There are three ways to determine the field distortion produced by astronomical telescopes: a) the direct comparison of measured coordinates with theoretical coordinates derived of an astrometrical catalog of high precision: b) the analysis of the ...
Maria Jeanette Stock Leyton +2 more
doaj
VLBA Astrometry of the Galactic Double Neutron Stars PSR J0509+3801 and PSR J1930-1852: A Preliminary Transverse Velocity Distribution of Double Neutron Stars and Its Implications [PDF]
Ding Hao +5 more
openalex +1 more source
Improving catalogue matching by supplementing astrometry with additional photometric information [PDF]
Tom J. Wilson, T. Naylor
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Astrometry, orbit determination, and thermal inertia of the Tianwen-2 target asteroid (469219) Kamo`oalewa [PDF]
Marco Fenucci +11 more
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Constraining the properties of HD 206893 B. A combination of radial velocity, direct imaging, and astrometry data [PDF]
A. Grandjean +27 more
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The IAU 2000 Resolutions for Astrometry, Celestial Mechanics, and Metrology in the Relativistic Framework: Explanatory Supplement [PDF]
M. Söffel +19 more
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Erratum: Light propagation in the gravitational field of
Sven Zschocke
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Challenges and opportunities for time-delay cosmography with multi-messenger gravitational lensing. [PDF]
Birrer S +4 more
europepmc +1 more source
Hayabusa2 extended mission target asteroid 1998 KY<sub>26</sub> is smaller and rotating faster than previously known. [PDF]
Santana-Ros T +18 more
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