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{{Short description|Observable quantity in imaging astronomical interferometry}} ...hase''' is an observable quantity in imaging [[astronomical interferometer|astronomical interferometry]], which allowed the use of [[Very Long Baseline Interferome ...

'''Kernel-phases''' are observable quantities used in high resolution astronomical imaging used for [[superresolution]] image creation.<ref name="kpfizeau">Ma [[Category:Astronomical imaging]] ...

...round. This shift is the apex angle in an [[isosceles triangle]], with 2 [[astronomical unit|AU]] (the distance between the extreme positions of Earth's orbit arou ...tars in the [[Milky Way]] disk, this corresponds to a mean baseline of 4 [[astronomical unit|AU]] per year, while for halo stars the baseline is 40 AU per year. Af ...

...Generally, transit time measurements are preferred for longer lengths, and interferometers for shorter lengths.<ref name=Yoshizawa/> ...to the idea behind the [[cosmic distance ladder]] for different ranges of astronomical length. Both calibrate different methods for length measurement using overl ...

|work=Gyros, Clocks, Interferometers ...: Testing Relativistic Gravity in Space == Gravitomagnetic fields of astronomical objects == ...

...ional-wave search''' refers to the use of extremely large [[Interferometry|interferometers]] built on the ground to passively detect (or "observe") [[gravitational wa ...ave observatory)|Cosmic Explorer]] forming a third generation. Space-borne interferometers such as [[Laser Interferometer Space Antenna|LISA]] are also planned, with ...

...: Laemmerzahl, C.; Everitt, C. W. F.; Hehl, F. W. (Eds.), ''Gyros, Clocks, Interferometers...: Testing Relativistic Gravity in Space''. Springer, Berlin, pp. 52–82, 2 == Astronomical evidence == ...

{{short description|Detection made by LIGO interferometers (2015)}} {{Infobox astronomical event ...

...high temperatures in the corona had previously been indicated by optical [[Astronomical spectroscopy|spectroscopy]] observations, but the idea remained controversi ...called [[aperture synthesis]]. Beginning in the 1950s, a number of simple interferometers were developed that could provide limited tracking of radio bursts.<ref nam ...

...Paris Observatory]] and proposed this unit of measurement to be called the astronomical radius (French: ''Rayon Astronomique'').<ref>{{Cite book |last=Picard |firs ...Polar Motion Service/International Latitude Service |journal=International Astronomical Union Colloquium |language=en |volume=178 |pages=147–162 |doi=10.1017/S0252 ...