Abstract
We have used the Five-hundred-meter Aperture Spherical radio Telescope (FAST) to conduct a blind ultradeep survey for neutral hydrogen (H i ). We present the complete results from the first of six fields (FUDS0). These observations of 95 hr allowed us to achieve a high-sensitivity (∼50 μ Jy beam −1 ) and a high-frequency resolution (22.9 kHz) over an area of 0.72 deg 2 . We detected 128 galaxies in H i distributed over the redshift range of 0 < z < 0.4, with H i masses in the range of 6.67 ≤ log ( M H I / h 70 − 2 M ⊙ ) ≤ 10.92 , and three faint high-velocity clouds, with a peak column density of N H i ≤ 3.1 × 10 17 cm −2 . Of the galaxies, 95 are new detections and six have z > 0.38, where no unlensed H i emission has previously been directly detected. Estimates of completeness and reliability are presented for the catalog. The consistency of continuum and H i flux estimates with the NRAO VLA Sky Survey and the Arecibo Ultra-Deep Survey, respectively, confirms the accuracy of the calibration method and data reduction pipeline developed for the full FAST Ultra-Deep Survey.
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CITATION STYLE
Xi, H., Peng, B., Staveley-Smith, L., For, B.-Q., Liu, B., & Ding, D. (2024). FAST Ultra-Deep Survey: Data Release for FUDS0. The Astrophysical Journal Supplement Series, 274(1), 18. https://doi.org/10.3847/1538-4365/ad67d5
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