Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos

Emmanuel Schaan; Simone Ferraro; Stefania Amodeo; Nicholas Battaglia; Simone Aiola; Jason E. Austermann; James A. Beall; Rachel Bean; Daniel T. Becker; Richard J. Bond; Erminia Calabrese; Victoria Calafut; Steve K. Choi; Edward V. Denison; Mark J. Devlin; Shannon M. Duff; Adriaan J. Duivenvoorden; Jo Dunkley; Rolando Dünner; Patricio A. Gallardo; Yilun Guan; Dongwon Han; J. Colin Hill; Gene C. Hilton; Matt Hilton; Renée HloŽek; Johannes Hubmayr; Kevin M. Huffenberger; John P. Hughes; Brian J. Koopman; Amanda Macinnis; Jeff McMahon; Mathew S. Madhavacheril; Kavilan Moodley; Tony Mroczkowski; Sigurd Naess; Federico Nati; Laura B. Newburgh; Michael D. Niemack; Lyman A. Page; Bruce Partridge; Maria Salatino; Neelima Sehgal; Alessandro Schillaci; Cristóbal Sifón; Kendrick M. Smith; David N. Spergel; Suzanne Staggs; Emilie R. Storer; Hy Trac; Joel N. Ullom; Jeff Van Lanen; Leila R. Vale; Alexander Van Engelen; Mariana Vargas Magaña; Eve M. Vavagiakis; Edward J. Wollack; Zhilei Xu

doi:10.1103/PhysRevD.103.063513

Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos

Emmanuel Schaan, Simone Ferraro, Stefania Amodeo, Nicholas Battaglia, Simone Aiola, Jason E. Austermann, James A. Beall, Rachel Bean, Daniel T. Becker, Richard J. Bond, Erminia Calabrese, Victoria Calafut, Steve K. Choi, Edward V. Denison, Mark J. Devlin, Shannon M. Duff, Adriaan J. Duivenvoorden, Jo Dunkley, Rolando Dünner, Patricio A. GallardoYilun Guan, Dongwon Han, J. Colin Hill, Gene C. Hilton, Matt Hilton, Renée HloŽek, Johannes Hubmayr, Kevin M. Huffenberger, John P. Hughes, Brian J. Koopman, Amanda Macinnis, Jeff McMahon, Mathew S. Madhavacheril, Kavilan Moodley, Tony Mroczkowski, Sigurd Naess, Federico Nati, Laura B. Newburgh, Michael D. Niemack, Lyman A. Page, Bruce Partridge, Maria Salatino, Neelima Sehgal, Alessandro Schillaci, Cristóbal Sifón, Kendrick M. Smith, David N. Spergel, Suzanne Staggs, Emilie R. Storer, Hy Trac, Joel N. Ullom, Jeff Van Lanen, Leila R. Vale, Alexander Van Engelen, Mariana Vargas Magaña, Eve M. Vavagiakis, Edward J. Wollack, Zhilei Xu

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Abstract

The scattering of cosmic microwave background (CMB) photons off the free-electron gas in galaxies and clusters leaves detectable imprints on high resolution CMB maps: the thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ respectively).

Original language	English (US)
Article number	063513
Journal	Physical Review D
Volume	103
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevD.103.063513
State	Published - Mar 15 2021

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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10.1103/PhysRevD.103.063513

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Schaan, E., Ferraro, S., Amodeo, S., Battaglia, N., Aiola, S., Austermann, J. E., Beall, J. A., Bean, R., Becker, D. T., Bond, R. J., Calabrese, E., Calafut, V., Choi, S. K., Denison, E. V., Devlin, M. J., Duff, S. M., Duivenvoorden, A. J., Dunkley, J., Dünner, R., ... Xu, Z. (2021). Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos. Physical Review D, 103(6), Article 063513. https://doi.org/10.1103/PhysRevD.103.063513

