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Proper motions with Subaru II. A sample in the Subaru/XMM-Newton Deep Survey field

机译:适用于斯巴鲁II的运动。斯巴鲁/ Xmm-Newton Deep的样品   调查领域

摘要

We search for stars with proper motions in a set of deep Subaru images,covering about 0.48 square degrees to a depth of $i' \simeq 26$, taken over aspan of five and a half years. We follow the methods described in\citet{Richmond2009} to reduce and analyze this dataset. We present a sample of69 stars with motions of high significance, and discuss briefly the populationsfrom which they are likely drawn. Based on photometry and motions alone, weexpect that 14 of the candidates may be white dwarfs. Our candidate with thelargest proper motion is surprisingly faint and likely to prove interesting:its colors and motions suggest that it might be an M dwarf moving at over 500km/sec or an L dwarf in the halo.
机译:我们在一系列深层的Subaru影像中搜索具有适当运动的恒星,这些影像覆盖了约五年半的时间,覆盖了约0.48平方度的深度$ i'\ simeq 26 $。我们遵循\ citet {Richmond2009}中描述的方法来减少和分析此数据集。我们提出了一个具有高意义运动的69个恒星样本,并简要讨论了可能从中提取的总体。仅根据光度法和运动,我们预计其中14位候选人可能是白矮星。我们的具有最大适当运动的候选人出乎意料地微弱,并且可能证明很有趣:它的颜色和运动表明它可能是移动速度超过500 km / sec的M矮人或光环中的L矮人。

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