Operation of the HAWC Gamma-Ray Observatory

HAWC 伽马射线天文台的运行

• 批准号: 1308127
• 负责人: Jordan Goodman
• 金额: $ 310.77万
• 依托单位: University of Maryland, College Park
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2013
• 资助国家: 美国
• 起止时间: 2013-09-01 至 2019-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1308127&HistoricalAwards=false
• 关键词: Operation; HAWC; Gamma; Ray; Observatory

The High Altitude Water Cherenkov (HAWC) Gamma-ray Observatory is a wide field-of-view, continuously operating, teraelectronvolt (TeV) gamma-ray telescope that will explore the origin of cosmic rays, study the acceleration of particles in extreme physical environments, and search for new TeV physics. HAWC is under construction at an elevation of 4100 meters above sea level in Mexico by a collaboration of US and Mexican institutions. This award will fund operations that will begin in August 2013 even while construction is being completed. At the beginning of operations HAWC, with 100 Water Cherenkov Detectors, will be the most sensitive wide-field detector in the TeV range. During the first year of operation, HAWC's sensitivity will steadily increase as more detectors are brought online. When completed in the Fall of 2014 HAWC will consist of an array of the 250-300 detectors and will be more than an order of magnitude more sensitive than its predecessors. HAWC will monitor the northern sky and make coincident observations with other observatories including VERITAS, HESS, Magic, IceCube and the Fermi Gamma-ray Space Telescope for multi-wavelength and multi-messenger studies of the high-energy sky. HAWC will observe Galactic sources in the TeV energy range, detect diffuse emission from regions of the Galactic plane, observe known TeV active galactic nuclei and the brightest known gigaelectronvolt (GeV) gamma-ray bursts, and with its significant increase in sensitivity it is poised to discover new high-energy phenomena in the Universe.Broader Impacts: HAWC is an all-sky instrument that will serve as a TeV 'finder' telescope for ground-based observatories, and it can be used to extend measurements of satellite-discovered sources to TeV energies. HAWC will build on the strong outreach record of Milagro to bring the high-energy astrophysics field to students and the general public. Since HAWC is a joint Mexican-American project, it presents an opportunity to attract Hispanic-American students to science and to particle astrophysics.

高空水切伦科夫（HAWC）伽马射线天文台是一个宽视场、连续运行的太电子伏（TeV）伽马射线望远镜，将探索宇宙射线的起源，研究极端物理环境中粒子的加速，并搜索新的 TeV 物理。 HAWC 正在墨西哥海拔 4100 米处由美国和墨西哥机构合作建造。 该奖项将为 2013 年 8 月开始的运营提供资金，即使施工正在进行中。 在运行初期，配备 100 个水切伦科夫探测器的 HAWC 将成为 TeV 范围内最灵敏的宽视场探测器。 在运行的第一年，随着更多探测器上线，HAWC 的灵敏度将稳步提高。 2014 年秋季完工后，HAWC 将由 250-300 个探测器组成的阵列组成，其灵敏度将比其前身高出一个数量级以上。 HAWC 将监测北方天空，并与 VERITAS、HESS、Magic、IceCube 和费米伽马射线太空望远镜等其他天文台进行同步观测，对高能天空进行多波长和多信使研究。 HAWC 将观测 TeV 能量范围内的银河源，探测银河平面区域的漫射发射，观测已知的 TeV 活动星系核和已知最亮的吉电子伏 (GeV) 伽马射线爆发，并且随着灵敏度的显着提高，它已准备就绪发现宇宙中新的高能现象。 更广泛的影响：HAWC 是一种全天空仪器，将作为地面天文台的 TeV“发现者”望远镜，它可以可用于将卫星发现的源的测量扩展到 TeV 能量。 HAWC 将在 Milagro 强大的外展记录的基础上，将高能天体物理领域带给学生和公众。 由于 HAWC 是一个墨西哥裔美国人联合项目，它提供了一个吸引西班牙裔美国学生学习科学和粒子天体物理学的机会。

项目成果

HAWC Search for High-mass Microquasars

• DOI: 10.3847/2041-8213/abf35a
• 发表时间: 2021-01
• 期刊: The Astrophysical Journal Letters
• 作者: A. Albert;R. Alfaro;C. Álvarez;J. Angeles Camacho;J. C. Arteaga-Velázquez;K. Arunbabu;D. Avila Rojas-D.-Avila