Kang, H. R. et al., 2018, Acta Astronomica Sinica, 59, 17 | View on ADS (2018AcASn..59...17K)
Pointing calibration and sub-reflector focusing are important task of antenna measurements, which significantly contribute to the observational performance of radio telescopes. According to the pointing accuracy and defocusing gain loss requirements of the 5 m Dome A Terahertz Explorer (DATE5), this paper has derived the requirements of signal-to-noise ratio for pointing and sub-reflector focusing calibration observations, and selected several astronomical radio sources suitable in terahertz band for pointing and focusing calibrations in Antarctica, which include planets and ultracompact HII regions. The effects of the atmospheric absorption and the source angular diameter on the calibration-measurement errors are analyzed. Simulations show that, when the telescope operates in Antarctica, these sources could provide sufficient flux density for verifying the pre-established pointing model and the focusing model.
This publication has been tagged as:
Characteristics/Other
Hemisphere/Antarctic
Site/Dome A (Kunlun Station)
Type/In-situ or ground-based observations
Type/Instrument design
Wavelength/Terahertz
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