TY - JOUR
T1 - Atacama Cosmology Telescope
T2 - Modeling the gas thermodynamics in BOSS CMASS galaxies from kinematic and thermal Sunyaev-Zel'dovich measurements
AU - Amodeo, Stefania
AU - Battaglia, Nicholas
AU - Schaan, Emmanuel
AU - Ferraro, Simone
AU - Moser, Emily
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
AU - Duff, Shannon M.
AU - Duivenvoorden, Adriaan J.
AU - Dunkley, Jo
AU - Dünner, Rolando
AU - Gallardo, Patricio A.
AU - Hall, Kirsten R.
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 - Schillaci, Alessandro
AU - Sehgal, Neelima
AU - Sifón, Cristóbal
AU - Spergel, David N.
AU - Staggs, Suzanne
AU - Storer, Emilie R.
AU - Ullom, Joel N.
AU - Vale, Leila R.
AU - Van Engelen, Alexander
AU - Van Lanen, Jeff
AU - Vavagiakis, Eve M.
AU - Wollack, Edward J.
AU - Xu, Zhilei
N1 - Funding Information:
The authors thank the anonymous referee for their helpful and constructive comments which improved the paper. 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). The Flatiron Institute is funded by the Simons Foundation. 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”. 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. 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). R. D. thanks CONICYT for Grant No. BASAL CATA AFB-170002. D. H., A. M., and N. S. acknowledge support from NSF Grants No. AST-1513618 and No. AST-1907657. M. H. acknowledges support from the National Research Foundation of South Africa. J. P. H. acknowledges funding for SZ cluster studies from NSF AAG No. AST-1615657. K. M. acknowledges support from the National Research Foundation of South Africa. C. S. acknowledges support from the Agencia Nacional de Investigación y Desarrollo (ANID) through FONDECYT Iniciación Grant No. 11191125.
Publisher Copyright:
© 2021 us.
PY - 2021/3/15
Y1 - 2021/3/15
N2 - The thermal and kinematic Sunyaev-Zel'dovich effects (tSZ, kSZ) probe the thermodynamic properties of the circumgalactic and intracluster medium (CGM and ICM) of galaxies, groups, and clusters, since they are proportional, respectively, to the integrated electron pressure and momentum along the line of sight. We present constraints on the gas thermodynamics of CMASS (constant stellar mass) galaxies in the Baryon Oscillation Spectroscopic Survey using new measurements of the kSZ and tSZ signals obtained in a companion paper [Schaan et al.]. Combining kSZ and tSZ measurements, we measure within our model the amplitude of energy injection ϵM⋆c2, where M⋆ is the stellar mass, to be ϵ=(40±9)×10-6, and the amplitude of the nonthermal pressure profile to be αNth<0.2(2σ), indicating that less than 20% of the total pressure within the virial radius is due to a nonthermal component. We estimate the effects of including baryons in the modeling of weak-lensing galaxy cross-correlation measurements using the best-fit density profile from the kSZ measurement. Our estimate reduces the difference between the original theoretical model and the weak-lensing galaxy cross-correlation measurements in [A. Leauthaud et al., Mon. Not. R. Astron. Soc. 467, 3024 (2017)MNRAA40035-871110.1093/mnras/stx258] by half (50% at most), but does not fully reconcile it. Comparing the kSZ and tSZ measurements to cosmological simulations, we find that they underpredict the CGM pressure and to a lesser extent the CGM density at larger radii with probabilities to exceed ranging from 0.00 to 0.03 and 0.12 to 0.14, for tSZ and kSZ, respectively. This suggests that the energy injected via feedback models in the simulations that we compared against does not sufficiently heat the gas at these radii. We do not find significant disagreement at smaller radii. These measurements provide novel tests of current and future simulations. This work demonstrates the power of joint, high signal-to-noise kSZ and tSZ observations, upon which future cross-correlation studies will improve.
AB - The thermal and kinematic Sunyaev-Zel'dovich effects (tSZ, kSZ) probe the thermodynamic properties of the circumgalactic and intracluster medium (CGM and ICM) of galaxies, groups, and clusters, since they are proportional, respectively, to the integrated electron pressure and momentum along the line of sight. We present constraints on the gas thermodynamics of CMASS (constant stellar mass) galaxies in the Baryon Oscillation Spectroscopic Survey using new measurements of the kSZ and tSZ signals obtained in a companion paper [Schaan et al.]. Combining kSZ and tSZ measurements, we measure within our model the amplitude of energy injection ϵM⋆c2, where M⋆ is the stellar mass, to be ϵ=(40±9)×10-6, and the amplitude of the nonthermal pressure profile to be αNth<0.2(2σ), indicating that less than 20% of the total pressure within the virial radius is due to a nonthermal component. We estimate the effects of including baryons in the modeling of weak-lensing galaxy cross-correlation measurements using the best-fit density profile from the kSZ measurement. Our estimate reduces the difference between the original theoretical model and the weak-lensing galaxy cross-correlation measurements in [A. Leauthaud et al., Mon. Not. R. Astron. Soc. 467, 3024 (2017)MNRAA40035-871110.1093/mnras/stx258] by half (50% at most), but does not fully reconcile it. Comparing the kSZ and tSZ measurements to cosmological simulations, we find that they underpredict the CGM pressure and to a lesser extent the CGM density at larger radii with probabilities to exceed ranging from 0.00 to 0.03 and 0.12 to 0.14, for tSZ and kSZ, respectively. This suggests that the energy injected via feedback models in the simulations that we compared against does not sufficiently heat the gas at these radii. We do not find significant disagreement at smaller radii. These measurements provide novel tests of current and future simulations. This work demonstrates the power of joint, high signal-to-noise kSZ and tSZ observations, upon which future cross-correlation studies will improve.
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U2 - 10.1103/PhysRevD.103.063514
DO - 10.1103/PhysRevD.103.063514
M3 - Article
AN - SCOPUS:85103099860
SN - 2470-0010
VL - 103
JO - Physical Review D
JF - Physical Review D
IS - 6
M1 - 063514
ER -