The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

被引：77

作者：

Madhavacheril, Mathew S. ^{[1
,2
]}

Qu, Frank J. ^{[3
]}

Sherwin, Blake D. ^{[3
,4
]}

Maccrann, Niall ^{[3
]}

Li, Yaqiong ^{[5
]}

Abril-Cabezas, Irene ^{[3
]}

Ade, Peter A. R. ^{[6
]}

Aiola, Simone ^{[7
,8
]}

Alford, Tommy ^{[9
]}

Amiri, Mandana ^{[10
]}

Amodeo, Stefania ^{[11
]}

An, Rui ^{[12
]}

Atkins, Zachary ^{[8
]}

Austermann, Jason E. ^{[13
]}

Battaglia, Nicholas ^{[14
]}

Battistelli, Elia Stefano ^{[15
]}

Beall, James A. ^{[13
]}

Bean, Rachel ^{[14
]}

Beringue, Benjamin ^{[6
]}

Bhandarkar, Tanay ^{[1
]}

Biermann, Emily ^{[16
]}

Bolliet, Boris ^{[3
]}

Bond, J. Richard ^{[17
]}

Cai, Hongbo ^{[16
]}

Calabrese, Erminia ^{[6
]}

Calafut, Victoria ^{[17
]}

Capalbo, Valentina ^{[15
]}

Carrero, Felipe ^{[18
]}

Challinor, Anthony ^{[3
,4
,19
]}

Chesmore, Grace E. ^{[9
]}

Cho, Hsiao-mei ^{[13
,20
]}

Choi, Steve K. ^{[5
,14
]}

Clark, Susan E. ^{[21
,22
]}

Rosado, Rodrigo Cordova ^{[23
]}

Cothard, Nicholas F. ^{[24
]}

Coughlin, Kevin ^{[9
]}

Coulton, William ^{[7
]}

Crowley, Kevin T. ^{[25
]}

Dalal, Roohi ^{[23
]}

Darwish, Omar ^{[26
]}

Devlin, Mark J. ^{[1
]}

Dicker, Simon ^{[1
]}

Doze, Peter ^{[27
]}

Duell, Cody J. ^{[5
]}

Duff, Shannon M. ^{[13
]}

Duivenvoorden, Adriaan J. ^{[7
,8
]}

Dunkley, Jo ^{[8
,23
]}

Duenner, Rolando ^{[18
]}

Fanfani, Valentina ^{[28
]}

Fankhanel, Max ^{[29
]}

机构：

[1] Univ Penn, Dept Phys & Astron, 209 South 33rd St, Philadelphia, PA 19104 USA

[2] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada

[3] Univ Cambridge, Ctr Math Sci, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England

[4] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England

[5] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA

[6] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[7] Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA

[8] Princeton Univ, Joseph Henry Labs Phys, Jadwin Hall, Princeton, NJ 08544 USA

[9] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[10] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada

[11] Univ Strasbourg, CNRS, Observ Astron Strasbourg, UMR 7550, F-67000 Strasbourg, France

[12] Univ Southern Calif, Dept Phys & Astron, 825 Bloom Walk ACB 439, Los Angeles, CA 90089 USA

[13] NIST Quantum Sensors Grp, 325 Broadway Mailcode 817-03, Boulder, CO 80305 USA

[14] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

[15] Sapienza Univ Rome, Phys Dept, Piazzale Aldo Moro 5, I-00185 Rome, Italy

[16] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA

[17] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada

[18] Pontificia Univ Catolica Chile, Fac Fis, Ctr Astroingn, Av Vicuna Mackenna 4860, Santiago 7820436, Chile

[19] Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[20] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA

[21] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[22] Kavli Inst Particle Astrophys & Cosmol, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[23] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA

[24] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771, Albania

[25] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[26] Hop Univ Geneve, Dept Phys Theor & CAP, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland

[27] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA

[28] Univ Milano Bicocca, Dept Phys, Piazza Sci I-3, I-20126 Milan, MI, Italy

[29] Soc Radiosk & Asesorias Ingn Limitada, Camino Toconao 145-A, Ayllu De Solor, San Pedro De At, Chile

[30] Phys Div, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[31] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA

