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Window to the Universe for less money 10 years of PAIX from Antarctica

机译:用更少的钱向宇宙之窗南极洲的PAIX十年

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Time has come to implement a new way to study the stellar physics from the ground with long-term uninterrupted time series, multi-color photometry, flexibility during observing runs and all for less money. PAIX, Photometer Antarctica extinction, gives new insight to cope with unresolved stellar enigma and stellar oscillation challenges and bears witness, for the first time, to a new technology of the polar instrumental robotization under extreme human and weather conditions in the heart of Antarctica. In fact, the stellar pulsation plays a crucial role in understanding the Universe, however progress is limited by the data accuracy needed to detect numerous modes of oscillations with small amplitudes and by the discontinuous nature of typical ground-based data strings which often introduce ambiguities in the determination of oscillation frequencies. The recent space missions enable to overcome both difficulties, However, the outcome of the space missions shows large gaps in terms of flexibility during the observing runs, the choice of targets, the repair of failures and the inexorable high costs. We present here the new technology from Antarctica, in particular from South Polar Site Dome C that benefits from great image quality and 150 days high time coverage, where the seeing reaches a median value of 1 arcsec during the polar night. We briefly describe the instrumental performances of PAIX, its low-cost commercial components, robotic telescope, multi-band photometer and automatic control, working under harsh weather conditions, even when the temperature reach values as low as -80°C. The polar mission PAIX challenges the space missions and even has more advantages than CoRoT and KEPLER in observing in UBVRI bands and then collecting multicolor light curves simultaneously of several targets. We discuss here the first, outcomes of stellar physics from the heart of Antarctica during 10 polar nights and PAIX new results and perspectives on the pulsating stars from Antarctica, especially the connection between the stellar pulsation enigma and the Universe mysteries. Finally, we highlight the impact of PAIX -the robotic Antarctica photometer- on the Astronomy development.
机译:现在是时候以一种新的方式从地面研究恒星物理的方法,即长期不间断的时间序列,多色光度法,观察运行时的灵活性以及所有这些都需要花费更少的钱。 PAIX(南极灭绝光度计)为应对尚未解决的恒星谜团和恒星振荡挑战提供了新的见识,并首次见证了极地仪器机器人技术在极端人类和极端天气条件下在南极心脏地带的一项新技术。实际上,恒星脉动在理解宇宙中起着至关重要的作用,然而,进步受到检测小幅度的多种振荡模式所需的数据精度以及典型的基于地面的数据串的不连续性的限制,该数据串常常会引起模棱两可。确定振荡频率。最近的太空飞行任务可以克服这两个困难,但是,太空飞行的结果显示,在观察运行,目标选择,故障修复和无可避免的高昂费用方面存在很大的差距。我们在这里展示了南极洲的新技术,特别是南极站点Dome C的新技术,该技术得益于出色的图像质量和150天的长时间覆盖,在极地之夜的视线中值达到1 arcsec。我们简要介绍了PAIX的仪器性能,其低成本的商业组件,机器人望远镜,多波段光度计和自动控制,即使在温度达到-80°C时也能在恶劣的天气条件下工作。极地任务PAIX挑战太空任务,甚至比CoRoT和KEPLER更具优势,它可以观察UBVRI波段,然后同时收集多个目标的多色光曲线。我们将在这里讨论第一个十个极夜之夜来自南极心脏的恒星物理学的结果,以及PAIX对来自南极的脉动恒星的新结果和观点,尤其是恒星脉动之谜与宇宙之谜之间的联系。最后,我们重点介绍了PAIX(南极机器人光度计)对天文学发展的影响。

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