Dark Energy Survey: Y1 Observing Shift

暗能量调查：Y1 观测转变

• 批准号: ST/L006529/1
• 负责人: Anita Romer
• 金额: $ 0.25万
• 依托单位: University of Sussex
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2014
• 资助国家: 英国
• 起止时间: 2014 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FL006529%2F1
• 关键词: Dark; Energy; Survey; Y1; Observing

The following is taken from the abstract of the attached observing proposal: The Nobel Prize in Physics for 2011 was awarded for the discovery of the accelerating expansion of the Universe. The primary scientic objective of the Dark Energy Survey (DES) is to address the question: why is the expansion of the Universe speeding up? Is cosmic acceleration due to dark energy or does it require a modication of General Relativity? If dark energy, is it the energy density of the vacuum (Einstein's cosmological constant) or something else? DES will address these questions by measuring the properties of dark energy with unprecedented precision, using four complementary techniques: galaxy clusters, large-scale galaxy clustering (including baryon acoustic oscillations), weak gravitational lensing, and type Ia supernovae. To achieve the requisite precision, we will conduct two optimally interleaved surveys over 525 nights: a wide-area grizY survey covering 5000 sq. deg. to 24th mag and a deeper time-domain griz survey with 5-day cadence covering 30 sq. deg. In response to an NOAO AO in 2003, the DES collaboration was formed and has built the Dark Energy Camera (DECam), a 570-megapixel, red-sensitive imager with 2.2 degree field of view, five uniform, high-throughput filters, a five-element optical corrector, and a hexapod system for active focus and alignment. We have constructed and will operate a data management system to process and serve DES survey data and a Community Pipeline for NOAO to process community data. The DES data products will provide a rich legacy for the astronomy community, and DECam will be an extraordinary asset as a facility instrument on the Blanco Telescope.

2011年诺贝尔物理学奖授予发现宇宙加速膨胀的科学家。暗能量调查（DES）的主要科学目标是解决这个问题：为什么宇宙膨胀加速？宇宙加速是由于暗能量还是需要广义相对论的修正？如果是暗能量，它是真空的能量密度（爱因斯坦的宇宙常数）还是别的什么？DES将通过使用四种互补技术以前所未有的精度测量暗能量的性质来解决这些问题：星系团，大规模星系团（包括重子声振荡），弱引力透镜和Ia型超新星。为了达到必要的精度，我们将在525个夜晚进行两次最佳交错调查：一次是覆盖5000平方米的广域格利兹调查。°的到24日mag和更深的时域griz调查，5天的节奏，覆盖30平方米。°的为了响应2003年的NOAO AO AO，DES合作成立，并建造了暗能量相机（DECam），这是一个5.7亿像素的红敏成像器，具有2.2度视场，五个均匀的高通量滤光片，五元件光学校正器和一个用于主动聚焦和对准的六足系统。我们已经建立并将运行一个数据管理系统来处理和服务DES调查数据，并为NOAO处理社区数据提供社区管道。DES数据产品将为天文学界提供丰富的遗产，而DECam作为布兰科望远镜上的设施仪器将是一项非凡的资产。

项目成果

VizieR Online Data Catalog: The Dark Energy Survey (DES): Data Release 2 (Abbott+, 2021)

VizieR 在线数据目录：暗能量调查 (DES)：数据发布 2（Abbott，2021 年）

• 发表时间: 2022
• 期刊: VizieR Online Data Catalog
• 作者: Abbott T. M. C.

