Continuing Support of Two Astronomical Imagers for Cosmology, Education, and Diverse Other Projects

两台天文成像仪持续支持宇宙学、教育和各种其他项目

• 批准号: 2109035
• 负责人: Antony Stark
• 金额: $ 59.52万
• 依托单位: Smithsonian Institution Astrophysical Observatory
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2021
• 资助国家: 美国
• 起止时间: 2021-10-01 至 2024-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2109035&HistoricalAwards=false
• 关键词: Continuing; Support; Two; Astronomical; Imagers

This project funds the ongoing operation of the Parallel Imager for Southern Cosmology Observations (PISCO), a fast, general-purpose imaging photometer in Chile. The South Pole Telescope (SPT) consortium is conducting the SPT-3G deep millimeter-wave continuum survey, which is detecting thousands of previously unknown galaxy clusters and groups. PISCO observations play a key role in the production of an extensive catalog of galaxy clusters over about 9% of the sky. The resulting searchable public database will include imaging as well as spectroscopy in the optical, infrared, and X-ray, contributing to a wide variety of scientific studies. This project also funds the operation and maintenance of a MicroObservatory telescope for remote STEM education and outreach, operated as part of the Smithsonian Astrophysical Observatory’s Science Education Department Robotic Telescope Network for the online STEM learning community.This program will produce photometric and spectroscopic catalogs of volume-complete samples of galaxy clusters over a 4000 square degree area of sky. After analyzing candidate cluster positions in existing survey data such as DES and VISTA, the SPT team will: (1) make the additional photometric imaging observations needed for completeness in redshift and mass limit, (2) obtain weak lensing measurements during periods of excellent seeing for a representative sub-sample of these clusters, (3) make these evolving data sets available to the astronomical and STEM learning communities in both raw and reduced form, through publications and a web-accessible, searchable archive, and (4) analyze the data for cosmology and the determination of neutrino properties.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

该项目资助南方宇宙学观测并行成像仪（PISCO）的持续运行，这是智利的一种快速通用成像光度计。 南极望远镜 (SPT) 联盟正在进行 SPT-3G 深毫米波连续谱巡天，该任务正在探测数千个以前未知的星系团和星系团。 PISCO 观测在生成覆盖约 9% 天空的广泛星系团目录方面发挥着关键作用。由此产生的可搜索公共数据库将包括光学、红外和 X 射线成像以及光谱学，为广泛的科学研究做出贡献。 该项目还资助用于远程 STEM 教育和推广的微型天文台望远镜的运营和维护，该望远镜作为史密森天体物理天文台科学教育部机器人望远镜网络的一部分，用于在线 STEM 学习社区。该项目将生成 4000 平方度天空区域上星系团体积完整样本的光度和光谱目录。在分析了 DES 和 VISTA 等现有调查数据中的候选星团位置后，SPT 团队将：(1) 进行红移和质量限制完整性所需的额外光度成像观测，(2) 在这些星团的代表性子样本的良好视宁度期间获得弱透镜测量，(3) 通过出版物和出版物，以原始和简化形式向天文学和 STEM 学习社区提供这些不断变化的数据集。 一个可通过网络访问、可搜索的档案，(4) 分析宇宙学数据和确定中微子特性。该奖项反映了 NSF 的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

Redshift Evolution of the Feedback–Cooling Equilibrium in the Core of 48 SPT Galaxy Clusters: A Joint Chandra–SPT–ATCA Analysis

48 个 SPT 星系团核心的反馈的红移演化 - 冷却平衡：钱德拉 - SPT - ATCA 联合分析

• DOI: 10.3847/1538-4357/acc38d
• 发表时间: 2023
• 期刊: The Astrophysical Journal
• 作者: Ruppin, F.;McDonald, M.;Hlavacek-Larrondo, J.;Bayliss, M.;Bleem, L. E.;Calzadilla, M.;Edge, A. C.;Filipović, M. D.;Floyd, B.;Garmire, G.
• 通讯作者: Garmire, G.

The ISM in the z = 6.9 Interacting Galaxies of SPT0311-58

• DOI: 10.3847/1538-4357/acc93a
• 发表时间: 2023-06
• 期刊: The Astrophysical Journal
• 作者: K. Litke;D. Marrone;M. Aravena;M. Archipley;M. Béthermin;James Burgoyne;Jared Cathey;S. Chapman;Anthony H. Gonzalez;T. Greve;G. Gururajan;C. Hayward;M. Malkan;K. Phadke;C. Reuter;K. Rotermund;J. Spilker;A. Stark;N. Sulzenauer;J. Vieira;D. Vizgan;A. Weiss

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck . II. Cross-correlation measurements and cosmological constraints

对暗能量调查第 3 年数据以及 SPT 和普朗克的 CMB 透镜的联合分析。

• DOI: 10.1103/physrevd.107.023530
• 发表时间: 2023
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Chang, C.;Omori, Y.;Baxter, E. J.;Doux, C.;Choi, A.;Pandey, S.;Alarcon, A.;Alves, O.;Amon, A.;Andrade-Oliveira, F.
• 通讯作者: Andrade-Oliveira, F.

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck . III. Combined cosmological constraints

对暗能量调查第 3 年数据以及 SPT 和普朗克的 CMB 透镜的联合分析。

• DOI: 10.1103/physrevd.107.023531
• 发表时间: 2023
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Abbott, T. M. C.;Aguena, M.;Alarcon, A.;Alves, O.;Amon, A.;Andrade-Oliveira, F.;Annis, J.;Ansarinejad, B.;Avila, S.;Bacon, D.
• 通讯作者: Bacon, D.

Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future

利用 CMB 星团透镜数据改善星系团数量计数的宇宙学约束：SPT-SZ 巡天结果和未来预测

• DOI: 10.3847/1538-4357/ac6a55
• 发表时间: 2022
• 期刊: The Astrophysical Journal
• 作者: Chaubal, P. S.;Reichardt, C. L.;Gupta, N.;Ansarinejad, B.;Aylor, K.;Balkenhol, L.;Baxter, E. J.;Bianchini, F.;Benson, B. A.;Bleem, L. E.
• 通讯作者: Bleem, L. E.