Dark energy survey year 3 results: weak lensing shape catalogue
Dark energy survey year 3 results: weak lensing shape catalogue
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暗能量调查第三年结果：弱透镜形状目录
DOI：
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发表时间：
2020
影响因子：
4.8
通讯作者：
R. Wilkinson
中科院分区：
文献类型：
--
作者：
M. Gatti;E. Sheldon;A. Amon;M. Becker;M. Troxel;A. Choi;C. Doux;N. MacCrann;A. Navarro;I. Harrison;D. Gruen;G. Bernstein;M. Jarvis;L. Secco;A. Ferté;T. Shin;J. McCullough;R. Rollins;R. Chen;C. Chang;S. Pandey;I. Tutusaus;J. Prat;J. Elvin;C. Sánchez;A. Plazas;A. Roodman;J. Zuntz;T. Abbott;M. Aguena;S. Allam;J. Annis;S. Ávila;D. Bacon;E. Bertin;S. Bhargava;D. Brooks;D. Burke;A. Rosell;M. Kind;J. Carretero;F. Castander;C. Conselice;M. Costanzi;M. Crocce;L. Costa;T. Davis;J. Vicente;S. Desai;H. Diehl;J. Dietrich;P. Doel;A. Drlica;K. Eckert;S. Everett;I. Ferrero;J. Frieman;J. García;D. Gerdes;T. Giannantonio;R. Gruendl;J. Gschwend;G. Gutiérrez;W. Hartley;S. Hinton;D. Hollowood;K. Honscheid;B. Hoyle;E. Huff;D. Huterer;B. Jain;D. James;T. Jeltema;E. Krause;R. Kron;N. Kuropatkin;M. Lima;M. Maia;J. Marshall;R. Miquel;R. Morgan;J. Myles;A. Palmese;F. Paz;E. Rykoff;S. Samuroff;E. Sánchez;V. Scarpine;M. Schubnell;S. Serrano;I. Sevilla;M. Smith;M. Soares;E. Suchyta;M. Swanson;G. Tarlé;D. Thomas;C. To;D. Tucker;T. Varga;Risa Wechsler;J. Weller;W. Wester;R. Wilkinson
我们提出和表征的星系形状目录从第一个3年的暗能量调查（DES）的观测，在南部天空的4143 deg2的有效区域。我们描述了我们的数据分析过程和我们的自校准剪切测量管道元校准，它建立并改进了DES第1年分析中使用的管道在几个方面。DES第三年弱透镜形状星表由100 204 026个星系组成，在riz波段测量，得到加权源数密度neff = 5.59 gal arcmin−2，相应的形状噪声σe = 0.261。我们进行了电池的内部零测试的目录，包括测试系统学相关的点扩散函数（PSF）建模，虚假目录B模式信号，目录污染，和星系的属性。
We present and characterize the galaxy shape catalogue from the first 3 yr of Dark Energy Survey (DES) observations, over an effective area of 4143 deg2 of the southern sky. We describe our data analysis process and our self-calibrating shear measurement pipeline metacalibration, which builds and improves upon the pipeline used in the DES Year 1 analysis in several aspects. The DES Year 3 weak-lensing shape catalogue consists of 100 204 026 galaxies, measured in the riz bands, resulting in a weighted source number density of neff = 5.59 gal arcmin−2 and corresponding shape noise σe = 0.261. We perform a battery of internal null tests on the catalogue, including tests on systematics related to the point spread function (PSF) modelling, spurious catalogue B-mode signals, catalogue contamination, and galaxy properties.
