当前位置: X-MOL 学术J. Cosmol. Astropart. Phys. › 论文详情
Our official English website, www.x-mol.net, welcomes your feedback! (Note: you will need to create a separate account there.)
The Atacama Cosmology Telescope: a measurement of the Cosmic Microwave Background power spectra at 98 and 150 GHz
Journal of Cosmology and Astroparticle Physics ( IF 6.4 ) Pub Date : 2020-12-30 , DOI: 10.1088/1475-7516/2020/12/045
Steve K. Choi 1, 2, 3 , Matthew Hasselfield 4, 5, 6 , Shuay-Pwu Patty Ho 3 , Brian Koopman 7 , Marius Lungu 3, 8 , Maximilian H. Abitbol 9 , Graeme E. Addison 10 , Peter A. R. Ade 11 , Simone Aiola 3, 4 , David Alonso 9 , Mandana Amiri 12 , Stefania Amodeo 2 , Elio Angile 8 , Jason E. Austermann 13 , Taylor Baildon 14 , Nick Battaglia 2 , James A. Beall 13 , Rachel Bean 2 , Daniel T. Becker 13 , J Richard Bond 15 , Sarah Marie Bruno 3 , Erminia Calabrese 11 , Victoria Calafut 2 , Luis E. Campusano 16 , Felipe Carrero 17 , Grace E. Chesmore 18 , Hsiao-mei Cho 13, 19 , Susan E. Clark 20 , Nicholas F. Cothard 21 , Devin Crichton 22 , Kevin T. Crowley 3, 23 , Omar Darwish 24 , Rahul Datta 10 , Edward V. Denison 13 , Mark J. Devlin 8 , Cody J. Duell 1 , Shannon M. Duff 13 , Adriaan J. Duivenvoorden 3 , Jo Dunkley 3, 25 , Rolando Dünner 26 , Thomas Essinger-Hileman 27 , Max Fankhanel 17 , Simone Ferraro 28 , Anna E. Fox 13 , Brittany Fuzia 29 , Patricio A. Gallardo 1 , Vera Gluscevic 30 , Joseph E. Golec 18 , Emily Grace 3 , Megan Gralla 31 , Yilun Guan 32 , Kirsten Hall 10 , Mark Halpern 12 , Dongwon Han 33 , Peter Hargrave 11 , Shawn Henderson 19 , Brandon Hensley 25 , J. Colin Hill 4, 34 , Gene C. Hilton 13 , Matt Hilton 22 , Adam D. Hincks 35 , Renée Hložek 35, 36 , Johannes Hubmayr 13 , Kevin M. Huffenberger 29 , John P. Hughes 37 , Leopoldo Infante 26 , Kent Irwin 38 , Rebecca Jackson 18 , Jeff Klein 8 , Kenda Knowles 22 , Arthur Kosowsky 32 , Vincent Lakey 29 , Dale Li 13, 19 , Yaqiong Li 3 , Zack Li 25 , Martine Lokken 15, 35 , Thibaut Louis 39 , Amanda MacInnis 33 , Mathew Madhavacheril 40 , Felipe Maldonado 29 , Maya Mallaby-Kay 41 , Danica Marsden 8 , Loïc Maurin 26, 42 , Jeff McMahon 14, 18, 41, 43, 44 , Felipe Menanteau 45, 46 , Kavilan Moodley 22 , Tim Morton 30 , Sigurd Naess 4 , Toshiya Namikawa 24 , Federico Nati 8, 47 , Laura Newburgh 7 , John P. Nibarger 13 , Andrina Nicola 25 , Michael D. Niemack 1, 2 , Michael R. Nolta 15 , John Orlowski-Sherer 8 , Lyman A. Page 3 , Christine G. Pappas 13 , Bruce Partridge 48 , Phumlani Phakathi 22 , Heather Prince 25 , Roberto Puddu 26 , Frank J. Qu 24 , Jesus Rivera 37 , Naomi Robertson 49 , Felipe Rojas 17, 26 , Maria Salatino 38, 50 , Emmanuel Schaan 28 , Alessandro Schillaci 51 , Benjamin L. Schmitt 8 , Neelima Sehgal 33 , Blake D. Sherwin 24 , Carlos Sierra 18 , Jon Sievers 52 , Cristobal Sifon 53 , Precious Sikhosana 22 , Sara Simon 14 , David N. Spergel 4, 25 , Suzanne T. Staggs 3 , Jason Stevens 1 , Emilie Storer 3 , Dhaneshwar D. Sunder 22 , Eric R. Switzer 27 , Ben Thorne 54 , Robert Thornton 8, 55 , Hy Trac 56 , Jesse Treu 57 , Carole Tucker 11 , Leila R. Vale 13 , Alexander Van Engelen 58 , Jeff Van Lanen 13 , Eve M. Vavagiakis 1 , Kasey Wagoner 3 , Yuhan Wang 3 , Jonathan T. Ward 8 , Edward J. Wollack 27 , Zhilei Xu 8 , Fernando Zago 52 , Ningfeng Zhu 8
Affiliation  

