KiDS-i-800: comparing weak gravitational lensing measurements from same-sky surveys

被引:24
作者
Amon, A. [1 ]
Heymans, C. [1 ]
Klaes, D. [2 ]
Erben, T. [2 ]
Blake, C. [3 ]
Hildebrandt, H. [2 ]
Hoekstra, H. [4 ]
Kuijken, K. [4 ]
Miller, L. [5 ]
Morrison, C. B. [6 ]
Choi, A. [7 ]
de Jong, J. T. A. [4 ,8 ]
Glazebrook, K. [3 ]
Irisarri, N. [4 ]
Joachimi, B. [9 ]
Joudaki, S. [5 ]
Kannawadi, A. [4 ]
Lidman, C. [10 ]
Napolitano, N. [11 ]
Parkinson, D. [12 ]
Schneider, P. [2 ]
van Uitert, E. [9 ]
Viola, M. [4 ]
Wolf, C. [13 ]
机构
[1] Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[2] Argelander Inst Astronomie, Auf hugel 71, D-53121 Bonn, Germany
[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, POB 218, Hawthorn, Vic 3122, Australia
[4] Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands
[5] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
[6] Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA
[7] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA
[8] Univ Groningen, Kapteyn Astron Inst, NL-9700 AD Groningen, Netherlands
[9] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[10] Australian Astron Observ, POB 915, N Ryde, NSW 1670, Australia
[11] Osserv Astron Capodimonte, INAF, Via Moiariello 16, I-80131 Naples, Italy
[12] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia
[13] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia
基金
澳大利亚研究理事会; 欧洲研究理事会; 美国国家科学基金会;
关键词
gravitational lensing: weak; surveys; galaxies: photometry; cosmology: observations; COSMIC SHEAR; REDSHIFT DISTRIBUTIONS; PHOTOMETRIC REDSHIFTS; CROSS-CORRELATIONS; GALAXY; CFHTLENS; CONSTRAINTS; COSMOLOGY; PROGRAM; CATALOG;
D O I
10.1093/mnras/sty859
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a weak gravitational lensing analysis of 815 deg(2) of i-band imaging from the Kilo-Degree Survey (KiDS-i-800). In contrast to the deep r-band observations, which take priority during excellent seeing conditions and form the primary KiDS data set (KiDS-r-450), the complementary yet shallower KiDS-i-800 spans a wide range of observing conditions. The overlapping KiDS-i-800 and KiDS-r-450 imaging therefore provides a unique opportunity to assess the robustness of weak lensing measurements. In our analysis we introduce two new 'null' tests. The 'nulled' two-point shear correlation function uses a matched catalogue to show that the calibrated KiDS-i-800 and KiDS-r-450 shear measurements agree at the level of 1 +/- 4 per cent. We use five galaxy lens samples to determine a 'nulled' galaxy-galaxy lensing signal from the full KiDS-i-800 and KiDS-r-450 surveys and find that the measurements agree to 7 +/- 5 per cent when the KiDS-i-800 source redshift distribution is calibrated using either spectroscopic redshifts, or the 30-band photometric redshifts from the COSMOS survey.
引用
收藏
页码:4285 / 4307
页数:23
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