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影响因子：
4.8
作者：
M. Jarvis;G. Bernstein;A. Amon;C. Davis;P. L'eget;K. Bechtol;I. Harrison;M. Gatti;A. Roodman
通讯作者：
M. Jarvis;G. Bernstein;A. Amon;C. Davis;P. L'eget;K. Bechtol;I. Harrison;M. Gatti;A. Roodman
影响因子：
4.8
作者：
H. Hildebrandt;M. Viola;C. Heymans;S. Joudaki;K. Kuijken;C. Blake;T. Erben;B. Joachimi;D. Klaes
通讯作者：
H. Hildebrandt;M. Viola;C. Heymans;S. Joudaki;K. Kuijken;C. Blake;T. Erben;B. Joachimi;D. Klaes
CFHTLenS：加拿大、法国、夏威夷望远镜透镜调查 成像数据和目录产品
DOI：
10.1111/j.1365-2966.2012.21952.x
发表时间：
2012
影响因子：
4.8
作者：
C. Heymans
通讯作者：
C. Heymans
影响因子：
4.8
作者：
T. McClintock;T. Varga;D. Gruen;E. Rozo;E. Rykoff;T. Shin;Peter Melchior;J. DeRose;S. Seitz;J. Dietrich;E. Sheldon;Y. Zhang;A. V. D. Linden;T. Jeltema;A. Mantz;A. Romer;S. Allen;M. Becker;A. Bermeo;S. Bhargava;M. Costanzi;S. Everett;A. Farahi;N. Hamaus;W. Hartley;D. Hollowood;B. Hoyle;H. Israel;P. Li;N. MacCrann;G. Morris;A. Palmese;A. Plazas;G. Pollina;M. Rau;M. Simet;M. Soares-Santos;M. Troxel;C. Cervantes;Risa Wechsler;J. Zuntz;T. Abbott;F. Abdalla;S. Allam;J. Annis;S. Ávila;S. Bridle;D. Brooks;D. Burke;A. Rosell;M. Kind;J. Carretero;F. Castander;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;C. Davis;J. Vicente;H. Diehl;P. Doel;A. Drlica-Wagner;A. Evrard;B. Flaugher;P. Fosalba;J. Frieman;J. Garc'ia-Bellido;E. Gaztañaga;D. Gerdes;T. Giannantonio;R. Gruendl;G. Gutiérrez;K. Honscheid;D. James;D. Kirk;E. Krause;K. Kuehn;O. Lahav;T. Li;M. Lima;M. March;J. Marshall;F. Menanteau;R. Miquel;J. Mohr;B. Nord;R. Ogando;A. Roodman;E. Sánchez;V. Scarpine;R. Schindler;I. Sevilla-Noarbe;M. Smith;R. C. Smith;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;D. Tucker;V. Vikram;A. Walker;J. Weller
通讯作者：
T. McClintock;T. Varga;D. Gruen;E. Rozo;E. Rykoff;T. Shin;Peter Melchior;J. DeRose;S. Seitz;J. Dietrich;E. Sheldon;Y. Zhang;A. V. D. Linden;T. Jeltema;A. Mantz;A. Romer;S. Allen;M. Becker;A. Bermeo;S. Bhargava;M. Costanzi;S. Everett;A. Farahi;N. Hamaus;W. Hartley;D. Hollowood;B. Hoyle;H. Israel;P. Li;N. MacCrann;G. Morris;A. Palmese;A. Plazas;G. Pollina;M. Rau;M. Simet;M. Soares-Santos;M. Troxel;C. Cervantes;Risa Wechsler;J. Zuntz;T. Abbott;F. Abdalla;S. Allam;J. Annis;S. Ávila;S. Bridle;D. Brooks;D. Burke;A. Rosell;M. Kind;J. Carretero;F. Castander;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;C. Davis;J. Vicente;H. Diehl;P. Doel;A. Drlica-Wagner;A. Evrard;B. Flaugher;P. Fosalba;J. Frieman;J. Garc'ia-Bellido;E. Gaztañaga;D. Gerdes;T. Giannantonio;R. Gruendl;G. Gutiérrez;K. Honscheid;D. James;D. Kirk;E. Krause;K. Kuehn;O. Lahav;T. Li;M. Lima;M. March;J. Marshall;F. Menanteau;R. Miquel;J. Mohr;B. Nord;R. Ogando;A. Roodman;E. Sánchez;V. Scarpine;R. Schindler;I. Sevilla-Noarbe;M. Smith;R. C. Smith;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;D. Tucker;V. Vikram;A. Walker;J. Weller
DOI：
10.1111/j.1365-2966.2006.10198.x
发表时间：
2006-05-21
影响因子：
4.8
作者：
Heymans, C;Van Waerbeke, L;Wittman, D
通讯作者：
Wittman, D