首页> 外文期刊>The Astrophysical Journal. Supplement Series >THE NEXT GENERATION VIRGO CLUSTER SURVEY-INFRARED (NGVS-IR). I. A NEW NEAR-ULTRAVIOLET, OPTICAL, AND NEAR-INFRARED GLOBULAR CLUSTER SELECTION TOOL?
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THE NEXT GENERATION VIRGO CLUSTER SURVEY-INFRARED (NGVS-IR). I. A NEW NEAR-ULTRAVIOLET, OPTICAL, AND NEAR-INFRARED GLOBULAR CLUSTER SELECTION TOOL?

机译:下一代处女座群集测量 - 红外(NGVS-IR)。 I.一种新的近紫外线,光学和近红外球簇选择工具?

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摘要

The NGVS-IR project (Next Generation Virgo Cluster Survey-Infrared) is a contiguous, near-infrared imaging survey of the Virgo cluster of galaxies. It complements the optical wide-field survey of Virgo (NGVS). In its current state, NGVS-IR consists of K_s-band imaging of 4 deg~2 centered on M87 and J- and K_s-band imaging of ~16 deg~2 covering the region between M49 and M87.We present observations of the central 4 deg~2 centered on Virgo's core region. The data were acquired with WIRCam on the Canada-France-Hawaii Telescope, and the total integration time was 41 hr distributed over 34 contiguous tiles. A survey-specific strategy was designed to account for extended galaxies while still measuring accurate sky brightness within the survey area. The average 5σ limiting magnitude is K_s = 24.4 AB mag, and the 50% completeness limit is K_s = 23.75 AB mag for point-source detections, when using only images with better than 0."7 seeing (median seeing 0."54). Star clusters are marginally resolved in these image stacks, and Virgo galaxies with μ_K)s ? 24.4 AB mag arcsec~(?2) are detected. Combining the K_s data with optical and ultraviolet data, we build the uiK_s color-color diagram, which allows a very clean color-based selection of globular clusters in Virgo. This diagnostic plot will provide reliable globular cluster candidates for spectroscopic follow-up campaigns, needed to continue the exploration of Virgo's photometric and kinematic substructures, and will help the design of future searches for globular clusters in extragalactic systems. We show that the new uiKs diagram displays significantly clearer substructure in the distribution of stars, globular clusters, and galaxies than the gzK_s diagram-the NGVS + NGVS-IR equivalent of the BzK diagram that is widely used in cosmological surveys. Equipped with this powerful new tool, future NGVS-IR investigations based on the uiK_s diagram will address the mapping and analysis of extended structures and compact stellar systems in and around Virgo galaxies.
机译:NGVS-IR项目(下一代Virgo Cluster Revely-Invarared)是一个连续的近乎红外成像的星系群体群。它补充了Virgo(NGV)的光学宽场调查。在其当前状态下,NGVS-IR由K_S带成像组成,以4°和覆盖M87和J-和K_S带成像,覆盖M49和M87之间的区域的M87和J和K_S带成像.WE呈现中央的观察以维戈的核心地区为中心4°〜2。在加拿大 - 法国 - 夏威夷望远镜上用威拉姆获取数据,总集成时间为41小时,分布在34个连续瓷砖上。调查特定的策略旨在考虑扩展的星系,同时仍在测量调查区域内的准确天空亮度。平均5σ限制幅度为k_s = 24.4ab mag,并且对于点源检测,50%的完整性限制为k_s = 23.75Ab mag,当时仅使用优于0.“看到(中位数0.”54) 。星集群在这些图像堆栈中略微解决,以及具有μ_k的处女座星系)s?检测到24.4 AB Magsec〜(?2)。将K_S数据与光学和紫外数据组合,我们构建了UIK_S颜色图,该图允许在处女座中非常干净的基于颜色的球簇选择。这种诊断图将为光谱跟踪活动提供可靠的球形集群候选者,以继续探索处于处女座的光度和运动学子结构,并有助于在刷新系统中设计未来搜索球簇的搜索。我们表明,新的UIK图表在恒星,球簇和星系的分布中显示出明显更清晰的子结构,而不是GZK_S图 - NGVS + NGVS-IR相当于广泛用于宇宙学调查的BZK图。配备这种强大的新工具,未来的基于UIK_S图的NGVS-IR调查将解决维槽星系中的扩展结构和紧凑型恒星系统的映射和分析。

