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Weak lensing of Type Ia Supernovae from the Dark Energy Survey
Monthly Notices of the Royal Astronomical Society ( IF 4.7 ) Pub Date : 2020-06-29 , DOI: 10.1093/mnras/staa1852
E Macaulay 1, 2 , D Bacon 2 , R C Nichol 2 , T M Davis 3 , J Elvin-Poole 4, 5 , D Brout 6, 7 , D Carollo 6, 8 , K Glazebrook 9 , S R Hinton 3 , G F Lewis 10 , C Lidman 11 , A Möller 12 , M Sako 7 , D Scolnic 13 , M Smith 14 , N E Sommer 11 , B E Tucker 11 , T M C Abbott 15 , M Aguena 16, 17 , J Annis 18 , S Avila 19 , E Bertin 20, 21 , S Bhargava 22 , D Brooks 23 , D L Burke 24, 25 , A Carnero Rosell 26 , M Carrasco Kind 27, 28 , J Carretero 29 , F J Castander 30, 31 , M Costanzi 32, 33 , L N da Costa 17, 34 , S Desai 35 , H T Diehl 18 , P Doel 23 , B Flaugher 18 , R J Foley 36 , J García-Bellido 19 , E Gaztanaga 30, 31 , D W Gerdes 37, 38 , D Gruen 24, 25, 39 , R A Gruendl 27, 28 , J Gschwend 17, 34 , G Gutierrez 18 , D L Hollowood 36 , K Honscheid 4, 5 , D Huterer 38 , D J James 40 , K Kuehn 41, 42 , N Kuropatkin 18 , O Lahav 23 , M Lima 16, 17 , M A G Maia 17, 34 , J L Marshall 43 , P Melchior 44 , F Menanteau 27, 28 , R Miquel 29, 45 , A Palmese 18, 46 , A A Plazas 44 , A K Romer 22 , A Roodman 24, 25 , E Sanchez 26 , V Scarpine 18 , M Schubnell 38 , S Serrano 30, 31 , I Sevilla-Noarbe 26 , M Soares-Santos 47 , E Suchyta 48 , M E C Swanson 28 , G Tarle 38 , T N Varga 49, 50 , A R Walker 15 , J Weller 49, 50 ,
Affiliation  

We consider the effects of weak gravitational lensing on observations of 196 spectroscopically confirmed Type Ia Supernovae (SNe Ia) from years 1 to 3 of the Dark Energy Survey (DES). We simultaneously measure both the angular correlation function and the non-Gaussian skewness caused by weak lensing. This approach has the advantage of being insensitive to the intrinsic dispersion of SNe Ia magnitudes. We model the amplitude of both effects as a function of σ_8, and find σ_8 =1.2|$^{+0.9}_{-0.8}$|⁠. We also apply our method to a subsample of 488 SNe from the Joint Light-curve Analysis (JLA; chosen to match the redshift range we use for this work), and find σ_8 =0.8|$^{+1.1}_{-0.7}$|⁠. The comparable uncertainty in σ_8 between DES–SN and the larger number of SNe from JLA highlights the benefits of homogeneity of the DES–SN sample, and improvements in the calibration and data analysis.

中文翻译:

暗能量调查中 Ia 型超新星的弱透镜效应

我们考虑了弱引力透镜对暗能量巡天 (DES) 的第 1 年至第 3 年的 196 颗光谱确认的 Ia 型超新星 (SNe Ia) 观测的影响。我们同时测量角相关函数和弱透镜引起的非高斯偏度。这种方法的优点是对 SNe Ia 震级的固有色散不敏感。我们将两种效应的幅度建模为 σ_8 的函数,并发现 σ_8 =1.2|$^{+0.9}_{-0.8}$|⁠。我们还将我们的方法应用于联合光曲线分析(JLA;选择匹配我们用于这项工作的红移范围)的 488 SNe 子样本,并发现 σ_8 =0.8|$^{+1.1}_{-0.7 }$|⁠。DES-SN 和来自 JLA 的大量 SNe 之间 σ_8 的可比不确定性突出了 DES-SN 样本同质性的好处,
更新日期:2020-06-29
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