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 | |
State | Published - Mar 15 2021 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
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In: Physical Review D, Vol. 103, No. 6, 063513, 15.03.2021.
Research output: Contribution to journal › Article › peer-review
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).
UR - http://www.scopus.com/inward/record.url?scp=85103087831&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85103087831&partnerID=8YFLogxK
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 -