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arxiv: 1705.04210 · v1 · pith:BLCETCIXnew · submitted 2017-05-11 · 🌌 astro-ph.CO · astro-ph.GA

Tracing HI Beyond the Local Universe

Martin Meyer , Aaron Robotham , Danail Obreschkow , Tobias Westmeier , Alan Duffy , Lister Staveley-Smith This is my paper
classification 🌌 astro-ph.CO astro-ph.GA
keywords beyondemissionlocaltracinguniversewillanalysisappropriate
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The SKA and its pathfinders will enable studies of HI emission at higher redshifts than ever before. In moving beyond the local Universe, this will require the use of cosmologically appropriate formulae that have traditionally been simplified to their low-redshift approximations. In this paper, we summarise some of the most important relations for tracing HI emission in the SKA era, and present an online calculator to assist in the planning and analysis of observations (hifi.icrar.org).

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  1. The FAST Hundred-Deg$^2$ HI Deep (HD$^2$) Survey: Early Results from the Pilot Survey

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    Pilot FAST HD² survey reports 339 new HI detections in 10 deg² with 0.45 mJy rms, high DESI optical matching rates, and gas fraction relations consistent with ALFALFA, DINGO, and xGASS.