Masses of Sunyaev-Zel'dovich galaxy clusters detected by the Atacama Cosmology Telescope: Stacked lensing measurements with Subaru HSC year 3 data

被引：0

作者：

Shirasaki, Masato ^{[1
,2
]}

Sifon, Cristobal ^{[3
]}

Miyatake, Hironao ^{[4
,5
,6
]}

Lau, Erwin ^{[7
]}

Zhang, Zhuowen ^{[8
,9
]}

Bahcall, Neta ^{[10
]}

Battaglia, Nicholas ^{[11
]}

Devlin, Mark ^{[9
,12
]}

Dunkley, Jo ^{[10
,13
]}

Farahi, Arya ^{[14
]}

Hilton, Matt ^{[15
,16
]}

Lin, Yen-Ting ^{[17
]}

Nagai, Daisuke ^{[18
]}

Staggs, Suzanne T. ^{[13
]}

Sunayama, Tomomi ^{[4
,19
]}

Spergel, David ^{[20
]}

Wollack, Edward J. ^{[21
]}

机构：

[1] Natl Inst Nat Sci, Natl Astron Observ Japan NAOJ, Mitaka, Tokyo 1818588, Japan

[2] Inst Stat Math, Tachikawa, Tokyo 1908562, Japan

[3] Pontificia Univ Catolica Valparaiso, Inst Fis, Casilla 4059, Valparaiso, Chile

[4] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Universe, Nagoya 4648602, Japan

[5] Nagoya Univ, Inst Adv Res, Nagoya 4648601, Japan

[6] Univ Tokyo, Inst Adv Study UTIAS, Kavli Inst Phys & Math Universe WPI, Chiba 2778583, Japan

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

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

[9] Fermilab Natl Accelerator Lab, Kirk & Pine Rd, Batavia, IL 60510 USA

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

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

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

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

[14] Univ Texas Austin, Dept Stat & Data Sci, Austin, TX 78712 USA

[15] Univ Witwatersrand, Sch Phys, Private Bag 3, WITS-2050 Johannesburg, South Africa

[16] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys Res Ctr, Westville Campus, ZA-4041 Durban, South Africa

[17] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan

[18] Yale Univ, Dept Phys, New Haven, CT 06520 USA

[19] Univ Arizona, Steward Observ, Tucson, AZ 85704 USA

[20] Simons Fdn, 160 Fifth Ave, New York, NY 10010 USA

[21] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

来源：

PHYSICAL REVIEW D | 2024年 / 110卷 / 10期

基金：

美国国家科学基金会; 新加坡国家研究基金会; 美国国家航空航天局; 日本学术振兴会;

关键词：

DARK-MATTER; HALO-MASS; SHEAR CALIBRATION; ASSEMBLY BIAS; COSMIC SHEAR; DATA RELEASE; SKY SURVEYS; SIMULATIONS; DENSITY; EVOLUTION;

D O I：

10.1103/PhysRevD.110.103006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel'dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a 5 sigma-level SZ threshold in CMB observations from the Atacama Cosmology Telescope, while we define background source galaxies for the lensing analysis with secure photometric redshift cuts in Year 3 data of the Subaru Hyper Suprime Cam survey. We detect the stacked lensing signal in the range of 0.1<R[h(-1) Mpc]<100 in each of three cluster redshift bins, 0.092 <z <= 0.445, 0.445 <z <= 0.695, and 0.695 <z <= 1.180, with 32 galaxy clusters in each bin. The cumulative signal-to-noise ratios of the lensing signal are 14.6, 12.0, and 6.6, respectively. Using a halo-based forward model, we then constrain statistical relationships between the mass inferred from the SZ observation (i.e. SZ mass) and the total mass derived from our stacked lensing measurements. At the average SZ mass in the cluster sample (2.1 -2.4 x10(14)h(-1)M(circle dot)), our likelihood analysis shows that the average total mass differs from the SZ counterpart by a factor of 1.3 +/- 0.2, 1.6 +/- 0.2, and 1.6 +/- 0.3 (68%) in the aforementioned redshift ranges, respectively. Our limits are consistent with previous lensing measurements, and we find that the cluster modeling choices can introduce a 1 sigma-level difference in our parameter inferences.

引用

页数：36

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