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| [[Global mm-VLBI Array]] (successor to the ''Coordinated Millimeter VLBI Array'')|| || 0.000012 (12 μas)|| radio (at 1.3 cm) || [[very long baseline interferometry]] array of different [[radio telescope]]s || a range of locations on Earth and in space<ref name="Max Planck Institute for Radio Astronomy 2022">{{cite web | title=Images at the Highest Angular Resolution in Astronomy | website=Max Planck Institute for Radio Astronomy | date=2022-05-13 | url=https://www.mpifr-bonn.mpg.de/pressreleases/2022/2 | access-date=2022-09-26}}</ref> || 2002 -
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| [[Very Large Telescope]]/[[PIONIER (VLTI)|PIONIER]]|| [[File:Paranal and the Pacific at sunset (dsc4088, retouched, cropped).jpg|50px]] || 0.001 (1 mas)|| light (1-2 [[micrometre]])<ref name="de Zeeuw p. ">{{cite journal | last=de Zeeuw | first=Tim | title=Reaching New Heights in Astronomy - ESO Long Term Perspectives | journal=The Messenger | year=2017 | volume=166 | arxiv=1701.01249 | page=2| bibcode=2016Msngr.166....2D }}</ref> || largest [[optical astronomy|optical]] array of 4 [[reflecting telescope]]s || [[Paranal Observatory]], [[Antofagasta Region]], Chile || 2002/2010 -
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| [[Hubble Space Telescope]]|| [[File:HST.jpg|50px]] || 0.04 || light (near 500 nm)<ref name="NASA 2007">{{cite web | title=Hubble Space Telescope | website=NASA | date=2007-04-09 | url=https://www.nasa.gov/missions/highlights/webcasts/shuttle/sts109/hubble-qa.html#:~:text=In%20visible%20light%20(at%20wavelengths,by%20about%2040%20arc%20seconds. | access-date=2022-09-27}}</ref> || [[space telescope]] || [[Geocentric orbit|Earth orbit]] || 1990 -
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