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基于盖亚(Gaia)DR3 XP光谱的650万颗主红团簇星全天星表

An All-Sky Catalog of 6.5 Million Primary Red Clump Stars from Gaia DR3 XP Spectra

Zheng Yu, Bingqiu Chen

arXiv 2608.28522首次发表:更新:

AI 中文总结

该研究利用盖亚DR3 XP光谱训练混合密度网络,构建含650万颗主红团簇星的全天星表,校准盖亚视差零点偏移,为银河考古学提供重要资源。

AI 中文摘要

红团簇(RC)星是绘制银河系三维结构的极佳标准烛光。我们利用从盖亚(Gaia)DR3低分辨率XP光谱推断出的星震参数的光谱估计值,构建了包含650万颗主RC星的全天星表。我们在交叉匹配样本上训练了混合密度网络(MDN),该网络将每个343维的校正XP光谱映射到偶极重力模式的渐近周期间隔ΔΠ₁和大频率间隔Δν的估计值。我们利用这两个估计值筛选主RC星,发布了两个互补星表,分别由不同的参数空间切割和阈值定义:纯度达97%的高纯度Tier 1样本,包含532,189颗恒星;以及 completeness达86%的高完备性Tier 2样本,包含6,534,931颗恒星。两个星表均覆盖全天球,我们为所有恒星提供了距离和消光值。对于Tier 1 RC星,我们获得了6%的测光距离中值精度;利用所得距离,我们独立校准了盖亚(Gaia)DR3的视差零点偏移。Tier 2样本追踪的三维密度分布连续延伸至R≈25千秒差距(kpc),两个星表均公开可用。这些星表为银河考古学提供了宝贵资源,提供了均匀数据集以追踪银河系的化学动力学演化,并校准恒星族模型。

英文摘要

Red clump (RC) stars are excellent standard candles for mapping the three-dimensional structure of the Milky Way. We construct an all-sky catalog of 6.5 million primary RC stars using spectroscopic estimates of asteroseismic parameters inferred from Gaia DR3 low-resolution XP spectra. We train a mixture density network (MDN) on a cross-matched sample. The network maps each 343-dimensional corrected XP spectrum to estimates of $ΔΠ_{1}$, the asymptotic period spacing of dipole gravity modes, and $Δν$, the large frequency separation. We select primary RC stars using these two estimates. We release two complementary catalogs defined by different parameter-space cuts and thresholds: a high-purity Tier 1 sample of 532,189 stars with 97% purity and a high-completeness Tier 2 sample of 6,534,931 stars with 86% completeness. Both catalogs cover the full celestial sphere. We provide distances and extinction values for all stars. We obtain a median photometric distance precision of 6% for Tier 1 RC stars. Using the resultant distances, we independently calibrate the Gaia DR3 parallax zero-point offset. The three-dimensional density distribution traced by the Tier 2 sample extends continuously to $R\approx25$ kpc. Both catalogs are publicly available. These catalogs provide a valuable resource for Galactic archaeology, delivering a homogeneous dataset to trace the chemo-dynamical evolution of the Milky Way and to calibrate models of stellar populations.

Comments15 pages, 6 figures, 1 table. Catalogs available at https://nadc.china-vo.org/res/r101871/

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