论文标题
全套NOIRLAB源目录的第二个数据发布
Second Data Release of the All-sky NOIRLab Source Catalog
论文作者
论文摘要
我们使用来自CTIO-4M+DECAM,KPNO-4M+MOSAIC3和BOK-2.3M+90PRIME的412,116个公共图像宣布NOIRLAB源目录(NSC)的第二个数据发布(DR2),使用412,116张公共图像。 NSC DR2包含超过39亿个独特的对象,680亿个单个源测量值,覆盖$ \ $ 35,000平方度的天空,在大多数宽带过滤器中,$ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ \ the $ \ $ \ $ \ $ \ $ \ $ \ $ \ $ 1-2%。 $ \ $ \ $ 30,000平方度的天空中约有19亿个物体具有三个或更多频段的光度法。 NSC DR1有几个改进。 DR2包括156,662(61%)的暴露量超过2年,其范围比DR1多。通过使用Skymapper DR1和Atlas-Ref2目录,$ GRIZ $中的Southern Sphotric zeropoints更为准确,并且将改进的灭绝校正用于高灭绝区域。此外,在校准单个图像的WC时,通过利用Gaia DR2的适当运动来提高星体精度。这将NSC的适当动作提高到$ \ sim $ 2.5 mas/yr(精度)和$ \ sim $ 0.2 mas/yr(准确性)。使用DBSCAN算法和每个对象的平均参数(例如平均幅度,正确运动等)将源成唯一对象的组合使用更加稳健地计算。最后,为每个对象计算了八个多波段光度变异性指标,并标记了变量对象(2300万个对象)。 NSC DR2对于探索太阳系对象,恒星流,矮卫星星系,QSOS,可变星,高播音器运动星和瞬变将很有用。提出了这些科学用例的几个例子。 NSC DR2目录可通过NOIRLAB的Astro Data Lab Science平台公开获得。
We announce the second data release (DR2) of the NOIRLab Source Catalog (NSC), using 412,116 public images from CTIO-4m+DECam, the KPNO-4m+Mosaic3 and the Bok-2.3m+90Prime. NSC DR2 contains over 3.9 billion unique objects, 68 billion individual source measurements, covers $\approx$35,000 square degrees of the sky, has depths of $\approx$23rd magnitude in most broadband filters with $\approx$1-2% photometric precision, and astrometric accuracy of $\approx$7 mas. Approximately 1.9 billion objects within $\approx$30,000 square degrees of sky have photometry in three or more bands. There are several improvements over NSC DR1. DR2 includes 156,662 (61%) more exposures extending over 2 more years than in DR1. The southern photometric zeropoints in $griz$ are more accurate by using the Skymapper DR1 and ATLAS-Ref2 catalogs, and improved extinction corrections were used for high-extinction regions. In addition, the astrometric accuracy is improved by taking advantage of Gaia DR2 proper motions when calibrating the WCS of individual images. This improves the NSC proper motions to $\sim$2.5 mas/yr (precision) and $\sim$0.2 mas/yr (accuracy). The combination of sources into unique objects is performed using a DBSCAN algorithm and mean parameters per object (such as mean magnitudes, proper motion, etc.) are calculated more robustly with outlier rejection. Finally, eight multi-band photometric variability indices are calculated for each object and variable objects are flagged (23 million objects). NSC DR2 will be useful for exploring solar system objects, stellar streams, dwarf satellite galaxies, QSOs, variable stars, high-proper motion stars, and transients. Several examples of these science use cases are presented. The NSC DR2 catalog is publicly available via the NOIRLab's Astro Data Lab science platform.