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The closure phase is an observable quantity in imaging astronomical interferometry, which allowed the use of interferometry with very long baselines. It forms the basis of the self-calibration approach to interferometric imaging. The observable which is usually used in most "closure phase" observations is actually the complex quantity called the triple…
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phase closure displaystyle complex interferometry used phases antennas quantity astronomical baselines observable imaging errors optical radio three source signal long
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Closure phase | is a | observable quantity in imaging astronomical interferometry | 0.90 | text |
| Closure phase | is a | phase | 0.90 | text |
| the Very Long Baseline Array | instance of | The radio signals received are recorded onto magnetic tapes and sent to a laboratory | 0.80 | text |
| Closure phase | has application | Aperture | 0.60 | section |
| Closure phase | has application | Kernel-phases | 0.60 | section |
| Closure phase | related to Definition | In | 0.60 | section |
| Closure phase | related to Definition | The | 0.60 | section |
| Closure phase | related to Definition | Very Long Baseline Array | 0.60 | section |
| Closure phase | related to Definition | When | 0.60 | section |
| Closure phase | related to Definition | Taking | 0.60 | section |
| Closure phase | related to Definition | Fourier | 0.60 | section |
| Closure phase | related to Definition | These | 0.60 | section |
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