Catalog Description

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This catalog contains 339 extragalactic HI sources detected in the pilot survey of FAST Hundred-Deg² HI Deep (HD²) Survey, corresponding to Table 5 of Xu et al. 2026 in the FITS format.

Title: The FAST Hundred-Deg² HI Deep (HD²) Survey: Early Results from the Pilot Survey
Authors: Xu C., Jing Y., Wang J., Zou H., Du W., Yu N., Guo H., Liu Z., Chen Q., Liang T., Hou Z., Xu Y., Li X., Hu H., Liu Z., Zhao P., Fang T., Gao L., Guo Q., Gu Q., Jiang Z., Kang X., Kong X., Li C., Pan J., Wang T., Zhou Y., Wang W., Wang J.
Paper: arXiv:XXXX.XXXXX
Version: Pre-release (2026/05, v2.6)
Contact: For questions regarding the catalog, please contact Chen Xu (xuchen[at]nao.cas.cn).

Important: This is not the published version provided by ApJS. We have added several extra columns for convenience, including Peak flux density, Notes, and internal IDs based on the original published table.

Columns

Column Unit Description
HGCN---Unique identifier in Hundred-deg² Galaxy Catalog
Name---Source name; format of Jhhmmss.s +ddmmss
HIRAdegdegFlux-weighted HI centroid right ascension (J2000)
HIDEdegdegFlux-weighted HI centroid declination (J2000)
OCRAdegdegRight ascension of most probable optical counterpart (J2000)
OCDEdegdegDeclination of most probable optical counterpart (J2000)
VHelkm/sHeliocentric HI velocity measured (1)
VOCkm/sHeliocentric velocity of optical counterpart
Zcmb---Redshift in the CMB reference frame
W50km/sHI line width at 50% of peak flux (1)
e_W50km/sUncertainty in W50
W20km/sHI line width at 20% of peak flux (1)
HIfluxJy km/sIntegrated HI flux
e_HIfluxJy km/sUncertainty in HIflux
SpeakmJyPeak flux density
RMSmJyRMS noise of spatially integrated HI spectrum
SNR---Signal-to-noise ratio
V85cogkm/sHI line width enclosing 85% of total flux (2)
e_V85cogkm/sUncertainty in V85cog
HIfluxcogJy km/sTotal HI (2)
e_HIfluxcogJy km/sUncertainty in HIfluxcog
SNRcog---Signal-to-noise ratio from curve-of-growth measurement
DisMpcDistance derived from Cosmicflows-4
logMHIsolMassLogarithm of HI mass in solar unit
e_logMHIsolMassUncertainty in logMHI
HIcode---HI detection category code; G=good, L=low S/N
OCcode---Optical counterpart category code (3)
PbestOC---Probability of the best optical counterpart
PbestOCRef---Reference optical survey used for counterpart matching
No.---Internal running sequence number
sofia_id---SoFiA source id
Notes---Additional notes just for reference

Notes

  • (1): By method given in Springob et al. 2005 [2005ApJS..160..149S].
  • (2): From curve-of-growth method in Yu et al. 2020 [2020ApJ...898..102Y].
  • (3): G = good; B = bad; C = confused; U = uncertain.