Results 21 to 30 of about 909 (203)
RADIO ASTROMETRY OF THE CLOSE ACTIVE BINARY HR 5110 [PDF]
The close active binary HR 5110 was observed at six epochs over 26 days using a global VLBI array at 15.4~GHz. We used phase-referencing to determine the position of the radio centroid at each epoch with an uncertainty significantly smaller than the component separation.
Abbuhl, E. +3 more
openaire +4 more sources
Abstract This paper describes the design, implementation, and field‐testing of a low‐cost autonomous control system on the Platform for Expanding Autonomous Underwater Vehicles (AUV) exploRation to Longer ranges (PEARL). PEARL is a floating, solar‐powered platform designed as a servicing station for AUVs.
Ethan S. Rolland +2 more
wiley +1 more source
Radio astrometry is now the premier astrometric technique for measuring the positions of celestial objects. The precision with which absolute positions can be determined is approaching a few milliarc-seconds. The progress towards establishing an almost inertial reference frame based upon the positions of extragalactic radio sources is reviewed as of ...
openaire +1 more source
The Use of the Ratan-600 Radio Telescope in Astrometry [PDF]
The RATAN-600 radio telescope (Kaidanovsky & al. 1972) was designed for solving various problems of astrophysics and radiophysics (Pariisky & al. 1972, Gelfreikh & al. 1972). Because of its high resolving power and large collecting area, this instrument can be used to measure accurate positions of radio sources.
P. M. Afanasieva +5 more
openaire +1 more source
Abstract We report the results of position ties for short baselines at eight geodetic sites based on phase delays that are extracted from global geodetic very‐long‐baseline interferometry (VLBI) observations rather than dedicated short‐baseline experiments.
Ming H. Xu +13 more
wiley +1 more source
Photographic astrometry of radio stars [PDF]
Photographic astrometry of four radio stars has been carried out in a test program using the Wide Field Camera at the f/8 focus of the Jacobus Kapteyn Telescope (JKT). The accuracy of the positions is 0.04 arcsec. Comparisons are made with positions obtained by the Carlsberg and Bordeaux automatic meridian circles and with the radio positions measured ...
R. W. Argyle +3 more
openaire +1 more source
Optical and radio astrometry of the galaxy associated with FRB 150418 [PDF]
Abstract A fading radio source, coincident in time and position with the fast radio burst FRB 150418, has been associated with the galaxy WISE J071634.59−190039.2. Subsequent observations of this galaxy have revealed that it contains a persistent, but variable, radio source. We present e-Multi-Element Radio Linked Interferometer Network,
Bassa, C. G. +12 more
openaire +6 more sources
Radio and Optical Astrometry [PDF]
Radio positional measurements have achieved an accuracy as high as that of optical astrometry, with uncertainties no greater than a few hundredths of an arc second in each coordinate. Declinations and relative right ascensions are determined absolutely.
openaire +1 more source
VLBI astrometry on the white dwarf pulsar AR Scorpii [PDF]
AR Scorpii (AR Sco), the only-known radio-pulsing white dwarf binary, shows unusual pulsating emission at the radio, infrared, optical, and ultraviolet bands.
Cao, Hongmin +14 more
core +1 more source
S˜ìvÑRALS : outhern hemisphere parallax interferometric radio astrometry legacy survey
The exact structure of the spiral arms of our home Galaxy, the Milky Way, is an unknown that can be resolved by a higher sampling of parallaxes to high mass star-forming regions from both the Northern and Southern Hemispheres. The Northern Hemisphere has
Lucas Hyland (14739874)
core +1 more source

