Design and characterization of W-band and D-band calibration sources for the AliCPT-1 experiment

Authors:
  • AZAi-Mei Zhang
    Ai-Mei Zhang
  • ZLZheng-Wei Li
    Zheng-Wei Li
  • XLXue-Feng Lu
    Xue-Feng Lu
  • ZXZhong-Xue Xin
    Zhong-Xue Xin
  • GWGuo-Feng Wang
    Guo-Feng Wang
  • YLYong-Ping Li
    Yong-Ping Li
  • YZYong-Jie Zhang
    Yong-Jie Zhang
  • SSShi-Bo Shu
    Shi-Bo Shu
  • YZYi-Fei Zhang
    Yi-Fei Zhang
  • YLYa-Qiong Li
    Ya-Qiong Li
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Abstract
Ali Cosmic Microwave Background Polarization Telescope (AliCPT-1) is the first Chinese cosmic microwave background experiment aiming to make sensitive polarization maps of the potential B-mode signal from inflationary gravitational waves. The telescope was deployed on the Tibet Ali site at 5250 m above sea level in early 2025. Before and after each observation season, the instrument performance must be carefully calibrated, including the far field beam performance, far sidelobe, spectral response, polarization angle, and cross-polar beam response. To characterize these optical performances, several calibrators have been developed. We developed a W-band source and a D-band source for the AliCPT-1 telescope's beam characterizations. We present the design and performance of the two calibration sources.

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