论文标题

银河磁盘以外的VVV近IIR Galaxy目录

The VVV Near-IR Galaxy Catalogue beyond the Galactic disk

论文作者

Baravalle, Laura D., Alonso, M. Victoria, Minniti, Dante, Castellón, José Luis Nilo, Soto, Mario, Valotto, Carlos, Villalón, Carolina, Graña, Darío, Amôres, Eduardo B., Castro, F. Milla

论文摘要

关于星系的大规模分布的知识远非避免区域的完整,这主要是由于星际灭绝率高,并且在较低的银河纬度上产生了混乱。过去的近红外(NIR)调查,例如两个微米的所有天空调查(2量),已经显示出在这些纬度上探测大型结构的力量。我们的目的是使用VíaLáctea调查(VVV)中的Vista变量来绘制整个银河平面的星系分布,该变量达到了比2个质量更深的2至4个大小。我们使用sextractor + psfex识别扩展对象并测量其大小,光浓度指数,大小和颜色。形态和颜色限制和视觉检查用于确认星系。我们介绍了5563个视觉确认星系的结果VVV NIR星系目录,其中只有45个已知。这是向银河平面的星系目录最大的目录,其中99%的星系是新发现。我们发现,星系密度分布与现有NIR图的低星间灭绝分布非常相似。我们还介绍了该地区观察到的185 2个质量扩展来源的描述,其中16%的对象没有以前的描述,我们现在已经对其进行了分类。我们得出的结论是,星际灭绝和恒星密度是检测回避区域背景星系的主要局限性。 VVV NIR Galaxy目录是一个新数据集,为银河系平面中的乳乳外研究提供了信息。

Knowledge about the large-scale distribution of galaxies is far from complete in the Zone of Avoidance, which is mostly due to high interstellar extinction and to source confusion at lower Galactic latitudes. Past near-infrared (NIR) surveys, such as the Two Micron All Sky Survey (2MASS), have shown the power of probing large-scale structure at these latitudes. Our aim is to map the galaxy distribution across the Southern Galactic plane using the VISTA Variables in the Vía Láctea Survey (VVV), which reach 2 to 4 magnitudes deeper than 2MASS. We used SExtractor + PSFEx to identify extended objects and to measure their sizes, the light concentration index, magnitudes, and colours. Morphological and colour constraints and visual inspection were used to confirm galaxies. We present the resulting VVV NIR Galaxy Catalogue of 5563 visually confirmed galaxies, of which only 45 were previously known. This is the largest catalogue of galaxies towards the Galactic plane, with 99% of these galaxies being new discoveries. We found that the galaxy density distribution closely resembled the distribution of low interstellar extinction of the existing NIR maps. We also present a description of the 185 2MASS extended sources observed in the region, of which 16% of these objects had no previous description, which we have now classified. We conclude that interstellar extinction and stellar density are the main limitations for the detection of background galaxies in the Zone of Avoidance. The VVV NIR Galaxy Catalogue is a new data set providing information for extragalactic studies in the Galactic plane.

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