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  • 作者单位

    Instituto de Astrofísica Facultad de Física Pontificia Universidad Católica de Chile Av. Vicu?a Mackenna 4860 7820436 Macul Santiago Chile;

    Instituto de Astrofísica Facultad de Física Pontificia Universidad Católica de Chile Av. Vicu?a Mackenna 4860 7820436 Macul Santiago Chile;

    Observatoire astronomique de Strasbourg Université de Strasbourg CNRS UMR 7550 11 rue de l'Universite F-67000 Strasbourg France;

    Department of Astronomy Peking University Beijing 100871 China;

    Herzberg Institute of Astrophysics National Research Council of Canada Victoria BC V9E 2E7 Canada;

    Herzberg Institute of Astrophysics National Research Council of Canada Victoria BC V9E 2E7 Canada;

    Herzberg Institute of Astrophysics National Research Council of Canada Victoria BC V9E 2E7 Canada;

    GEPI Observatoire de Paris CNRS Université Paris Diderot 5 Place J. Janssen F-92190 Meudon Cedex France;

    Canada-France-Hawaii Telescope Corporation Kamuela HI 96743 USA;

    Institut d'Astrophysique de Paris UMR 7095 CNRS &

    UPMC 98 bis Boulevard Arago F-75014 Paris France;

    Department of Physics Engineering Physics and Astronomy Queen's University Kingston ON Canada;

    Laboratoire AIM Paris-Saclay CNRS/INSU Université Paris Diderot CEA/IRFU/SAp F-91191 Gif-sur-Yvette Cedex France;

    Department of Physics and Astronomy University of Waterloo Waterloo ON N2L 3G1 Canada;

    Aix Marseille Université CNRS LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326 F-13388 Marseille France;

    Laboratoire AIM Paris-Saclay CNRS/INSU Université Paris Diderot CEA/IRFU/SAp F-91191 Gif-sur-Yvette Cedex France;

    Department of Astronomy and Astrophysics University of Toronto Toronto ON M5S 3H4 Canada;

    Institute of Astronomy University of Cambridge Madingley Road Cambridge CB3 0HA UK;

    Department of Physics and Astronomy Youngstown State University One University Plaza Youngstown OH 44555 USA;

    Instituto de Astrofísica Facultad de Física Pontificia Universidad Católica de Chile Av. Vicu?a Mackenna 4860 7820436 Macul Santiago Chile;

    Université de Lyon 1 CRAL Observatoire de Lyon 9 av. Charles André F-69230 Saint-Genis Laval CNRS UMR 5574 ENS de Lyon France;

    Università degli Studi di Milano-Bicocca Piazza della Scienza 3 I-20126 Milano Italy;

    Herzberg Institute of Astrophysics National Research Council of Canada Victoria BC V9E 2E7 Canada;

    GEPI Observatoire de Paris CNRS Université Paris Diderot 5 Place J. Janssen F-92190 Meudon Cedex France;

    Aix Marseille Université CNRS LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326 F-13388 Marseille France;

    Instituto de Astrofísica Facultad de Física Pontificia Universidad Católica de Chile Av. Vicu?a Mackenna 4860 7820436 Macul Santiago Chile;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天体物理学;
  • 关键词

    galaxies; clusters; individual (Virgo) - galaxies; distances and redshifts - galaxies; luminosity function; mass function - galaxies; photometry - galaxies; star clusters; general;

    机译:星系;个人(处女座) - 星系;距离和红移 - 星系;亮度函数;质量功能 - 星系;光度法 - 星系;星团;一般;
  • 入库时间 2022-08-20 07:00:49

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