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Mapping the stellar age of the Milky Way bulge with the VVV

机译:用VVV绘制银河系隆起的恒星年龄

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Context . The bulge represents the best compromise between old and massive Galactic components, and as such its study is a valuable opportunity to understand how the bulk of the Milky Way formed and evolved. In addition, being the only bulge in which we can individually resolve stars in all evolutionary sequences, the properties of its stellar content provide crucial insights into the formation of bulges. Aims . We are providing a detailed and comprehensive census of the Milky Way bulge stellar populations by producing deep and accurate photometric catalogs of the inner ~300 deg~(2)of the Galaxy. Methods . We performed DAOPHOT/ALLFRAME point spread function (PSF) fitting photometry of multi-epochs J and K _( s )images provided by the VISTA Variables in the Vía Láctea (VVV) survey to obtain deep photometric catalogs. Artificial star experiments have been conducted on all images to properly assess the completeness and the accuracy of the photometric measurements. Results . We present a photometric database containing nearly 600 million stars across the bulge area surveyed by the VVV. Through the comparison of derived color-magnitude diagrams of selected fields representative of different levels of extinction and crowding, we show the quality, completeness and depth of the new catalogs. With the exception of the fields located along the plane, this new photometry samples stars down to ~1–2 mag below the old main sequence turnoff with unprecedented accuracy. To demonstrate the tremendous potential inherent to this new dataset, we give a few examples of possible applications, including (i) star count studies through the dataset completeness map; (ii) surface brightness map; and (iii) cross-correlation with Gaia DR2. Conclusions . The database presented here represents an invaluable collection for the whole community, and we encourage its exploitation. The photometric catalogs including completeness information are publicly available through the ESO Science Archive as part of the MW-BULGE-PSPHOT release.
机译:语境。隆起代表了旧的和巨大的银河系组件之间的最佳折衷,因此,它的研究是了解银河系大部分形成和演化的宝贵机会。此外,作为唯一可以单独解析所有进化序列中的恒星的凸起,其恒星含量的性质为凸起的形成提供了至关重要的见解。目的。我们通过对银河系内部〜300度〜(2)的深度和准确的光度学目录,提供了银河系凸起恒星种群的详细而全面的人口普查。方法 。我们对VíaLáctea(VVV)调查中VISTA变量提供的多周期J和K _(s)图像执行了DAOPHOT / ALLFRAME点扩散函数(PSF)拟合光度法,以获得较深的光度学目录。已经对所有图像进行了人工星实验,以正确评估光度测量的完整性和准确性。结果。我们提供了一个光度数据库,该数据库包含VVV所调查的整个凸起区域中近6亿颗恒星。通过比较得出的代表不同灭绝和拥挤程度的选定字段的色度图表,我们显示了新目录的质量,完整性和深度。除了沿平面分布的场外,这种新的光度学以前所未有的精度对旧主序道岔下方的低至约1-2 mag的恒星进行采样。为了展示该新数据集固有的巨大潜力,我们给出了一些可能的应用示例,包括(i)通过数据集完整性图进行星数研究; (ii)表面亮度图; (iii)与Gaia DR2互相关。结论。这里介绍的数据库代表了整个社区的宝贵收藏,我们鼓励对其进行开发。包含完整性信息的测光目录可作为MW-BULGE-PSPHOT版本的一部分通过ESO科学存档公开获得。

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