The HD^2 Pilot Survey Extragalactic HI Source Catalog

Description

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-Deg^2^ HI Deep (HD^2^) 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.

Version: Pre-release (2026/05, v2.6)

Contact: For questions regarding the catalog, please contact Chen Xu (xuchen@nao.cas.cn).

Columns

Column Unit Description
HGCN Unique identifier in Hundred-deg² Galaxy Catalog
Name Source name; format of Jhhmmss.s +ddmmss
HIRAdeg deg Flux-weighted HI centroid right ascension (J2000)
HIDEdeg deg Flux-weighted HI centroid declination (J2000)
OCRAdeg deg Right ascension of most probable optical counterpart (J2000)
OCDEdeg deg Declination of most probable optical counterpart (J2000)
VHel km/s Heliocentric HI velocity measured (1)
VOC km/s Heliocentric velocity of optical counterpart
Zcmb Redshift in the CMB reference frame
W50 km/s HI line width at 50% of peak flux (1)
e_W50 km/s Uncertainty in W50
W20 km/s HI line width at 20% of peak flux (1)
HIflux Jy km/s Integrated HI flux
e_HIflux Jy km/s Uncertainty in HIflux
Speak mJy Peak flux density
RMS mJy RMS noise of spatially integrated HI spectrum
SNR Signal-to-noise ratio
V85cog km/s HI line width enclosing 85% of total flux (2)
e_V85cog km/s Uncertainty in V85cog
HIfluxcog Jy km/s Total HI (2)
e_HIfluxcog Jy km/s Uncertainty in HIfluxcog
SNRcog Signal-to-noise ratio from curve-of-growth measurement
Dis Mpc Distance derived from Cosmicflows-4
logMHI solMass Logarithm of HI mass in solar unit
e_logMHI solMass Uncertainty 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 Sp05 [2005ApJS..160..149S].

(2): From curve-of-growth method in Yu20 [2020ApJ…898..102Y].

(3): G = good; B = bad; C = confused; U = uncertain.

2026/05/22, NAOC-CCG