Probing the Low Surface Brightness Universe with Dragonfly

用蜻蜓号探测低表面亮度宇宙

• 批准号: RGPIN-2017-05989
• 负责人: Abraham, Roberto
• 金额: $ 7.87万
• 依托单位: University of Toronto
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2019
• 资助国家: 加拿大
• 起止时间: 2019-01-01 至 2020-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=692932
• 关键词: Probing; Low; Surface; Brightness; Universe

Over the past 40 years the cutting edge of astronomical imaging has transitioned from photographic plates on ground based telescopes to CCD detectors on space telescopes. This has improved our ability to detect small faint galaxies by about seven magnitudes (over a factor of 600). Over this same period of time there has been no improvement in our ability to detect large but faint (low surface brightness) structures in the Universe. This is because the limiting factor in this case is not photon statistics or image resolution, it is control of systematic errors, such as the scattering of light and sky variability. Working with a colleague at Yale, I recently developed a novel new telescope, the Dragonfly Telephoto Array, which has succeeded in breaking through this technical barrier and which is revealing the composition of the Universe at very faint surface brightness levels (Abraham g as the Milky Way but have only 1/100 1/1000 of its mass, and explaining how they survive in the very hostile environment of a galaxy cluster is a major puzzle that has become a highly active area of investigation in the last year. But these early results from Dragonfly are only the tip of the iceberg. It is now clear that the low surface brightness Universe is a treasure trove of almost totally unexplored astrophysical phenomena, and the race is now on to study these. In this proposal I describe a program of investigation whose goals are to: (1) explore the nature of dark matter in ultra-diffuse galaxies by determining their masses in galactic stellar halos; (2) test fundamental predictions of models for galaxy assembly by undertaking an ambitious wide-area survey of the low surface brightness sky; (3) determine the ultimate limits for the performance of the Dragonfly concept, in order to see if we can grow the system to the point that we can directly explore the "cosmic web" a predicted large-scale network of dark matter filaments believed to connect galaxies to each other.

在过去的40年里，天文成像的前沿已经从地面望远镜的照相底片过渡到空间望远镜的CCD探测器。这提高了我们探测微弱星系的能力，大约提高了7个星等（超过600倍）。在这段时间里，我们探测宇宙中巨大但微弱（低表面亮度）结构的能力没有任何提高。这是因为在这种情况下，限制因素不是光子统计或图像分辨率，而是对系统误差的控制，例如光的散射和天空变化。我最近与耶鲁大学的一位同事合作，开发了一种新颖的新望远镜，蜻蜓长焦阵列，它成功地突破了这一技术障碍，并在非常微弱的表面亮度水平上揭示了宇宙的组成（亚伯拉罕g作为银河系，但只有其质量的1/100 1/1000，解释它们如何在星系团的恶劣环境中生存是一个主要的谜团，在去年已经成为一个高度活跃的研究领域。但蜻蜓的这些早期结果只是冰山一角。现在很清楚，低表面亮度的宇宙是一个几乎完全未被探索的天体物理现象的宝库，现在正在进行研究。在这个建议中，我描述了一个研究计划，其目标是：（1）通过确定银河系恒星晕中暗物质的质量来探索超漫射星系中暗物质的性质：（2）通过对低表面亮度天空进行雄心勃勃的广域调查来测试星系聚集模型的基本预测;（3）确定“蜻蜓”概念性能的极限，为了看看我们是否可以将系统发展到我们可以直接探索“宇宙网”的地步，一个预测的大型-暗物质细丝的规模网络，被认为是将星系彼此连接起来。