@article{a4b9be390ab9419faaadb0077388222a,

title = "Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos",

abstract = "The scattering of cosmic microwave background (CMB) photons off the free-electron gas in galaxies and clusters leaves detectable imprints on high resolution CMB maps: the thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ respectively).",

author = "Emmanuel Schaan and Simone Ferraro and Stefania Amodeo and Nicholas Battaglia and Simone Aiola and Austermann, {Jason E.} and Beall, {James A.} and Rachel Bean and Becker, {Daniel T.} and Bond, {Richard J.} and Erminia Calabrese and Victoria Calafut and Choi, {Steve K.} and Denison, {Edward V.} and Devlin, {Mark J.} and Duff, {Shannon M.} and Duivenvoorden, {Adriaan J.} and Jo Dunkley and Rolando D{\"u}nner and Gallardo, {Patricio A.} and Yilun Guan and Dongwon Han and Hill, {J. Colin} and Hilton, {Gene C.} and Matt Hilton and Ren{\'e}e Hlo{\v Z}ek and Johannes Hubmayr and Huffenberger, {Kevin M.} and Hughes, {John P.} and Koopman, {Brian J.} and Amanda Macinnis and Jeff McMahon and Madhavacheril, {Mathew S.} and Kavilan Moodley and Tony Mroczkowski and Sigurd Naess and Federico Nati and Newburgh, {Laura B.} and Niemack, {Michael D.} and Page, {Lyman A.} and Bruce Partridge and Maria Salatino and Neelima Sehgal and Alessandro Schillaci and Crist{\'o}bal Sif{\'o}n and Smith, {Kendrick M.} and Spergel, {David N.} and Suzanne Staggs and Storer, {Emilie R.} and Hy Trac and Ullom, {Joel N.} and {Van Lanen}, Jeff and Vale, {Leila R.} and {Van Engelen}, Alexander and Maga{\~n}a, {Mariana Vargas} and Vavagiakis, {Eve M.} and Wollack, {Edward J.} and Zhilei Xu",

note = "Funding Information: We thank the anonymous referees for their insightful suggestions which improved this article. We thank Shirley Ho, Eliot Quataert, Chung-Pei Ma, Uro{\v s} Seljak and Martin White for their comments and suggestions on this work. E. S. is supported by the Chamberlain fellowship at Lawrence Berkeley National Laboratory. S. F. is supported by the Physics Division of Lawrence Berkeley National Laboratory. N. B. acknowledges support from NSF Grant No. AST-1910021. N. B. and J. C. H. acknowledge support from the Research and Technology Development fund at the Jet Propulsion Laboratory through the project entitled “Mapping the Baryonic Majority.” This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We used the software VisIt to generate the 3D visualization of the galaxy catalog and reconstructed velocities. This work was supported by the U.S. National Science Foundation through Grants No. AST-1440226, No. AST0965625 and No. AST-0408698 for the ACT project, as well as Grants No. PHY-1214379 and No. PHY-0855887. Funding was also provided by Princeton University, the University of Pennsylvania, and a Canada Foundation for Innovation (CFI) award to UBC. ACT operates in the Parque Astron{\'o}mico Atacama in northern Chile under the auspices of the Comisi{\'o}n Nacional de Investigaci{\'o}n Cient{\'i}fica y Tecnol{\'o}gica de Chile (CONICYT). Computations were performed on the GPC and Niagara supercomputers at the SciNet HPC Consortium. SciNet is funded by the CFI under the auspices of Compute Canada, the Government of Ontario, the Ontario Research Fund—Research Excellence; and the University of Toronto. The development of multichroic detectors and lenses was supported by NASA Grants No. NNX13AE56G and No. NNX14AB58G. Colleagues at AstroNorte and RadioSky provide logistical support and keep operations in Chile running smoothly. We also thank the Mishrahi Fund and the Wilkinson Fund for their generous support of the project. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site in (See Ref. ). SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. R. D. thanks CONICYT for Grant No. BASAL CATA AFB-170002. The Flatiron Institute is funded by the Simons Foundation. E. C. acknowledges support from the STFC Ernest Rutherford Fellowship ST/M004856/2 and STFC Consolidated Grant No. ST/S00033X/1, and from the Horizon 2020 ERC Starting Grant (Grant agreement No. 849169). J. D. is supported through NSF Grant No. AST-1814971. J. P. H. acknowledges funding for SZ cluster studies from NSF Grant No. AST-1615657. K. M. acknowledges support from the National Research Foundation of South Africa. D. H., A. M., and N. S. acknowledge support from NSF Grants No. AST-1513618 and No. AST-1907657. M. Hi. acknowledges support from the National Research Foundation of South Africa. Publisher Copyright: {\textcopyright}=0.55 and host halo mass ⟨Mvir ",

