Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
USNO
U. S. Naval Observatory, USA
USNO;
US Naval Observatory
Iowa, University, Iowa City
NRL
U.S. Naval Research Lab., Washington, DC, US
US Naval Observatory, 3450 Massachusetts Avenue, NW, Washington, DC 20392-5420.
Iowa, University, Iowa City; U.S. Navy, Naval Research Laboratory, Washington, DC
U.S. Naval Observatory
United States Naval Observatory, 3450 Massachusetts Avenue NW, Washington, DC 20392-5420
U.S. Naval Obs.
US Naval Observatory, Washington DC, USA
U.S. Naval Observatory 3450 Massachusetts Ave., NW, Washington, DC 20392-5420, USA
US Naval Observatory, Code EO, 3450 Massachusetts Avenue, NW, Washington, DC 20392-5420
University of Tasmania, Hobart, Australia
U.S. Naval Observatory, Earth Orientation Department, 3450 Massachusetts Ave., Washington, DC 20392, USA
United States Naval Observatory, Washington, D.C., USA
US Naval Observatory, Washington, DC, USA
USNO, Washington DC, USA
US Naval Observatory, 3450 Massachusetts Avenue, NW, Washington, DC 20392-5240
U.S. Naval Observatory, 3450 Massachusetts Ave., NW, Washington, DC 20392-5420, USA
United States Naval Observatory, 3450 Massachusetts Avenue, NW, Washington, DC 20392-5420
US Naval Observatory, 3450 Massachusetts Avenue NW, Washington, DC 20392-5420 Navy, Naval Research Laboratory, Washington, DC
United States Naval Observatory, 3450 Massachusetts Avenue NW, Washington, DC 20392-5420.
US Naval Observatory, 3450 Massachusetts Avenue, NW, Washington, DC 20392-5420 Research Lab., Washington, DC, US
U.S. Naval Observatory, 3450 Massachusetts Avenue NW, Washington, DC 20392-5420 Navy, Naval Research Lab., Washington
Naval Research Laboratory, Washington, DC, US
15 GHz VLA observations of the radio galaxies 3C 166 and 3C 411
608 MHz VLBI Observations of 2050 + 364: Constraints on Interstellar Scattering
608 MHz VLBI observations of the compact double radio source 2050 + 364 - Constraints on interstellar scattering
A Classification of ICRF Sources Based on Observed Structure for Ultra-precise VLBI Astrometry and Geodesy.
A radio optical reference frame. 7: Additional source positions from a Southern hemisphere short baseline survey
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