publication . Article . Preprint . 2019

Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zel’dovich effect cross-correlations

Pandey, S.; Baxter, E. J.; Xu, Z.; Orlowski-Scherer, J.; Zhu, N.; Lidz, A.; Aguirre, J.; DeRose, J.; Devlin, M.; Hill, J. C.; ...
Open Access English
  • Published: 16 Sep 2019
  • Publisher: HAL CCSD
  • Country: France
Abstract
An understanding of astrophysical feedback is important for constraining models of galaxy formation and for extracting cosmological information from current and future weak lensing surveys. The thermal Sunyaev-Zel'dovich effect, quantified via the Compton-$y$ parameter, is a powerful tool for studying feedback, because it directly probes the pressure of the hot, ionized gas residing in dark matter halos. Cross-correlations between galaxies and maps of Compton-$y$ obtained from cosmic microwave background surveys are sensitive to the redshift evolution of the gas pressure, and its dependence on halo mass. In this work, we use galaxies identified in year one data ...
Persistent Identifiers
Subjects
arXiv: Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy Astrophysics
free text keywords: Cosmology, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics, Correlation and dependence, Library science, Research council, European union, media_common.cataloged_instance, media_common, European research, Fundamental physics, Christian ministry, High energy, Physics, Higher education, business.industry, business
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Communities with gateway
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Funded by
EC| TESTDE
Project
TESTDE
Testing the Dark Energy Paradigm and Measuring Neutrino Mass with the Dark Energy Survey
  • Funder: European Commission (EC)
  • Project Code: 291329
  • Funding stream: FP7 | SP2 | ERC
,
EC| COSMICDAWN
Project
COSMICDAWN
Understanding the Origin of Cosmic Structure
  • Funder: European Commission (EC)
  • Project Code: 306478
  • Funding stream: FP7 | SP2 | ERC
,
EC| COGS
Project
COGS
Capitalizing on Gravitational Shear
  • Funder: European Commission (EC)
  • Project Code: 240672
  • Funding stream: FP7 | SP2 | ERC
,
NSF| Advanced ACTPol
Project
  • Funder: National Science Foundation (NSF)
  • Project Code: 1440226
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
,
NSF| Collaborative Research: The Dark Energy Survey Data Management Operations
Project
  • Funder: National Science Foundation (NSF)
  • Project Code: 1138766
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
72 references, page 1 of 5

[1] Abazajian K. N., et al., 2016, preprint, (arXiv:1610.02743)

[2] Ade P., et al., 2019, Journal of Cosmology and Astro-Particle Physics, 2019, 056

[3] Aghanim P. C. N., Arnaud M., Ashdown M., Aumont J., Baccigalupi C., Banday A. J., Barreiro R. B., 2015, arXiv: 1502.01596v1 [astro-ph.CO 10.1051/0004-6361/201525826, p. 25

[4] Battaglia N., Bond J. R., Pfrommer C., Sievers J. L., Sijacki D., 2010, ApJ, 725, 91

[5] Battaglia N., Bond J. R., Pfrommer C., Sievers J. L., 2012, ApJ, 758, 75

[6] Benson B. A., et al., 2014, in Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. p. 91531P (arXiv:1407.2973), doi:10.1117/12.2057305

[7] Böhringer H., Werner N., 2010, A&A Rev., 18, 127

[8] Bruzual G., Charlot S., 2003, MNRAS, 344, 1000

[9] Carlstrom J. E., Holder G. P., Reese E. D., 2002, Annual Review of Astronomy and Astrophysics, 40, 643

[10] Carlstrom J. E., et al., 2011, Publications of the Astronomical Society of the Pacific, 123, 568

[11] Carretero J., Castander F. J., Gaztañaga E., Crocce M., Fosalba P., 2015, MNRAS, 447, 646

[12] Cawthon R., et al., 2018, MNRAS, 481, 2427

[13] Cooray A., Sheth R., 2002, Phys. Rep., 372, 1

[14] Crocce M., Castander F. J., Gaztañaga E., Fosalba P., Carretero J., 2015, MNRAS, 453, 1513

