首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program strategy and clustering properties of similar to 2000 Ly alpha emitters at z=6-7 over the 0.3-0.5 Gpc(2) survey area
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Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program strategy and clustering properties of similar to 2000 Ly alpha emitters at z=6-7 over the 0.3-0.5 Gpc(2) survey area

机译:蛛网HSC(Silverrush)可见勘探和标准研究的系统鉴定。 I.在0.3-0.5 GPC(2)调查区域的Z = 6-7的2000 Lyα发射器类似于2000 Lyα发射器的程序策略和聚类性质

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摘要

We present the SILVERRUSH program strategy and clustering properties investigated with similar to 2000 Ly alpha emitters (LAEs) at z = 5.7 and 6.6 found in the early data of the Hyper Suprime-Cam (HSC) Subaru Strategic Program survey exploiting the carefully designed narrow-band filters. We derive angular correlation functions with the unprecedentedly large samples of LAEs at z = 6-7 over the large total area of 14-21 deg(2) corresponding to 0.3-0.5 comoving Gpc(2). We obtain the average large-scale bias values of b(avg) = 4.1 +/- 0.2 (4.5 +/- 0.6) at z = 5.7 (z = 6.6) for greater than or similar to L* LAEs, indicating a weak evolution of LAE clustering from z = 5.7 to 6.6. We compare the LAE clustering results with two independent theoretical models that suggest an increase of an LAE clustering signal by the patchy ionized bubbles at the epoch of reionization (EoR), and estimate the neutral hydrogen fraction to be x(HI) = 0.15-(+0.15)(0.15) at z = 6.6. Based on the halo occupation distributionmodels, we find that the greater than or similar to L* LAEs are hosted by dark-matter halos with an average mass of log( M-h/M-circle dot ) = 11.1(-0.4)(+0.2) (10.8(-0.5)(+0.3)) at z = 5.7 (6.6) with a Ly alpha duty cycle of 1% or less, where the results of z = 6.6 LAEs may be slightly biased, due to the increase of the clustering signal at the EoR. Our clustering analysis reveals the low-mass nature of greater than or similar to L* LAEs at z = 6-7, and that these LAEs probably evolve into massive super-L* galaxies in the present-day universe.
机译:我们提出了Silverrush计划策略和集群特性,并在Z = 5.7和6.6中以类似于2000年的alpha发射器(Laes),在超级Suprime-CAM(HSC)斯巴鲁战略计划调查中发现的Z = 5.7和6.6,利用精心设计的狭义 - 带滤波器。我们通过在对应于0.3-0.5的大面积为0.3-0.5的GPC(2)的大小为0.3-0.5的大面积为0.3-0.5的Z = 6-7的前所未有的Laes的角度相关函数。我们在Z = 5.7(z = 6.6)中获得B(AVG)= 4.1 +/- 0.2(4.5 +/- 0.6)的平均大规模偏置值大于或类似于L * Laes,表示弱进化从z = 5.7到6.6的Lae聚类。我们将LAE聚类结果与两个独立的理论模型进行比较,这表明通过在环化(EOR)时期的斑块电离气泡增加了LAE聚类信号,并估计中性氢馏分为X(HI)= 0.15-( +0.15)(0.15)在z = 6.6。基于光环占领分布模型,我们发现大于或类似的L * Laes由暗物晕圈托管,彩色卤素,平均物质量的对数(& mh / m圆点&)= 11.1(-0.4) (+0.2)(10.8(-0.5)(+ 0.3)),z = 5.7(6.6),Ly alpha占空比为1%或更少,其中Z = 6.6的结果可能略微偏置,由于EOR处的聚类信号的增加。我们的聚类分析揭示了大于或类似于Z = 6-7的L * Laes的低质量性质,并且这些Laes可能在当今宇宙中进化到大规模的超级L *星系中。

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  • 作者单位

    Univ Tokyo Inst Cosm Ray Res 5-1-5 Kashiwanoha Kashiwa Chiba 2778582 Japan;

    Univ Tokyo Inst Cosm Ray Res 5-1-5 Kashiwanoha Kashiwa Chiba 2778582 Japan;

    Univ Tokyo Inst Cosm Ray Res 5-1-5 Kashiwanoha Kashiwa Chiba 2778582 Japan;

    Univ Tokyo Grad Sch Sci Dept Astron Bunkyo Ku 7-3-1 Hongo Tokyo 1130033 Japan;

    Open Univ Japan Mihama Ku Wakaba 2-11 Chiba 2618586 Japan;

    Univ Tokyo Inst Cosm Ray Res 5-1-5 Kashiwanoha Kashiwa Chiba 2778582 Japan;

    Kure Coll Natl Inst Technol Fac Nat Sci 2-2-11 Agaminami Kure Hiroshima 7378506 Japan;

    Ehime Univ Res Ctr Space &

    Cosm Evolut 2-5 Bunkyo Cho Matsuyama Ehime 7908577 Japan;

    Ehime Univ Res Ctr Space &

    Cosm Evolut 2-5 Bunkyo Cho Matsuyama Ehime 7908577 Japan;

    Univ Tokyo Inst Cosm Ray Res 5-1-5 Kashiwanoha Kashiwa Chiba 2778582 Japan;

    Osaka Sangyo Univ Fac Design Technol Dept Environm Sci &

    Technol 3-1-1 Nagaito Daito Osaka 5748530 Japan;

    Univ Tsukuba Ctr Computat Sci 1-1-1 Tennodai Tsukuba Ibaraki 3058577 Japan;

    Univ Tsukuba Ctr Computat Sci 1-1-1 Tennodai Tsukuba Ibaraki 3058577 Japan;

    Nagoya Univ Dept Phys &

    Astrophys Chikusa Ku Furo Cho Nagoya Aichi 4648602 Japan;

    Univ Tokyo Inst Cosm Ray Res 5-1-5 Kashiwanoha Kashiwa Chiba 2778582 Japan;

    Natl Astron Observ Japan 2-21-1 Osawa Mitaka Tokyo 1818588 Japan;

    Natl Astron Observ Japan 2-21-1 Osawa Mitaka Tokyo 1818588 Japan;

    European Southern Observ Karl Schwarzschild Str 2 D-85748 Garching Germany;

    Univ Hyogo Ctr Astron Nishi Harima Astron Observ 407-2 Nishigaichi Sayo Cho Sayo Hyogo 6795313 Japan;

    Acad Sinica Inst Astron &

    Astrophys 11F AS NTU Astron Math Bldg 1 Sec 4 Roosevelt Rd Taipei 10617 Taiwan;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

    cosmology: observations; galaxies: formation; galaxies: high-redshift;

    机译:宇宙学:观察;星系:形成;星系:高射频;

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