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- Fringe test between PV and NOEMA at 3mm
- Done with the EHT setup 4x2GHz dual-pol
- PV with 2-of-4 x R2DBE and 1 x DBBC3; on sky demonstration of DBBC3 GMVA fringes
- PV had poor IF bandpass equalization, and
e.g., scan No0028 SNR~450 over 2x512MHz improves to SNR~630 with 32x64MHz zoomsNOEMA had low optical power in parts of Rx LSB
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Version from 12:39, 12 Feb 2020
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- Fringe test between PV and NOEMA at 3mm
- Done with the EHT setup 4x2GHz dual-pol
- PV with 2-of-4 x R2DBE and 1 x DBBC3; on sky demonstration of DBBC3 GMVA fringes
- PV poor IF bandpass equalization,
e.g., scan No0028 SNR~450 over 2x512MHz improves to SNR~630 with 32x64MHz zooms - NOEMA had low optical power in parts of Rx LSB
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Version as of 12:44, 12 Feb 2020
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- Fringe test between PV and NOEMA at 3mm
- Done with the EHT setup 4x2GHz dual-pol
- PV with 2-of-4 x R2DBE and 1 x DBBC3; on sky demonstration of DBBC3 GMVA fringes
- PV had poor IF bandpass equalization, and NOEMA had low optical power in parts of Rx LSB
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