[15] DES Collaboration et al., 2017, preprint, (arXiv:1708.01530)

72 references, page 1 of 5
Abstract
An understanding of astrophysical feedback is important for constraining models of galaxy formation and for extracting cosmological information from current and future weak lensing surveys. The thermal Sunyaev-Zel'dovich effect, quantified via the Compton-$y$ parameter, is a powerful tool for studying feedback, because it directly probes the pressure of the hot, ionized gas residing in dark matter halos. Cross-correlations between galaxies and maps of Compton-$y$ obtained from cosmic microwave background surveys are sensitive to the redshift evolution of the gas pressure, and its dependence on halo mass. In this work, we use galaxies identified in year one data ...
Persistent Identifiers
Subjects
arXiv: Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy Astrophysics
free text keywords: Cosmology, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics, Correlation and dependence, Library science, Research council, European union, media_common.cataloged_instance, media_common, European research, Fundamental physics, Christian ministry, High energy, Physics, Higher education, business.industry, business
Communities
Communities with gateway
OpenAIRE Connect image
Funded by
EC| TESTDE
Project
TESTDE
Testing the Dark Energy Paradigm and Measuring Neutrino Mass with the Dark Energy Survey
  • Funder: European Commission (EC)
  • Project Code: 291329
  • Funding stream: FP7 | SP2 | ERC
,
EC| COSMICDAWN
Project
COSMICDAWN
Understanding the Origin of Cosmic Structure
  • Funder: European Commission (EC)
  • Project Code: 306478
  • Funding stream: FP7 | SP2 | ERC
,
EC| COGS
Project
COGS
Capitalizing on Gravitational Shear
  • Funder: European Commission (EC)
  • Project Code: 240672
  • Funding stream: FP7 | SP2 | ERC
,
NSF| Advanced ACTPol
Project
  • Funder: National Science Foundation (NSF)
  • Project Code: 1440226
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
,
NSF| Collaborative Research: The Dark Energy Survey Data Management Operations
Project
  • Funder: National Science Foundation (NSF)
  • Project Code: 1138766
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
72 references, page 1 of 5

[1] Abazajian K. N., et al., 2016, preprint, (arXiv:1610.02743)

[2] Ade P., et al., 2019, Journal of Cosmology and Astro-Particle Physics, 2019, 056

[3] Aghanim P. C. N., Arnaud M., Ashdown M., Aumont J., Baccigalupi C., Banday A. J., Barreiro R. B., 2015, arXiv: 1502.01596v1 [astro-ph.CO 10.1051/0004-6361/201525826, p. 25

[4] Battaglia N., Bond J. R., Pfrommer C., Sievers J. L., Sijacki D., 2010, ApJ, 725, 91

[5] Battaglia N., Bond J. R., Pfrommer C., Sievers J. L., 2012, ApJ, 758, 75

[6] Benson B. A., et al., 2014, in Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. p. 91531P (arXiv:1407.2973), doi:10.1117/12.2057305

[7] Böhringer H., Werner N., 2010, A&A Rev., 18, 127

[8] Bruzual G., Charlot S., 2003, MNRAS, 344, 1000

[9] Carlstrom J. E., Holder G. P., Reese E. D., 2002, Annual Review of Astronomy and Astrophysics, 40, 643

[10] Carlstrom J. E., et al., 2011, Publications of the Astronomical Society of the Pacific, 123, 568

[11] Carretero J., Castander F. J., Gaztañaga E., Crocce M., Fosalba P., 2015, MNRAS, 447, 646

[12] Cawthon R., et al., 2018, MNRAS, 481, 2427

[13] Cooray A., Sheth R., 2002, Phys. Rep., 372, 1

[14] Crocce M., Castander F. J., Gaztañaga E., Fosalba P., Carretero J., 2015, MNRAS, 453, 1513

[15] DES Collaboration et al., 2017, preprint, (arXiv:1708.01530)

72 references, page 1 of 5
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