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HiFAST: An Hi data calibration and imaging pipeline for FAST

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Abstract

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has the largest aperture and a 19-beam L-band receiver, making it powerful for investigating the neutral hydrogen atomic gas (Hi) in the universe. We present HiFAST (https://hifast.readthedocs.io), a dedicated, modular, and self-contained calibration and imaging pipeline for processing the Hi data of FAST. The pipeline consists of frequency-dependent noise diode calibration, baseline fitting, standing wave removal using an FFT-based method, flux density calibration, stray radiation correction, and gridding to produce data cubes. These modules can be combined as needed to process the data from most FAST observation modes: tracking, drift scanning, On-The-Fly mapping, and most of their variants. With HiFAST, the root-mean-square (RMS) noises of the calibrated spectra from all 19 beams were only slightly (∼5%) higher than the theoretical expectation. The results for the extended source M33 and the point sources are consistent with the results from Arecibo. The moment maps (0, 1 and 2) of M33 agree well with the results from the Arecibo Galaxy Environment Survey (AGES) with a fractional difference of less than 10%. For a common sample of 221 sources with signal-to-noise ratio S/N > 10 from the Arecibo Legacy Fast ALFA (ALFALFA) survey, the mean value of fractional difference in the integrated flux density, Sint, between the two datasets is approximately 0.005%, with a dispersion of 15.4%. Further checks on the integrated flux density of 23 sources with seven observations indicate that the variance in the flux density of the source with luminous objects (Sint > 2.5 Jy km s−1) is less than 5%. Our tests suggest that the FAST telescope, with the efficient, precise, and user-friendly pipeline HiFAST, will yield numerous significant scientific findings in the investigation of the Hi in the universe.

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Correspondence to Yingjie Jing.

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This work was supported by the National Key R&D Program of China (Grant No. 2022YFA1602901), the National Natural Science Foundation of China (Grant Nos. 11988101, 11873051, 12125302, and 12373011), the CAS Project for Young Scientists in Basic Research Grant (Grant No. YSBR-062), the K. C. Wong Education Foundation, and the science research grants from the China Manned Space Project. Yingjie Jing acknowledges support from the Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS. We would like to express our gratitude to Prof. Rendong Nan and his team for their groundbreaking efforts in establishing the FAST telescope. Additionally, we would like to acknowledge the FAST operation team for their invaluable assistance and support in the development of this pipeline. We also thank Martha P. Haynes for generously sharing ALFALFA spectra data and insightful discussions on source flux calculations, which significantly enhanced our study. This work made use of the data from FAST (Five-hundred-meter Aperture Spherical radio Telescope). FAST is a Chinese national mega-science facility, operated by National Astronomical Observatories, Chinese Academy of Sciences.

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Jing, Y., Wang, J., Xu, C. et al. HiFAST: An Hi data calibration and imaging pipeline for FAST. Sci. China Phys. Mech. Astron. 67, 259514 (2024). https://doi.org/10.1007/s11433-023-2333-8

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  • DOI: https://doi.org/10.1007/s11433-023-2333-8