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...aselines]]. It forms the basis of the '''self-calibration''' approach to [[interferometric imaging]]. The observable which is usually used in most "closure phase" obs [[Image:Recording data at each of the telescopes in a VLBI array.gif|thumb|400px|Three radio telescope receivers.]] ...

...and Real-time Analysis eXperiment''' ('''HIRAX''') is an [[interferometry|interferometric]] array of 1024 6-[[meter]] (20[[Foot (unit)|ft]]) diameter [[radio telesco |series = Ground-based and Airborne Telescopes VI ...

...ibution function of a distant, incoherent source is equal to its complex [[Interferometric visibility|visibility]].<ref>{{cite book |title=Modern Classical Optics |au ...of coherence]] at different points in the imaging plane (the so-called "[[interferometric visibility|visibility]] function") of an astronomical object, a radio astro ...

| title=MAST: Barbara A. Mikulski Archive for Space Telescopes ...|date=2024-09-01 |title=Study of the <var>μ</var> Cet Binary with Speckle Interferometric, Photometric, and Spectroscopic Techniques |journal=Astrophysical Bulletin ...

'''Ground-based interferometric gravitational-wave search''' refers to the use of extremely large [[Interfe ...=Patrice |url=https://inspirehep.net/literature/429042 |title=Couplings in interferometric gravitational wave detectors |date=December 1996 |year=1996}}</ref> Yet, se ...

...10173 |last1=Caleb |first1= M.|author1-link=Manisha Caleb |title=The first interferometric detections of Fast Radio Bursts| journal= Monthly Notices of the Royal Astr ...RB 150418 was detected by the Parkes observatory and within hours, several telescopes including the [[Australia Telescope Compact Array]] caught an apparent radi ...