A search for H i absorption in distant star-forming galaxies with ASKAP-FLASH – I. Selection and analysis of the radio sample

Le résumé fourni par la source

ABSTRACT We present and discuss two catalogues of ultraviolet (UV)-selected (near-UV (NUV)$\lt 22.8$ mag) galaxies that lie within a 200 deg$^2$ area of sky covered by the ASKAP First Large Absorption Survey in H i (FLASH) and have an impact parameter of less than 20 arcsec to a FLASH radio continuum source. These catalogues are designed to enable a future search for 21 cm H i absorption in and around star-forming galaxies at redshift $0.4\lt z\lt 1$. We outline the production of this UV-bright data set, which has optical spectroscopy from the WiggleZ and Sloan Digital Sky Survey (SDSS) surveys and a median redshift of ${\sim} 0.6$. Analysis of the optical spectra, using multiple diagnostic diagrams, shows that galaxies with an impact parameter of less than 5 arcsec are likely to be physically associated with the radio source and are five times more likely to be an active galactic nucleus than objects without a radio match. Conversely, objects with impact factors between 5 and 20 arcsec are largely (>80 per cent) star-forming and resemble the overall WiggleZ population. The ($g - i$) colour evolution with redshift is consistent with a history of active star formation, but the radio-associated objects are typically redder and have colours similar to high-excitation radio galaxies. The redshift distribution of the two catalogues matches the overall distribution for WiggleZ galaxies, despite their otherwise rare radio properties. These catalogues can be expanded in future as new radio data become available, and a forthcoming paper will present the H i absorption results.

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