[32] Univ Paris Saclay, CNRS IN2P3, IJCLab, F-91405 Orsay, France

[33] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[34] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA

[35] Columbia Univ, Dept Phys, New York, NY 10027 USA

[36] Univ Witwatersrand, Wits Ctr Astrophys, Sch Phys, Private Bag 3, ZA-2050 Johannesburg, South Africa

[37] Univ KwaZulu Natal, Astrophys Res Ctr, Sch Math Stat & Comp Sci, ZA-4001 Durban, South Africa

[38] Univ Toronto, David A Dunlap Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[39] Yale Univ, Dept Phys, 217 Prospect St, New Haven, CT 06511 USA

[40] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA

[41] Lincoln Univ, Dept Chem & Phys, Lincoln Univ, PA 19352 USA

[42] SUNY Stony Brook, Phys & Astron Dept, Stony Brook, NY 11794 USA

[43] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[44] Fermilab Natl Accelerator Lab, PO, MS209,POB 500, Batavia, IL 60510 USA

[45] Univ Chicago, Kavli Inst Cosmol Phys, 5640 S Ellis Ave, Chicago, IL 60637 USA

[46] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA

[47] Univ Illinois, Natl Ctr Supercomp Applicat NCSA, 1205 West Clark St, Urbana, IL 61801 USA

[48] Univ Illinois, Dept Astron, West Green St, Urbana, IL 61801 USA

[49] Brookhaven Natl Lab, Upton, NY 11973 USA

[50] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

来源：

ASTROPHYSICAL JOURNAL | 2024年 / 962卷 / 02期

基金：

美国国家科学基金会; 加拿大创新基金会; 新加坡国家研究基金会; 欧洲研究理事会;

关键词：

OSCILLATION SPECTROSCOPIC SURVEY; MICROWAVE BACKGROUND ANISOTROPIES; BARYON ACOUSTIC-OSCILLATIONS; PROBE WMAP OBSERVATIONS; ACCURATE HALO-MODEL; HUBBLE CONSTANT; POWER SPECTRA; DARK ENERGY; MASSIVE NEUTRINOS; CMB TEMPERATURE;

D O I：

10.3847/1538-4357/acff5f

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present cosmological constraints from a gravitational lensing mass map covering 9400 sq. deg(2). reconstructed from CMB measurements made by the Atacama Cosmology Telescope (ACT) from 2017 to 2021. In combination with BAO measurements (from SDSS and 6dF), we obtain the amplitude of matter fluctuations sigma(8)=0.819 +/- 0.015 at 1.8% precision, S-8 equivalent to sigma(8)(Omega(m)/0.3)(0.5)=0.840 +/- 0.028 and the Hubble constant H-0=(68.3 +/- 1.1)kms(-1)Mpc(-1) at 1.6% precision. A joint constraint with CMB lensing measured by the Planck satellite yields even more precise values: sigma(8)=0.812 +/- 0.013, S-8 equivalent to sigma(8)(Omega m/0.3)(0.5)=0.831 +/- 0.023 and H-0=(68.1 +/- 1.0)kms(-1)Mpc(-1). These measurements agree well with Lambda CDM-model extrapolations from the CMB anisotropies measured by Planck. To compare these constraints to those from the KiDS, DES, and HSC galaxy surveys, we revisit those data sets with a uniform set of assumptions, and find S-8 from all three surveys are lower than that from ACT+Planck lensing by varying levels ranging from 1.7-2.1 sigma. These results motivate further measurements and comparison, not just between the CMB anisotropies and galaxy lensing, but also between CMB lensing probing z similar to 0.5-5 on mostly-linear scales and galaxy lensing at z similar to 0.5 on smaller scales. We combine our CMB lensing measurements with CMB anisotropies to constrain extensions of Lambda CDM, limiting the sum of the neutrino masses to & sum;m(nu)<0.12 eV (95% c.l.), for example. Our results provide independent confirmation that the universe is spatially flat, conforms with general relativity, and is described remarkably well by the Lambda CDM model, while paving a promising path for neutrino physics with gravitational lensing from upcoming ground-based CMB surveys

引用

页数：22

共 166 条

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