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The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections

机译:莱顿/阿根廷/波恩(LAB)的银河HI调查:LDS和IAR组合调查的最终数据发布,具有改进的杂散辐射校正

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摘要

We present the final data release of observations of ?21-cm emission from Galactic neutral hydrogen over the entire sky, merging the Leiden/Dwingeloo Survey (LDS: Hartmann & Burton 1997, Atlas of Galactic Neutral Hydrogen) of the sky north of ? = ?30? with the Instituto Argentino de Radioastronomía Survey (IAR: Arnal et al. 2000, A&AS, 142, 35; and Bajaja et al. 2005, A&A, 440, 767) of the sky south of ? = ?25?. The angular resolution of the combined material is HPBW ? 0. ?6. The LSR velocity coverage spans the interval ?450 km s?1 to +400 km s?1, at a resolution of 1.3 kms?1. The data were corrected for stray radiation at the Institute for Radioastronomy of the University of Bonn, refining the original correction applied to the LDS. The rms brightness-temperature noise of the merged database is 0.07?0.09 K. Residual errors in the profile wings due to defects in the correction for stray radiation are for most of the data below a level of 20?40 mK. It would be necessary to construct a telescope with a main beam efficiency of ?MB >? 99% to achieve the same accuracy. The merged and refined material entering the LAB Survey of Galactic HI is intended to be a general resource useful to a wide range of studies of the physical and structural characteristices of the Galactic interstellar environment. The LAB Survey is the most sensitive Milky Way HI survey to date, with the most extensive coverage both spatially and kinematically.
机译:我们提出了整个星系中银河系中性氢在21厘米处发射的观测数据的最终数据发布,该数据合并了莱顿市北部天空的Leiden / Dwingeloo调查(LDS:Hartmann&Burton 1997,银河系中性氢图集)。 = 30?利用阿根廷南部射电天文学研究所(IAR:Arnal等2000,A&AS,142,35;和Bajaja等2005,A&A,440,767)对南半球的天空进行观测。 = 25。组合材料的角分辨率为HPBW? 0.?6。 LSR速度覆盖范围为450 km s-1至+400 km s-1,分辨率为1.3 kms-1。波恩大学放射天文学研究所对数据进行了杂散辐射校正,从而完善了应用于LDS的原始校正方法。合并后的数据库的均方根亮度-温度噪声为0.07-0.09K。对于杂散辐射校正中的缺陷,轮廓翼中的残留误差在大多数数据中都在20-40 mK以下。有必要建造一个主光束效率为“ MB>”的望远镜。达到相同精度的99%。合并后的精炼材料将进入银河HI实验室调查,旨在成为一种通用资源,可广泛用于研究银河星际环境的物理和结构特征。 LAB调查是迄今为止最敏感的银河系HI调查,在空间和运动学上涵盖最广泛。

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