Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. I. Evidence for Thermal Energy Anisotropy Using Oriented Stacking

被引：13

作者：

Lokken, M. ^{[1
,2
,3
]}

Hlozek, R. ^{[1
,2
]}

van Engelen, A. ^{[4
]}

Madhavacheril, M. ^{[5
,6
]}

Baxter, E. ^{[7
]}

DeRose, J. ^{[8
]}

Doux, C. ^{[9
]}

Pandey, S. ^{[9
]}

Rykoff, E. S. ^{[10
]}

Stein, G. ^{[8
,11
]}

To, C. ^{[12
]}

Abbott, T. M. C. ^{[13
]}

Adhikari, S. ^{[14
,15
]}

Aguena, M. ^{[16
]}

Allam, S. ^{[17
]}

Andrade-Oliveira, F. ^{[16
,18
]}

Annis, J. ^{[17
]}

Battaglia, N. ^{[19
]}

Bernstein, G. M. ^{[9
]}

Bertin, E. ^{[20
,21
]}

Bond, J. R. ^{[2
]}

Brooks, D. ^{[22
]}

Calabrese, E. ^{[23
]}

Rosell, A. Carnero ^{[16
,24
,25
]}

Kind, M. Carrasco ^{[26
,27
]}

Carretero, J. ^{[28
]}

Cawthon, R. ^{[29
]}

Choi, A. ^{[30
]}

Costanzi, M. ^{[31
,32
,33
]}

Crocce, M. ^{[34
,35
]}

da Costa, L. N. ^{[16
,36
]}

Pereira, M. E. da Silva ^{[37
]}

De Vicente, J. ^{[38
]}

Desai, S. ^{[39
]}

Dietrich, J. P. ^{[40
]}

Doel, P. ^{[22
]}

Dunkley, J. ^{[41
,42
]}

Everett, S. ^{[43
]}

Evrard, A. E. ^{[37
,44
]}

Ferraro, S. ^{[8
,11
]}

Flaugher, B. ^{[17
]}

Fosalba, P. ^{[34
,35
]}

Frieman, J. ^{[15
,17
]}

Gallardo, P. A. ^{[45
]}

Garcia-Bellido, J. ^{[46
]}

Gaztanaga, E. ^{[34
,35
]}

Gerdes, D. W. ^{[37
,44
]}

Giannantonio, T. ^{[47
,48
]}

Gruen, D. ^{[40
]}

Gruendl, R. A. ^{[26
,27
]}

机构：

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

[2] Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H4, Canada

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

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

[5] Perimeter Inst Theoret Phys, 31 Caroline St N, Waterloo, ON N2L 2Y5, Canada

[6] Univ Southern Calif, Dept Phys & Astron, Los Angeles, CA 90007 USA

[7] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[8] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA

[9] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[10] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[11] Univ Calif Berkeley, Berkeley Ctr Cosmol Phys, 341 Campbell Hall, Berkeley, CA 94720 USA

[12] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[13] Cerro Tololo Interamer Observ, NSFs Natl Opt Infrared Astron Res Lab, Casilla 603, La Serena, Chile

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

[15] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[16] Lab Interinst E Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[17] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[18] Univ Estadual Paulista, Inst Fis Teor, Sao Paulo, Brazil

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

[20] Inst Astrophys Paris, CNRS, UMR 7095, F-75014 Paris, France

[21] Univ Paris 06, Sorbonne Univ, UPMC, Inst Astrophys Paris,UMR 7095, F-75014 Paris, France

[22] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

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

[24] Inst Astrofis Canarias, E-38205 Tenerife, Spain

[25] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain

[26] Natl Ctr Supercomp Applicat, Ctr Astrophys Surveys, 1205 West Clark St, Urbana, IL 61801 USA

[27] Univ Illinois, Dept Astron, 1002 West Green St, Urbana, IL 61801 USA

[28] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, Campus UAB, E-08193 Bellaterra, Barcelona, Spain

[29] Univ Wisconsin, Dept Phys, 2320 Chamberlin Hall,1150 Univ Ave, Madison, WI 53706 USA

[30] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA

[31] Univ Trieste, Dept Phys, Astron Unit, Via Tiepolo 11, I-34131 Trieste, Italy

[32] Osserv Astron Trieste, INAF, Via GB Tiepolo 11, I-34143 Trieste, Italy

[33] Inst Fundamental Phys Universe, Via Beirut 2, I-34014 Trieste, Italy

[34] Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain

[35] CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain

[36] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[37] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[38] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid, Spain

[39] IIT Hyderabad, Dept Phys, Kandi 502285, Telangana, India

[40] Ludwig Maximilians Univ Munchen, Fac Phys, Scheinerstr 1, D-81679 Munich, Germany

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

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

[43] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[44] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[45] Cornell Univ, Dept Phys, Ithaca, NY 14850 USA

[46] Univ Autonoma Madrid, CSIC, UAM, Inst Fis Teor, E-28049 Madrid, Spain

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

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

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

[50] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA

来源：

ASTROPHYSICAL JOURNAL | 2022年 / 933卷 / 02期

基金：

英国科学技术设施理事会; 欧洲研究理事会; 美国国家科学基金会; 新加坡国家研究基金会; 加拿大自然科学与工程研究理事会; 加拿大创新基金会;

关键词：

GALAXY CLUSTERS; POWER SPECTRUM; AGN FEEDBACK; COSMIC WEB; SIMULATIONS; FILAMENTS; CALIBRATION; ALIGNMENTS; STATISTICS; RADIATION;

D O I：

10.3847/1538-4357/ac7043

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The cosmic web contains filamentary structure on a wide range of scales. On the largest scales, superclustering aligns multiple galaxy clusters along intercluster bridges, visible through their thermal Sunyaev-Zel'dovich signal in the cosmic microwave background. We demonstrate a new, flexible method to analyze the hot gas signal from multiscale extended structures. We use a Compton y-map from the Atacama Cosmology Telescope (ACT) stacked on redMaPPer cluster positions from the optical Dark Energy Survey (DES). Cutout images from the y-map are oriented with large-scale structure information from DES galaxy data such that the superclustering signal is aligned before being overlaid. We find evidence of an extended quadrupole moment of the stacked y signal at the 3.5 sigma level, demonstrating that the large-scale thermal energy surrounding galaxy clusters is anisotropically distributed. We compare our ACT x DES results with the Buzzard simulations, finding broad agreement. Using simulations, we highlight the promise of this novel technique for constraining the evolution of anisotropic, non-Gaussian structure using future combinations of microwave and optical surveys.

引用

页数：28

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