Discovery of two gravitationally lensed quasars in the Dark Energy Survey

• DOI: 10.1093/mnras/stv2171
• 发表时间: 2015-08
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: A. Agnello;T. Treu;F. Ostrovski;P. Schechter;E. Buckley-Geer;Huan Lin;M. Auger;F. Courbin;C. Fassnacht;J. Frieman;N. Kuropatkin;P. Marshall;R. McMahon;G. Meylan;A. More;S. Suyu;C. Rusu;D. Finley;T. Abbott;F. Abdalla;S. Allam;J. Annis;M. Banerji;A. Benoit-Lévy;E. Bertin;D. Brooks;D. Burke;A. Rosell;M. Kind;J. Carretero;C. Cunha;C. D'Andrea;L. Costa;S. Desai;H. Diehl;J. Dietrich;P. Doel;T. Eifler;J. Estrada;A. F. Neto;B. Flaugher;P. Fosalba;D. Gerdes;D. Gruen;G. Gutiérrez;K. Honscheid;D. James;K. Kuehn;O. Lahav;M. Lima;M. Maia;M. March;J. Marshall;P. Martini;Peter Melchior;C. Miller;R. Miquel;R. Nichol;R. Ogando;A. Plazas;K. Reil;A. Romer;A. Roodman;M. Sako;E. Sánchez;B. Santiago;V. Scarpine;M. Schubnell;I. Sevilla-Noarbe;R. C. Smith;M. Soares-Santos;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;J. Thaler;D. Tucker;A. Walker;Risa Wechsler;Yuanyuan Zhang

Cosmology from cosmic shear with Dark Energy Survey science verification data

• DOI: 10.1103/physrevd.94.022001
• 发表时间: 2015-07
• 期刊: Physical Review D
• 影响因子: 5
• 作者: The Dark Energy Survey Collaboration;T. Abbott;F. Abdalla;S. Allam;A. Amara;J. Annis;R. Armstrong;D. Bacon;M. Banerji;A. Bauer;E. Baxter;M. Becker;A. Benoit-Lévy;R. Bernstein;G. Bernstein;E. Bertin;J. Blazek;C. Bonnett;S. Bridle;D. Brooks;C. Bruderer;E. Buckley-Geer;D. Burke;M. Busha;D. Capozzi;A. Rosell;M. Kind;J. Carretero;F. Castander;C. Chang;J. Clampitt;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;R. Das;D. Depoy;S. Desai;H. Diehl;J. Dietrich;S. Dodelson;P. Doel;A. Drlica-Wagner;G. Efstathiou;T. Eifler;B. Erickson;J. Estrada;A. Evrard;A. F. Neto;E. Fernandez;D. Finley;B. Flaugher;P. Fosalba;O. Friedrich;J. Frieman;C. Gangkofner;J. García-Bellido;E. Gaztañaga;D. Gerdes;D. Gruen;R. Gruendl;G. Gutiérrez;W. Hartley;M. Hirsch;K. Honscheid;E. Huff;B. Jain;D. James;M. Jarvis;T. Kacprzak;S. Kent;D. Kirk;E. Krause;A. Kravtsov;K. Kuehn;N. Kuropatkin;J. Kwan;O. Lahav;B. Leistedt;T. Li;M. Lima;H. Lin;N. MacCrann;M. March;J. Marshall;P. Martini;R. McMahon;Peter Melchior;C. Miller;R. Miquel;J. Mohr;E. Neilsen;R. Nichol;A. Nicola;B. Nord;R. Ogando;A. Palmese;H. Peiris;A. Plazas;A. Réfrégier;N. Roe;A. Romer;A. Roodman;B. Rowe;E. Rykoff;C. Sabiu;I. Sadeh;M. Sako;S. Samuroff;C. S'anchez;E. Sánchez;H. Seo;I. Sevilla-Noarbe;E. Sheldon;R. C. Smith;M. Soares-Santos;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;J. Thaler;D. Thomas;M. Troxel;V. Vikram;A. Walker;R. Wechsler;J. Weller;Y. Zhang;J. Zuntz

