Results 111 to 120 of about 56,169 (259)

Astronomy using basic Mark 2 very long baseline interferometry [PDF]

open access: yes
Two experiments were performed in April and September 1976 to determine precise positions of radio sources using conventional Mark 2 VLBI techniques. Four stations in the continental United States observed at a wavelength of 18 cm.
Backer, D. C.   +3 more
core   +1 more source

Probing the close environment of young stellar objects with interferometry

open access: yes, 2003
The study of Young Stellar Objects (YSOs) is one of the most exciting topics that can be undertaken by long baseline optical interferometry. The magnitudes of these objects are at the edge of capabilities of current optical interferometers, limiting the ...
A Natta   +36 more
core   +2 more sources

Improved geodetic European very-long-baseline interferometry solution using models of antenna gravitational deformation

open access: yesAnnals of Geophysics, 2010
Very-long-baseline interferometry (VLBI) is used for establishing global geodetic networks where the coordinates attain a 1-mm level of precision. Technique-dependent bias can degrade the VLBI positioning accuracy if it is present and unaccounted for ...
Claudio Abbondanza   +2 more
doaj   +1 more source

Experience from geodetic very long baseline interferometry observations at Onsala using a digital backend

open access: yesJournal of Geodetic Science, 2015
The Onsala Space Observatory has installed a modern digital backend for geodetic and astronomical Very Long Baseline Interferometry (VLBI). This system consists of a Digital Base-Band Converter (DBBC) and a Mark 5B+ recorder.
Kareinen N., Haas R.
doaj   +1 more source

Time-lapse Very Long Baseline Interferometry Imaging of the Close Active Binary HR 1099

open access: yesThe Astrophysical Journal
We report multiepoch astrometric very long baseline interferometry observations of the chromospherically active binary HR 1099 (V711 Tau, HD 22468) at six epochs over 63 days using the Very Long Baseline Array at 22.2 GHz.
Walter W. Golay   +2 more
doaj   +1 more source

Solar VLBI [PDF]

open access: yes
In April, 1981, radio telescopes at Dwingeloo (The Netherlands) and Onsala (Sweden) were used as a long-baseline interferometer at a wavelength of 18 cm. The baseline of 619 km gave a spatial resolution on the Sun of about 45 km.
Kuijpers, J., Tapping, K. F.
core   +1 more source

Evolution of the Termination Region of the Parsec-scale Jet of 3C 84 Over the Past 20 yr

open access: yesThe Astrophysical Journal
We present the kinematics of the parsec-scale jet in 3C 84 from 2003 November to 2022 June observed with the Very Long Baseline Array at 43 GHz. We find that the C3 component, a bright feature at the termination region of the jet component ejected from ...
Minchul Kam   +6 more
doaj   +1 more source

Very long baseline interferometry using a radio telescope in Earth orbit [PDF]

open access: yes
Successful Very Long Baseline Interferometry (VLBI) observations at 2.3 GHz were made using an antenna aboard an Earth-orbiting spacecraft as one of the receiving telescopes.
Edwards, C. D.   +2 more
core   +1 more source

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

open access: yesThe Astrophysical Journal
The mergers of double neutron star (DNS) systems are believed to drive the majority of short γ -ray bursts (SGRBs), while also serving as production sites of heavy r -process elements.
Hao Ding   +5 more
doaj   +1 more source

An accuracy assessment of Magellan Very Long Baseline Interferometry (VLBI) [PDF]

open access: yes
Very Long Baseline Interferometry (VLBI) measurements of the Magellan spacecraft's angular position and velocity were made during July through September, 1989, during the spacecraft's heliocentric flight to Venus. The purpose of this data acquisition and
Border, J. S.   +2 more
core   +1 more source

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