Continuing Planck Surveyor LPAC Support

持续 Planck Surveyor LPAC 支持

• 批准号: ST/F01239X/1
• 负责人: Andrew Jaffe
• 金额: $ 57.94万
• 依托单位: Imperial College London
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2007
• 资助国家: 英国
• 起止时间: 2007 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FF01239X%2F1
• 关键词: Continuing; Planck; Surveyor; LPAC; Support

The Planck surveyor satellite is due for launch in 2008. It will create all-sky maps over 30-850GHz, allowing observation of galactic synchrotron and free-free emission at low frequencies, galactic dust emission at high frequencies, and emission from extragalactic sources due to these physical processes as well as other sources such as the Sunyaev-Zeldovich effect. Primarily, it will observe the cosmic microwave background (CMB) in both intensity and polarization and allow us to reconstruct the state of the primordial plasma, and thereby measure the underlying cosmological parameters. The task of the Imperial group, the London Planck Analysis Centre (LPAC) is primarily the geometric calibration of Planck/HFI: we determine the layout of the focal plane and the shape of the telescope beam using in situ measurements of planets and more distant point sources. We are also involved in several of the Planck Working Groups responsible for creating the intermediate and final data products: the various point-source catalogues to be shared with Herschel and other instruments, the CMB and foreground maps, and the CMB power spectrum. The case for support has already been reviewed and approved by the UK Herschel-Planck Oversight Committee (HPOC) in September 2006. Subsequent discussions with PPARC/STFC have been held to agree programme details.

普朗克勘测卫星定于2008年发射。它将创建超过30-850GHz的全天地图，允许观测银河系同步加速器和低频自由发射，银河系尘埃发射高频，以及由于这些物理过程以及其他来源（如Sunyaev-Zeldovich效应）而产生的河外源发射。首先，它将观察宇宙微波背景（CMB）的强度和极化，并允许我们重建原始等离子体的状态，从而测量潜在的宇宙参数。帝国集团，伦敦普朗克分析中心（LPAC）的任务主要是对普朗克/HFI进行几何校准：我们通过对行星和更远的点源的原位测量来确定焦平面的布局和望远镜光束的形状。我们还参与了几个普朗克工作组，负责创建中间和最终数据产品：与赫歇尔和其他仪器共享的各种点源目录，CMB和前景图，以及CMB功率谱。英国赫歇尔-普朗克监督委员会（HPOC）已经在2006年9月审查并批准了支持的理由。随后与PPARC/STFC进行了讨论，以商定方案细节。

项目成果

MULTI-WAVELENGTH LENS RECONSTRUCTION OF A PLANCK AND HERSCHEL-DETECTED STAR-BURSTING GALAXY

• DOI: 10.3847/0004-637x/829/1/21
• 发表时间: 2015-12
• 期刊: The Astrophysical Journal
• 作者: N. Timmons;A. Cooray;D. Riechers;H. Nayyeri;H. Fu;E. Jullo;M. Gladders;M. Baes;R. Bussmann;J. Calanog;D. Clements;E. D. Cunha;S. Dye;S. Eales;C. Furlanetto;J. González-Nuevo;J. Greenslade;M. Gurwell;H. Messias;M. Michałowski;I. Oteo;I. P'erez-Fournon;D. Scott;E. Valiante

Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps

• DOI: 10.1088/1475-7516/2018/04/020
• 发表时间: 2016-09
• 期刊: Journal of Cosmology and Astroparticle Physics
• 影响因子: 6.4
• 作者: G. Zotti;J. González-Nuevo;M. López-Caniego;M. Negrello;J. Greenslade;C. Hernandez-Monteagudo;J. Delabrouille;Z. Cai;M. Bonato;A. Achúcarro;P. Ade;R. Allison;M. Ashdown;M. Ballardini;A. Banday;R. Banerji;J. Bartlett;N. Bartolo;S. Basak;M. Bersanelli;M. Biesiada;Maciej Bilicki;A. Bonaldi;J. Borrill;F. Bouchet;F. Boulanger;T. Brinckmann;M. Bucher;C. Burigana;A. Buzzelli;M. Calvo;C. Carvalho;M. Castellano;A. Challinor;J. Chluba;D. Clements;S. Clesse;S. Colafrancesco;I. Colantoni;A. Coppolecchia;M. Crook;G. D’Alessandro;P. Bernardis;G. Gasperis;J. Diego;E. D. Valentino;J. Errard;S. Feeney;R. Fernández-Cobos;S. Ferraro;F. Finelli;F. Forastieri;S. Galli;R. Génova-Santos;M. Gerbino;S. Grandis;S. Hagstotz;S. Hanany;Will Handley;C. Hervías-Caimapo;M. Hills;E. Hivon;K. Kiiveri;T. Kisner;T. Kitching;M. Kunz;H.Kurki-Suonio;G. Lagache;L. Lamagna;A. Lasenby;M. Lattanzi;A. Brun;J. Lesgourgues;A. Lewis;M. Liguori;V. Lindholm;G. Luzzi;B. Maffei;N. Mandolesi;E. Martínez-González;C. Martins;S. Masi;M. Massardi;D. McCarthy;A. Melchiorri;J. Melin;D. Molinari;A. Monfardini;P. Natoli;A. Notari;A. Paiella;D. Paoletti;R. B. Partridge;G. Patanchon;M. Piat;G. Pisano;L. Polastri;G. Polenta;A. Pollo;V. Poulin;M. Quartin;M. Remazeilles;M. Roman;G. Rossi;B. Roukema;J. Rubiño-Martín;L. Salvati;D. Scott;S. Serjeant;A. Tartari;L. Toffolatti;M. Tomasi;N. Trappe;S. Triqueneaux;T. Trombetti;M. Tucci;C. Tucker;J. Valiviita;R. Weygaert;B. Tent;V. Vennin;P. Vielva;N. Vittorio;K. Young;F. T. B. collaboration

Planck Pre-Launch Status: The Planck Mission

• DOI: 10.1051/0004-6361/200912983
• 发表时间: 2010-09
• 期刊: Astronomy and Astrophysics
• 影响因子: 6.5
• 作者: J. Tauber;N. Mandolesi;J. Puget;T. Banos;M. Bersanelli;F. Bouchet;R. C. Butler;J. Charra

Cosmic sculpture: a new way to visualise the cosmic microwave background

宇宙雕塑：一种可视化宇宙微波背景的新方法

• DOI: 10.1088/0143-0807/38/1/015601
• 发表时间: 2017
• 期刊: European Journal of Physics
• 影响因子: 0.7
• 作者: Clements D

An introduction to the Planck mission

• DOI: 10.1080/00107514.2017.1362139
• 发表时间: 2017-07
• 期刊: Contemporary Physics
• 影响因子: 2
• 作者: D. Clements