论文标题

Gaia早期数据版本3-目录验证

Gaia Early Data Release 3 -- Catalogue validation

论文作者

Fabricius, C., Luri, X., Arenou, F., Babusiaux, C., Helmi, A., Muraveva, T., Reylé, C., Spoto, F., Vallenari, A., Antoja, T., Balbinot, E., Barache, C., Bauchet, N., Bragaglia, A., Busonero, D., Cantat-Gaudin, T., Carrasco, J. M., Diakité, S., Fabrizio, M., Figueras, F., Garcia-Gutierrez, A., Garofalo, A., Jordi, C., Kervella, P., Khanna, S., Leclerc, N., Licata, E., Lambert, S., Marrese, P. M., Masip, A., Ramos, P., Robichon, N., Robin, A. C., Romero-Gómez, M., Rubele, S., Weiler, M.

论文摘要

第三个Gaia数据发布分为两个阶段。早期部分Gaia EDR3提供了近20亿个来源的非常精确的星体和光度特性,并从Gaia DR2和700万个径向速度中提供了非常精确的天体和光度特性。完整的释放Gaia DR3将为大部分子集增加径向速度,光谱,光曲线和天体物理参数,以及太阳系对象的轨道。在发布目录之前,许多不同的数据项已经经过了专用验证过程。本文的目的是根据GAIA EDR3数据的完整性,准确性和精度来描述验证结果,并为使用目录数据提供建议。验证过程包括对目录内容的系统分析,以使用统计分析和对先前版本以及外部数据和模型的比较来检测各个错误或统计属性。与Gaia DR2相比,Gaia EDR3代表了前进的一步,就天文统计和光度法的精确性,准确性和完整性而言。我们提供了解决与零视差零点,负相似性,微弱来源的光度法和质量指标相关的问题的建议。

The third Gaia data release is published in two stages. The early part, Gaia EDR3, gives very precise astrometric and photometric properties for nearly two billion sources together with seven million radial velocities from Gaia DR2. The full release, Gaia DR3, will add radial velocities, spectra, light curves, and astrophysical parameters for a large subset of the sources, as well as orbits for solar system objects. Before the publication of the catalogue, many different data items have undergone dedicated validation processes. The goal of this paper is to describe the validation results in terms of completeness, accuracy, and precision for the Gaia EDR3 data and to provide recommendations for the use of the catalogue data. The validation processes include a systematic analysis of the catalogue contents to detect anomalies, either individual errors or statistical properties, using statistical analysis and comparisons to the previous release as well as to external data and to models. Gaia EDR3 represents a major step forward, compared to Gaia DR2, in terms of precision, accuracy, and completeness for both astrometry and photometry. We provide recommendations for dealing with issues related to the parallax zero point, negative parallaxes, photometry for faint sources, and the quality indicators.

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