Models of the Strongly Lensed Quasar DES J0408-5354

• DOI: 10.1093/mnras/stx2242
• 发表时间: 2017-02
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: A. Agnello;Huan Lin;L. Buckley-Geer;T. Treu;V. Bonvin;F. Courbin;C. Lemon;T. Morishita;A. Amara;M. Auger;S. Birrer;J. Chan;T. Collett;A. More;C. Fassnacht;J. Frieman;P. Marshall;R. McMahon;G. Meylan;S. Suyu;F.Castander;D. Finley;A.Howell;C. Kochanek;M. Makler;P. Martini;N. Morgan;B.Nord;F. Ostrovski;P. Schechter;D. Tucker;Risa Wechsler;T. Abbott;F. Abdalla;S. Allam;A. Benoit-Lévy;E. Bertin;D. Brooks;D. Burke;A. Rosell;M. Kind;J. Carretero;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;S. Desa;J. Dietrich;T. Eifler;B. Flaugher;P. Fosalba;J. Garc'ia-Bellido;E. Gaztañaga;D. Goldstein;D. Gruen;R. Gruendl;J. Gschwend;G. Gutiérrez;K. Honscheid;D. James;K. Kuehn;N. Kuropatkin;T. Li;M. Lima;M. Maia;M. March;J. Marshall;Peter Melchior;F. Menanteau;R. Miquel;R. Ogando;A. Plazas;A. Romer;E. Sánchez;R. Schindler;M. Schubnell;I. Sevilla-Noarbe;M. Smith;R. C. Smith;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;D. Thomas;A. Walker

Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions

• DOI: 10.1103/physrevd.100.023541
• 发表时间: 2018-10
• 期刊: Physical Review D
• 影响因子: 5
• 作者: T. Abbott;F. Abdalla;A. Alarcon;S. Allam;J. Annis;S. Ávila;K. Aylor;M. Banerji;N. Banik;E. Baxter;K. Bechtol;M. Becker;B. Benson;G. Bernstein;E. Bertin;F. Bianchini;J. Blazek;L. Bleem;L. Bleem;S. Bridle;D. Brooks;E. Buckley-Geer;D. Burke;J. Carlstrom;A. Rosell;M. Kind;J. Carretero;F. Castander;R. Cawthon;C. Chang;C. Chang;H.-M. Cho;A. Choi;R. Chown;T. Crawford;A. Crites;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;C. Davis;T. Haan;J. DeRose;S. Desai;J. Vicente;H. Diehl;J. Dietrich;M. Dobbs;S. Dodelson;P. Doel;A. Drlica-Wagner;T. Eifler;J. Elvin-Poole;W. Everett;B. Flaugher;P. Fosalba;O. Friedrich;J. Frieman;J. García-Bellido;M. Gatti;E. Gaztañaga;E. George;D. Gerdes;T. Giannantonio;D. Gruen;R. Gruendl;J. Gschwend;G. Gutiérrez;N. Halverson;N. Harrington;W. Hartley;G. Holder;D. Hollowood;W. Holzapfel;K. Honscheid;Z. Hou;B. Hoyle;J. Hrubeš;D. Huterer;B. Jain;D. James;M. Jarvis;T. Jeltema;M. Johnson;Michael D. Johnson;S. Kent;D. Kirk;L. Knox;N. Kokron;E. Krause;K. Kuehn;O. Lahav;Adrian T. Lee;E. Leitch;Tian Li;M. Lima;Huan Lin;D. Luong-Van;N. MacCrann;M. Maia;A. Manzotti;D. Marrone;J. Marshall;P. Martini;J. McMahon;F. Menanteau;S. Meyer;R. Miquel;L. Mocanu;J. J. Mohr-J.;J. Muir;T. Natoli;A. Nicola;B. Nord;Y. Omori;S. Padin;S. Pandey;A. Plazas;A. Porredon;J. Prat;C. Pryke;M. Rau;C. Reichardt;R. Rollins;A. Romer;A. Roodman;A. Ross;E. Rozo;J. Ruhl;E. Rykoff;S. Samuroff;C. Sánchez;E. Sánchez;J. Sayre;V. Scarpine;K. Schaffer;L. Secco;S. Serrano;I. Sevilla-Noarbe;E. Sheldon;E. Shirokoff;G. Simard;M. Smith;M. Soares-Santos;F. Sobreira;Z. Staniszewski;A. Stark;K. Story;E. Suchyta;M. Swanson;G. Tarlé;D. Thomas;M. Troxel;D. Tucker;K. Vanderlinde;J. Vieira;P. Vielzeuf;V. Vikram;A. Walker;Risa Wechsler;J. Weller;R. Williamson;W. L. K. Wu;B. Yanny;O. Zahn;Yuanyuan Zhang;J. Zuntz