Galaxy-galaxy lensing in the Dark Energy Survey Science Verification data

被引：40

作者：

Clampitt, J. ^{[1
]}

Sanchez, C. ^{[2
]}

Kwan, J. ^{[1
]}

Krause, E. ^{[3
]}

MacCrann, N. ^{[4
]}

Park, Y. ^{[5
,6
]}

Troxel, M. A. ^{[4
]}

Jain, B. ^{[1
]}

Rozo, E. ^{[5
]}

Rykoff, E. S. ^{[3
,7
]}

Wechsler, R. H. ^{[3
,7
,8
]}

Blazek, J. ^{[9
]}

Bonnett, C. ^{[2
]}

Crocce, M. ^{[10
]}

Fang, Y. ^{[1
]}

Gaztanaga, E. ^{[10
]}

Gruen, D. ^{[3
,7
]}

Jarvis, M. ^{[1
]}

Miquel, R. ^{[2
]}

Prat, J. ^{[2
]}

Ross, A. J. ^{[9
]}

Sheldon, E. ^{[11
]}

Zuntz, J. ^{[4
]}

Abbott, T. M. C. ^{[12
]}

Abdalla, F. B. ^{[13
,14
]}

Armstrong, R. ^{[15
]}

Becker, M. R. ^{[3
,8
]}

Benoit-Levy, A. ^{[13
,16
,17
]}

Bernstein, G. M. ^{[1
]}

Bertin, E. ^{[16
,17
]}

Brooks, D. ^{[13
]}

Burke, D. L. ^{[3
,7
]}

Carnero Rosell, A. ^{[18
,19
]}

Kind, M. Carrasco ^{[20
,21
]}

Cunha, C. E.

D'Andrea, C. B. ^{[22
,23
]}

da Costa, L. N. ^{[18
,19
]}

Desai, S. ^{[24
,25
]}

Diehl, H. T. ^{[26
]}

Dietrich, J. P. ^{[24
,25
]}

Doel, P. ^{[13
]}

Estrada, J. ^{[26
]}

Evrard, A. E. ^{[27
,28
]}

Fausti Neto, A. ^{[18
]}

Flaugher, B. ^{[26
]}

Fosalba, P. ^{[10
]}

Frieman, J. ^{[6
,26
]}

Gruendl, R. A. ^{[20
,21
]}

Honscheid, K. ^{[9
,29
]}

James, D. J. ^{[12
]}

机构：

[1] Univ Pennsylvania, Dept Phys & Astron, Philadelphia, PA 19104 USA

[2] Barcelona Inst Sci ence & Technol, Inst Fisica Altes Energies IFAE, Campus UAB, E-08193 Barcelona, Spain

[3] Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[4] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England

[5] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA

[6] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[7] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[8] StanfordUniversity, Dept Phys, 382 Via PuebloMall, Stanford, CA 94305 USA

[9] Ohio State Univ sity, Ctr Cosmol & Astro Particle Phys, Columbus, OH 43210 USA

[10] CSIC, IEEC, Inst Ciencies Espai, Campus UAB,Carrer Can Magrans,S-N, E-08193 Barcelona, Spain

[11] Brookhaven Natl Lab, Bldg 510, Upton, NY 11973 USA

[12] Cerro Tololo Interamer Observ, Natl Optic Astron Observ, Casilla 603, La Serena, Chile

[13] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[14] Rhodes Univ, Dept Phys & Elect, POB 94, ZA-6140 Grahamstown, South Africa

[15] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA

[16] Inst Astrophys Paris, CNRS, UMR 7095, F-75014 Paris, France

[17] Sorbonne Univ, UPMC Univ Paris 06, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[18] Laboratorio Interinstituc Astron LIneA, Rua Gal Jos Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[19] Observatorio Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[20] Univ Illinois, Dept Astron, 1002 Green St, Urbana, IL 61801 USA

[21] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA

[22] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[23] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England

[24] Ludwig Maximilians Univ Munchen, Fac Phys, Scheinerstr 1, D-81679 Munich, Germany

[25] Excellence Cluster Univ, Boltzmannstr 2, D-85748 Garching, Germany

[26] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[27] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[28] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[29] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA

[30] Australian Astron Observ, N Ryde, NSW 2113, Australia

[31] Univ Sao Paulo, Inst Fis, Departamento Fis Matemat, CP 66318, BR-05314970 Sao Paulo, Brazil

[32] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamen, College Stn, TX 77843 USA

[33] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[34] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

[35] Max Planck Inst Extraterrestrial Phys, Giessenbachstrasse, D-85748 Garching, Germany

[36] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[37] Univ Sussex, Dept Phys & Astron, Pevensey Bldg, Brighton BN1 9QH, E Sussex, England

[38] Centro Investigac Energeticas Medioambient Tecnol, Madrid, Spain

[39] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA

[40] Argonne Natl Lab, 9700 South Cass Ave, Lemont, IL 60439 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 465卷 / 04期

基金：

英国科学技术设施理事会; 美国国家科学基金会;

关键词：

gravitational lensing: weak; galaxies: haloes; HALO OCCUPATION DISTRIBUTION; SHEAR POWER SPECTRA; DIGITAL SKY SURVEY; 100 SQUARE DEGREES; SDSS-III; COSMOLOGICAL CONSTRAINTS; INTRINSIC ALIGNMENTS; MAXIMUM-LIKELIHOOD; MATTER HALOES; DATA RELEASE;

D O I：

10.1093/mnras/stw2988

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present galaxy-galaxy lensing results from 139 deg(2) of Dark Energy Survey (DES) Science Verification (SV) data. Our lens sample consists of red galaxies, known as redMaGiC, which are specifically selected to have a low photometric redshift error and outlier rate. The lensing measurement has a total signal-to-noise ratio of 29 over scales 0.09 < R < 15 Mpc h(-1), including all lenses over a wide redshift range 0.2 < z < 0.8. Dividing the lenses into three redshift bins for this constant moving number density sample, we find no evidence for evolution in the halo mass with redshift. We obtain consistent results for the lensing measurement with two independent shear pipelines, NGMIX and IM3SHAPE. We perform a number of null tests on the shear and photometric redshift catalogues and quantify resulting systematic uncertainties. Covariances from jackknife subsamples of the data are validated with a suite of 50 mock surveys. The result and systematic checks in this work provide a critical input for future cosmological and galaxy evolution studies with the DES data and redMaGiC galaxy samples. We fit a halo occupation distribution (HOD) model, and demonstrate that our data constrain the mean halo mass of the lens galaxies, despite strong degeneracies between individual HOD parameters.

引用

页码：4204 / 4218

页数：15

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