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Radio-frequency interference environment Solar and planetary science Synergies with other disciplines (e.g ...Radio-frequency interference environment Solar and planetary science Synergies with other disciplines (e.g ...
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报名链接: https://docs.qq.com/form/page/DU2lXdnBWbnlQRkF1 | ...
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This catalog is divided into two subsamples, i.e., the primary and secondary parts.
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The Gaia+PanSTARRS1(PS1)+SDSS+2MASS(GPS1)自行星表于2017年发布,为大约3.5亿目标提供了精确的自行数据,星等下限为r~20mag。在这个新版本中,作者介绍了GPS1扩展星表,基于Gaia DR2, PS1、SDSS和2MASS,GPS1扩展星表扩展到r~22.5Mag,为∼4亿目标提供了自行数据,其特征系统误差小于0.1mas/年 ...主要部分的∼2.64亿目标有或同时具有Gaia和SDSS天测数据,典型的精度为2.0-5.0mas/年。次要部分∼1.36亿目标只有PS1天体测量信息,其中平均精度要低于15.0mas/年。
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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Geostationary Operational Environmental Satellite class M1.0 and larger that occurred during 2010-2019, i.e.
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Geostationary Operational Environmental Satellite class M1.0 and larger that occurred during 2010-2019, i.e.
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investigate the origins of HiVelSCs, we perform orbit integrations and divide them into four types, i.e.
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investigate the origins of HiVelSCs, we perform orbit integrations and divide them into four types, i.e.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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Our method is valid for FGK stars with G ≤ 16, [Fe/H] ≥ -2.5, and E(B - V) ≤ 0.5.
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Our method is valid for FGK stars with G ≤ 16, [Fe/H] ≥ -2.5, and E(B - V) ≤ 0.5.
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forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[e] ...
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forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[e] ...
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aim of investigating how the magnetic field in solar active regions (ARs) controls flare activity, i.e.
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aim of investigating how the magnetic field in solar active regions (ARs) controls flare activity, i.e.