鼓吹呜呜祖拉：UltraDeep HI与MeerKAT的观测
Trumpeting the Vuvuzela: UltraDeep HI observations with MeerKAT
摘要：
MeerKAT UltraDeep HI Survey旨在观察中性氢气的21 cm发射线，红移为z=1或更高。从直接探测和叠加信号，我们将解决HI质量函数，宇宙的宇宙中性气体密度（Omega_HI）及其在宇宙时间内的演化，以及星系演化，例如，Tully-Fisher关系，HI质量与哈勃类型或恒星质量的关系，Schmidt-Kennicutt成星定律。我们建议观察两个领域，COSMOS和钱德拉深场南（CDF-S）各1000小时，在2015年将实现MeerKAT（0.58-2.5 GHz）的全部瞬时带宽时，再增加4000小时。
英文摘要：
The MeerKAT UltraDeep HI Survey aims to observe the 21 cm emission line of neutral hydrogen gas out to a redshift of z=1 and beyond. From both direct detections and stacked signal, we will address the HI mass function, the cosmic neutral gas density of the Universe (Omega_HI) and their evolution over cosmic times, as well as galaxy evolution via e.g., the Tully-Fisher relation, the relation between HI mass and Hubble Type or stellar mass, and the Schmidt-Kennicutt star-formation law. We propose to observe two fields, the COSMOS and Chandra Deep Field South (CDF-S) for 1000 hours each, adding an additional 4000 hours to one of these fields in 2015 when the full instantaneous bandwidth of MeerKAT (0.58-2.5 GHz) will be realised.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