year = "2021",

month = mar,

day = "15",

doi = "10.1103/PhysRevD.103.063513",

language = "English (US)",

volume = "103",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "6",

}

Schaan, E, Ferraro, S, Amodeo, S, Battaglia, N, Aiola, S, Austermann, JE, Beall, JA, Bean, R, Becker, DT, Bond, RJ, Calabrese, E, Calafut, V, Choi, SK, Denison, EV, Devlin, MJ, Duff, SM, Duivenvoorden, AJ, Dunkley, J, Dünner, R, Gallardo, PA, Guan, Y, Han, D, Hill, JC, Hilton, GC, Hilton, M, HloŽek, R, Hubmayr, J, Huffenberger, KM, Hughes, JP, Koopman, BJ, Macinnis, A, McMahon, J, Madhavacheril, MS, Moodley, K, Mroczkowski, T, Naess, S, Nati, F, Newburgh, LB, Niemack, MD, Page, LA, Partridge, B, Salatino, M, Sehgal, N, Schillaci, A, Sifón, C, Smith, KM, Spergel, DN, Staggs, S, Storer, ER, Trac, H, Ullom, JN, Van Lanen, J, Vale, LR, Van Engelen, A, Magaña, MV, Vavagiakis, EM, Wollack, EJ & Xu, Z 2021, 'Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos', Physical Review D, vol. 103, no. 6, 063513. https://doi.org/10.1103/PhysRevD.103.063513

TY - JOUR

T1 - Atacama Cosmology Telescope

T2 - Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos

AU - Schaan, Emmanuel

AU - Ferraro, Simone

AU - Amodeo, Stefania

AU - Battaglia, Nicholas

AU - Aiola, Simone

AU - Austermann, Jason E.

AU - Beall, James A.

AU - Bean, Rachel

AU - Becker, Daniel T.

AU - Bond, Richard J.

AU - Calabrese, Erminia

AU - Calafut, Victoria

AU - Choi, Steve K.

AU - Denison, Edward V.

AU - Devlin, Mark J.

AU - Duff, Shannon M.

AU - Duivenvoorden, Adriaan J.

AU - Dunkley, Jo

AU - Dünner, Rolando

AU - Gallardo, Patricio A.

AU - Guan, Yilun

AU - Han, Dongwon

AU - Hill, J. Colin

AU - Hilton, Gene C.

AU - Hilton, Matt

AU - HloŽek, Renée

AU - Hubmayr, Johannes

AU - Huffenberger, Kevin M.

AU - Hughes, John P.

AU - Koopman, Brian J.

AU - Macinnis, Amanda

AU - McMahon, Jeff

AU - Madhavacheril, Mathew S.

AU - Moodley, Kavilan

AU - Mroczkowski, Tony

AU - Naess, Sigurd

AU - Nati, Federico

AU - Newburgh, Laura B.

AU - Niemack, Michael D.

AU - Page, Lyman A.

AU - Partridge, Bruce

AU - Salatino, Maria

AU - Sehgal, Neelima

AU - Schillaci, Alessandro

AU - Sifón, Cristóbal

AU - Smith, Kendrick M.