We present the temperature and polarization angular power spectra of the CMB measured by the Atacama Cosmology Telescope (ACT) from 5400 deg$^2$ of the 2013-2016 survey, which covers $>$15000 deg$^2$ at 98 and 150 GHz. For this analysis we adopt a blinding strategy to help avoid confirmation bias and, related to this, show numerous checks for systematic error done before unblinding. Using the likelihood for the cosmological analysis we constrain secondary sources of anisotropy and foreground emission, and derive a "CMB-only" spectrum that extends to $\ell=4000$. At large angular scales, foreground emission at 150 GHz is $\sim$1% of TT and EE within our selected regions and consistent with that found by Planck. Using the same likelihood, we obtain the cosmological parameters for $\Lambda$CDM for the ACT data alone with a prior on the optical depth of $\tau=0.065\pm0.015$. $\Lambda$CDM is a good fit. The best-fit model has a reduced $\chi^2$ of 1.07 (PTE=0.07) with $H_0=67.9\pm1.5$ km/s/Mpc. We show that the lensing BB signal is consistent with $\Lambda$CDM and limit the celestial EB polarization angle to $\psi_P =-0.09^{\circ}\pm0.09^{\circ}$. We directly cross correlate ACT with Planck and observe generally good agreement but with some discrepancies in TE. All data on which this analysis is based will be publicly released.

中文翻译:

阿塔卡马宇宙学望远镜:测量 98 GHz 和 150 GHz 的宇宙微波背景功率谱

我们展示了阿塔卡马宇宙学望远镜 (ACT) 在 2013-2016 年调查的 5400 deg$^2$ 中测量的 CMB 的温度和偏振角功率谱,其中涵盖了 98 GHz 和 150 GHz 下的 $>$15000 deg$^2$ . 对于此分析,我们采用盲法策略来帮助避免确认偏差,并与此相关,显示在揭盲之前对系统错误进行的大量检查。使用宇宙学分析的可能性,我们限制了各向异性和前景发射的次要来源,并推导出了一个扩展到 $\ell=4000 $ 的“仅 CMB”光谱。在大角度尺度上,150 GHz 的前景发射是我们选定区域内 TT 和 EE 的 $\sim$1%,与普朗克发现的一致。使用相同的可能性,我们单独获得了 ACT 数据的 $\Lambda$CDM 的宇宙学参数,光学深度为 $\tau=0.065\pm0.015$。$\Lambda$CDM 非常适合。最佳拟合模型降低了 $\chi^2$ 为 1.07 (PTE=0.07),$H_0=67.9\pm1.5$ km/s/Mpc。我们表明透镜 BB 信号与 $\Lambda$CDM 一致,并将天体 EB 偏振角限制为 $\psi_P =-0.09^{\circ}\pm0.09^{\circ}$。我们直接将 ACT 与普朗克相互关联,并观察到总体上良好的一致性,但在 TE 中存在一些差异。本分析所依据的所有数据都将公开发布。我们表明透镜 BB 信号与 $\Lambda$CDM 一致,并将天体 EB 偏振角限制为 $\psi_P =-0.09^{\circ}\pm0.09^{\circ}$。我们直接将 ACT 与普朗克相互关联,并观察到总体上良好的一致性,但在 TE 中存在一些差异。本分析所依据的所有数据都将公开发布。我们表明透镜 BB 信号与 $\Lambda$CDM 一致,并将天体 EB 偏振角限制为 $\psi_P =-0.09^{\circ}\pm0.09^{\circ}$。我们直接将 ACT 与普朗克相互关联,并观察到总体上良好的一致性,但在 TE 中存在一些差异。本分析所依据的所有数据都将公开发布。
更新日期:2020-12-30
down
wechat
bug