basu
  • Jens Chluba
  • Jack Sayers
  • Rémi Adam
  • Eugene Churazov
  • Abigail Crites
  • Luca Di Mascolo
  • Dominique Eckert
  • Juan Macias-Perez
  • Frédéric Mayet
  • Laurence Perotto
  • Etienne Pointecouteau
  • Charles Romero
  • Florian Ruppin
  • Evan Scannapieco
  • John ZuHone
Article
Part of the following topical collections:
  1. Clusters of Galaxies: Physics and Cosmology

Abstract

In recent years, observations of the Sunyaev-Zeldovich (SZ) effect have had significant cosmological implications and have begun to serve as a powerful and independent probe of the warm and hot gas that pervades the Universe. As a few pioneering studies have already shown, SZ observations both complement X-ray observations—the traditional tool for studying the intra-cluster medium—and bring unique capabilities for probing astrophysical processes at high redshifts and out to the low-density regions in the outskirts of galaxy clusters. Advances in SZ observations have largely been driven by developments in centimetre-, millimetre-, and submillimetre-wave instrumentation on ground-based facilities, with notable exceptions including results from the Planck satellite. Here we review the utility of the thermal, kinematic, relativistic, non-thermal, and polarised SZ effects for studies of galaxy clusters and other large scale structures, incorporating the many advances over the past two decades that have impacted SZ theory, simulations, and observations. We also discuss observational results, techniques, and challenges, and aim to give an overview and perspective on emerging opportunities, with the goal of highlighting some of the exciting new directions in this field.

Keywords

Sunyaev-Zeldovich effect Clusters of galaxies Intra-cluster medium Millimetre and submillimetre-wave astronomy Cosmology 

Notes

Acknowledgements

We thank ISSI for the opportunity to provide this invited review. T.M. is supported for scientific activities by ESO’s Directorate for Science. D.N. acknowledges Yale University for granting a triennial leave and the Max-Planck-Institut für Astrophysik for hospitality when this work was carried out. J.C. is supported by the Royal Society as a Royal Society University Research Fellow at the University of Manchester, U.K. R.A. acknowledges support from Spanish Ministerio de Economía and Competitividad (MINECO) through grant number AYA2015-66211-C2-2. K.B. acknowledges partial funding from the Transregio programme TRR33 of the Deutsche Forschungsgemeinschaft (DFG). A.T.C. is supported by the National Science Foundation Astronomy and Astrophysics Postdoctoral Fellowship under Grant No. 1602677. F.M., L.P., J.F.M.P., and F.R. acknowledge funding from the French ANR under the contract ANR-15-CE31-0017 and from the ENIGMASS LabEx.

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Copyright information

© Springer Nature B.V. 2019

Authors and Affiliations

  • Tony Mroczkowski
    • 1
    Email author
  • Daisuke Nagai
    • 2
    • 3
  • Kaustuv Basu
    • 4
  • Jens Chluba
    • 5
  • Jack Sayers
    • 6
  • Rémi Adam
    • 7
  • Eugene Churazov
    • 8
    • 9
  • Abigail Crites
    • 10
  • Luca Di Mascolo
    • 8
  • Dominique Eckert
    • 11
  • Juan Macias-Perez
    • 12
  • Frédéric Mayet
    • 12
  • Laurence Perotto
    • 12
  • Etienne Pointecouteau
    • 13
  • Charles Romero
    • 14
  • Florian Ruppin
    • 12
    • 15
  • Evan Scannapieco
    • 16
  • John ZuHone
    • 17
  1. 1.European Southern Observatory (ESO)GarchingGermany
  2. 2.Department of PhysicsYale UniversityNew HavenUSA
  3. 3.Yale Center for Astronomy and AstrophysicsNew HavenUSA
  4. 4.Argelander-Institut für AstronomieUniversität BonnBonnGermany
  5. 5.Jodrell Bank Centre for Astrophysics, School of Physics and AstronomyThe University of ManchesterManchesterUK
  6. 6.Division of Physics, Math, and AstronomyCalifornia Institute of TechnologyPasadenaUSA
  7. 7.Laboratoire Leprince-Ringuet (LLR)PalaiseauFrance
  8. 8.Max-Planck-Institut für AstrophysikGarchingGermany
  9. 9.Space Research InstituteMoscowRussia
  10. 10.Department of PhysicsCalifornia Institute of TechnologyPasadenaUSA
  11. 11.Department of AstronomyUniversity of GenevaVersoixSwitzerland
  12. 12.LPSC-IN2P3Univ. Grenoble Alpes, CNRS, Grenoble INPGrenobleFrance
  13. 13.IRAPUniversité de Toulouse, CNRS, CNES, UPSToulouseFrance
  14. 14.University of PennsylvaniaPhiladelphiaUSA
  15. 15.Kavli Institute for Astrophysics and Space ResearchMassachusetts Institute of TechnologyCambridgeUSA
  16. 16.School of Earth and Space ExplorationArizona State UniversityTempeUSA
  17. 17.Smithsonian Astrophysical ObservatoryCambridgeUSA

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