AU - Spergel, David N.

AU - Staggs, Suzanne

AU - Storer, Emilie R.

AU - Trac, Hy

AU - Ullom, Joel N.

AU - Van Lanen, Jeff

AU - Vale, Leila R.

AU - Van Engelen, Alexander

AU - Magaña, Mariana Vargas

AU - Vavagiakis, Eve M.

AU - Wollack, Edward J.

AU - Xu, Zhilei

N1 - Funding Information: We thank the anonymous referees for their insightful suggestions which improved this article. We thank Shirley Ho, Eliot Quataert, Chung-Pei Ma, Uroš Seljak and Martin White for their comments and suggestions on this work. E. S. is supported by the Chamberlain fellowship at Lawrence Berkeley National Laboratory. S. F. is supported by the Physics Division of Lawrence Berkeley National Laboratory. N. B. acknowledges support from NSF Grant No. AST-1910021. N. B. and J. C. H. acknowledge support from the Research and Technology Development fund at the Jet Propulsion Laboratory through the project entitled “Mapping the Baryonic Majority.” This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We used the software VisIt to generate the 3D visualization of the galaxy catalog and reconstructed velocities. This work was supported by the U.S. National Science Foundation through Grants No. AST-1440226, No. AST0965625 and No. AST-0408698 for the ACT project, as well as Grants No. PHY-1214379 and No. PHY-0855887. Funding was also provided by Princeton University, the University of Pennsylvania, and a Canada Foundation for Innovation (CFI) award to UBC. ACT operates in the Parque Astronómico Atacama in northern Chile under the auspices of the Comisión Nacional de Investigación Científica y Tecnológica de Chile (CONICYT). Computations were performed on the GPC and Niagara supercomputers at the SciNet HPC Consortium. SciNet is funded by the CFI under the auspices of Compute Canada, the Government of Ontario, the Ontario Research Fund—Research Excellence; and the University of Toronto. The development of multichroic detectors and lenses was supported by NASA Grants No. NNX13AE56G and No. NNX14AB58G. Colleagues at AstroNorte and RadioSky provide logistical support and keep operations in Chile running smoothly. We also thank the Mishrahi Fund and the Wilkinson Fund for their generous support of the project. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site in (See Ref. ). SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. R. D. thanks CONICYT for Grant No. BASAL CATA AFB-170002. The Flatiron Institute is funded by the Simons Foundation. E. C. acknowledges support from the STFC Ernest Rutherford Fellowship ST/M004856/2 and STFC Consolidated Grant No. ST/S00033X/1, and from the Horizon 2020 ERC Starting Grant (Grant agreement No. 849169). J. D. is supported through NSF Grant No. AST-1814971. J. P. H. acknowledges funding for SZ cluster studies from NSF Grant No. AST-1615657. K. M. acknowledges support from the National Research Foundation of South Africa. D. H., A. M., and N. S. acknowledge support from NSF Grants No. AST-1513618 and No. AST-1907657. M. Hi. acknowledges support from the National Research Foundation of South Africa. Publisher Copyright: ©=0.55 and host halo mass ⟨Mvir

PY - 2021/3/15

Y1 - 2021/3/15

N2 - The scattering of cosmic microwave background (CMB) photons off the free-electron gas in galaxies and clusters leaves detectable imprints on high resolution CMB maps: the thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ respectively).

AB - The scattering of cosmic microwave background (CMB) photons off the free-electron gas in galaxies and clusters leaves detectable imprints on high resolution CMB maps: the thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ respectively).

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U2 - 10.1103/PhysRevD.103.063513

DO - 10.1103/PhysRevD.103.063513

M3 - Article

AN - SCOPUS:85103087831

SN - 2470-0010

VL - 103

JO - Physical Review D

JF - Physical Review D

IS - 6

M1 - 063513

ER -

Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos

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