FAST and Dark: A catalogue of Dark Galaxy Candidates within 50 Mpc
Marco Monaci, Duncan A. Forbes, Jonah S. Gannon, Bärbel S. Koribalski, Kenji Bekki + 2 more
TLDR
A new catalogue identifies 70 dark galaxy candidates within 50 Mpc using FAST HI data, showing they have higher linewidths than optically visible galaxies.
Key contributions
- Identifies 70 dark galaxy candidates (DGCs) within 50 Mpc using FAST HI survey data.
- DGCs are selected based on lacking optical counterparts in the DESI Legacy Survey.
- DGCs show higher HI linewidths for a given HI mass compared to optically detected galaxies.
- The catalogue provides a crucial basis for future follow-up studies of dark galaxies.
Why it matters
This paper presents the first catalogue of dark galaxy candidates from the FAST HI survey, offering crucial targets for understanding the nature of these elusive objects. Their distinct kinematic properties provide new insights into galaxy formation and dark matter distribution.
Original Abstract
Using the first data release of the Five-hundred-meter Aperture Spherical radio Telescope (FAST) All-Sky HI survey (FASHI), we compile a catalogue of 70 dark galaxy candidates (DGCs) within 50 Mpc. We select DGCs without an identified optical counterpart at a limiting g-band magnitude of ~ 28 mag arcsec^-2 in the DESI Legacy Survey, using both automatic cross-checking with optical catalogues and visual inspection of the colour images. After validating our DGCs, excluding potential spurious detections, issues in the registered position of the HI sources, and possible Radio Frequency Interferences (RFIs), we analyse their distribution over the surveyed sky, HI mass, linewidths, and inferred distance. They appear evenly distributed across the surveyed area, with no apparent bias to isolation. We did not find any DGC within the Local Volume (11 Mpc) in the sky surveyed by this first release of FASHI. We compare the observed properties of DGCs with those of galaxies with optical counterparts, finding that DGCs tend to have higher linewidths for a given HI mass. We discuss our DGCs in light of theoretical works, and compare them with other observational samples from previous HI surveys. This work presents a catalogue of dark galaxy candidates, which can serve as a basis for follow-up studies.
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