《欧洲南方天文台成为切伦科夫望远镜阵列天文台的股东》

  • 来源专题:重大科技基础设施领域知识集成服务平台
  • 编译者: 魏韧
  • 发布时间:2019-11-08
  • 在以观察员身份参与切伦科夫望远镜阵列(CTA)天文台项目一段时间后,3月7日,欧洲南方天文台今天正式成为其股东。切伦科夫望远镜阵列理事会在欧洲南方天文台总部会议上履行了正式手续。切伦科夫望远镜阵列是下一代地基天文台,设计用于探测高能伽马射线,由位于南北半球的118个望远镜组成。

    2018年12月19日,欧洲南方天文台已签署协议,在智利欧洲南方天文台 Paranal天文台附近的阿塔卡马沙漠进行切伦科夫望远镜阵列的南半球选址。凭借良好的观测条件和完善的基础设施,Paranal成在南半球部署切伦科夫望远镜阵列等新设施的极佳地点。切伦科夫望远镜阵列的北半球选址为加那利群岛的拉帕尔马。

    作为股东,欧洲南方天文台将在切伦科夫望远镜阵列理事会设置代表处,管理天文台,吸纳来自11个国家的股东和来自另外两个国家的准成员。参与国目前正在建立切伦科夫望远镜阵列天文台欧洲研究基础设施联盟,负责建造、委托和运营这座巨大的天文台。

    切伦科夫望远镜阵列是一个大型国际项目,得益于来自五大洲的1400多名科学家和工程师的投入。它将是世界上最大的高能伽马射线观测站,在伽马射线谱段具有独特的灵敏度,旨在探测一些极端环境,包括脉冲星和超新星残骸等伽马射线源,将有助于加深对相对论宇宙粒子起源和作用的理解。

