1. Sun fringe at 660 MHz
2. Sun fringe at 460 MHz
3. Tau A fringe at 460 MHz
4. Cyg A fringe at 660 MHz

• Site: Fuguei
• Notes: 4 antennas in a row with a separation of $\sim$ 2 meters from each other

• Observation date: 2022.12.22 04:00 UT (12:00 CST; 3 hours)

baseline 0-1

baseline 0-2

baseline 0-3

baseline 1-2

baseline 1-3

baseline 2-3

• Nmodes = 1, 2, 3

baseline 0-1

baseline 0-2

baseline 0-3

baseline 1-2

baseline 1-3

baseline 2-3

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• Observation date: 2022.12.22 01:00 UT (09:00 CST; 3 hours)
• Only the data for the first 4500 sec were processed.

baseline 0-1

baseline 0-2

baseline 0-3

baseline 1-2

baseline 1-3

baseline 2-3

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• Site: Fuguei
• Notes: 4 antennas in a row with a separation of $\sim$ 2 meters from each other Both 460 MHz and 660 MHz were recorded, but there is something wrong with 660 MHz. The 660 MHz data is being checked.

• Observation date: 2023.01.13 11:00 UT (3 hours)

baseline 0-1

baseline 0-2

baseline 0-3

baseline 1-2

baseline 1-3

baseline 2-3

• Nmodes = 1, 2, 3

baseline 0-1

baseline 0-2

baseline 0-3

baseline 1-2

baseline 1-3

baseline 2-3

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• Site: Fuguei
• Observation date:
    2023-03-08 22:00 UT (06:00+1 CST) (460 MHz)
    2023-03-10 22:00 UT (06:00+1 CST) (660 MHz)
• Notes:
   * Search for the coarse delay does not give a constant value for both frequencies.
   * Fringe searching with an integration time of 60 sec does not work (Being checked)

• It turned out that the reference clock is unlocked, so the previous results were commented out.

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