论文标题

与盖亚(Gaia)一起研究的热分子恒星的种群 - iv。基于Gaia EDR3的热级别星星的目录

The population of hot subdwarf stars studied with Gaia -- IV. Catalogues of hot subluminous stars based on Gaia EDR3

论文作者

Culpan, Richard, Geier, Stephan, Pelisoli, Ingrid, Reindl, Nicole, Fusillo, Nicola Gentile, Vorontseva, Alina

论文摘要

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data release 3 (DR3) catalogue of the known hot subdwarf stars contains 6,616 unique sources and provides multi-band photometry, and astrometry from Gaia EDR3以及基于光谱和颜色的分类。这比DR2目录增加了742个对象。该新目录为3,087颗恒星和径向速度提供了大气参数,用于文献中的2,791颗恒星。此外,我们使用Gaia EDR3数据集的精确度以及更新的质量和选择标准,以产生61,585个热糖星的Gaia EDR3目录,更新了热溢流星的Gaia数据版本2(DR2)目录,以提高了21,785个对象的GAIA EDR3目录。与Gaia DR2相比,GAIA EDR3天文测量和光度法的改进使我们能够定义更复杂的选择功能。特别是,我们通过包括具有明显的邻居但范围占主导地位的通量水平的来源,改善了银河平面拥挤区域以及麦哲伦云方向的热舒张星的检测。

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data release 3 (DR3) catalogue of the known hot subdwarf stars contains 6,616 unique sources and provides multi-band photometry, and astrometry from Gaia EDR3 as well as classifications based on spectroscopy and colours. This is an increase of 742 objects over the DR2 catalogue. This new catalogue provides atmospheric parameters for 3,087 stars and radial velocities for 2,791 stars from the literature. In addition, we have updated the Gaia Data Release 2 (DR2) catalogue of hot subluminous stars using the improved accuracy of the Gaia EDR3 data set together with updated quality and selection criteria to produce the Gaia EDR3 catalogue of 61,585 hot subluminous stars, representing an increase of 21,785 objects. The improvements in Gaia EDR3 astrometry and photometry compared to Gaia DR2 have enabled us to define more sophisticated selection functions. In particular, we improved hot subluminous star detection in the crowded regions of the Galactic plane as well as in the direction of the Magellanic Clouds by including sources with close apparent neighbours but with flux levels that dominate the neighbourhood.

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