  • 原文来源:https://www.eso.org/public/announcements/ann19013/
相关报告
  • 《欧洲南方天文台搜寻类地行星的望远镜初光》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2018-12-06
    • Four telescopes devoted to the search for habitable planets around nearby ultra-cool stars get off to a successful start at ESO’s Paranal Observatory The SPECULOOS Southern Observatory (SSO) has been successfully installed at the Paranal Observatory and has obtained its first engineering and calibration images — a process known as first light. After finishing this commissioning phase, this new array of planet-hunting telescopes will begin scientific operations, starting in earnest in January 2019. SSO is the core facility of a new exoplanet-hunting project called Search for habitable Planets EClipsing ULtra-cOOl Stars (SPECULOOS) [1], and consists of four telescopes equipped with 1-metre primary mirrors. The telescopes — named Io, Europa, Ganymede and Callisto after the four Galilean moons of Jupiter — will enjoy pristine observing conditions at the Paranal site, which is also home to ESO’s flagship Very Large Telescope (VLT). Paranal provides a near-perfect site for astronomy, with dark skies and a stable, arid climate. These telescopes have a momentous task — SPECULOOS aims to search for potentially habitable Earth-sized planets surrounding ultra-cool stars or brown dwarfs, whose planetary populations are still mostly unexplored. Only a few exoplanets have been found orbiting such stars, and even fewer lie within their parent star’s habitable zone. Even though these dim stars are hard to observe, they are abundant — comprising about 15% of the stars in the nearby universe. SPECULOOS is designed to explore 1000 such stars, including the nearest, brightest, and smallest, in search of Earth-sized habitable planets. “SPECULOOS gives us an unprecedented ability to detect terrestrial planets eclipsing some of our smallest and coolest neighbouring stars,” elaborated Michaël Gillon of the University of Liège, principal investigator of the SPECULOOS project. “This is a unique opportunity to uncover the details of these nearby worlds.” SPECULOOS will search for exoplanets using the transit method [2], following the example of its prototype TRAPPIST-South telescope at ESO’s La Silla Observatory. That telescope has been operational since 2011 and detected the famous TRAPPIST-1 planetary system. As a planet passes in front of its star it blocks some of the star’s light — essentially causing a small partial eclipse — resulting in a subtle but detectable dimming of the star. Exoplanets with smaller host stars block more of their star’s light during a transit, making these periodic eclipses much easier to detect than those associated with larger stars. Thus far, only a small fraction of the exoplanets detected by this method have been Earth-sized or smaller. However, the small size of the SPECULOOS target stars combined with the high sensitivity of its telescopes allows detection of Earth-sized transiting planets located in the habitable zone. These planets will be ideally suited for follow-up observations with large ground- or space-based facilities. “The telescopes are kitted out with cameras that are highly sensitive in the near-infrared,” explained Laetitia Delrez of the Cavendish Laboratory, Cambridge, a co-investigator in the SPECULOOS team. “This radiation is a little beyond what human eyes can detect, and is the primary emission from the dim stars SPECULOOS will be targeting.” The telescopes and their brightly coloured mounts were built by the German company ASTELCO and are protected by domes made by the Italian manufacturer Gambato. The project will receive support from the two TRAPPIST 60-cm telescopes, one at ESO’s La Silla Observatory and the other in Morocco [3]. The project will in due course also include the SPECULOOS Northern Observatory and SAINT-Ex, which are currently under construction in Tenerife, Spain, and at San Pedro Mártir, Mexico, respectively. There is also potential for an exciting future collaboration with the Extremely Large Telescope (ELT), ESO’s future flagship telescope, currently under construction on Cerro Armazones. The ELT will be able to observe planets detected by SPECULOOS in unprecedented detail — perhaps even analysing their atmospheres. “These new telescopes will allow us to investigate nearby Earth-like worlds in the Universe in greater detail than we could have imagined only ten years ago,” concluded Gillon. “These are tremendously exciting times for exoplanet science.” Notes [1] Speculoos, or speculaas, is a delicious type of spiced biscuit traditionally baked in Belgium and other countries for Saint Nicholas's day on December 6. The name, with its sweet connotations, reflects the Belgian origins of the SPECULOOS project. The TRAPPIST project also has a similar Belgian namesake — it was named after Trappist beers, most of which are brewed in Belgium. [2] The transit method is one of several ways exoplanets are discovered. A variety of instruments, including ESO’s planet-hunting HARPS spectrograph at the La Silla Observatory, use the radial velocity method to detect exoplanets, measuring changes in a star’s velocity due to an orbiting exoplanet. [3] SSO also received funding from the European Research Council under the European Union's Seventh Framework Programme (FP7/2007-2013)/ ERC grant agreement number 336480, from the Simons and MERAC Foundations, and from private sponsors. More information ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It has 16 Member States: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile and with Australia as a Strategic Partner. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its world-leading Very Large Telescope Interferometer as well as two survey telescopes, VISTA working in the infrared and the visible-light VLT Survey Telescope. ESO is also a major partner in two facilities on Chajnantor, APEX and ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre Extremely Large Telescope, the ELT, which will become “the world’s biggest eye on the sky”. The SPECULOOS Southern Observatory (SSO) is a project conducted by the University of Liège (Belgium), the Cavendish Laboratory, Cambridge (UK) and the King Abdulaziz University (Saudi Arabia), under the leadership of Michaël Gillon, research scientist and head of the group EXOplanets in Transit: Identification and Characterization (EXOTIC) at the Department of Astrophysics, Geophysics and Oceanography (AGO) of the University of Liège. SSO also involves scientists from the Universities of Bern, Birmingham, and Warwick. ESO supports SSO and hosts it at the Paranal Observatory in the Chilean Atacama Desert.
  • 《欧洲南方天文台决定建设39米极大望远镜主镜全部子镜》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2017-12-15
    • ESO’s governing body, the Council, has just authorised additional spending to cover the cost of both the five inner rings of segments for the main mirror (M1) of the Extremely Large Telescope (ELT), and one spare set of 133 mirror segments (one sixth of the total M1), and also an additional mirror segment maintenance unit. The decision was made at the recent meeting of the Council in Garching, Germany, after the positive recommendation by the ESO Finance Committee and made possible by an improved funding scenario. The ELT is a revolutionary ground-based telescope concept which will have a 39-metre main mirror made of 798 hexagonal segments. It will be the largest optical telescope in the world: “the world’s biggest eye on the sky”. First light for the ELT is targeted for 2024. Up to now the inner five rings of segments of the ELT primary mirror were in Phase 2 of the project, and had not yet been funded. This second phase also included a mirror segment washing, stripping and coating plant that was needed to keep the mirror at its full performance, as well as a spare set of 133 mirror segments [1]. These parts of the telescope’s Phase 2 have now received the green light. Construction of the telescope is proceeding rapidly and nearly 90% of the contracts for Phase 1, by value, are already awarded.