Results 41 to 50 of about 9,059 (229)

Astrometric Apparent Motion of High-redshift Radio Sources

open access: yesThe Astronomical Journal, 2023
Radio-loud quasars at high redshift ( z ≥ 4) are rare objects in the universe and rarely observed with Very Long Baseline Interferometry (VLBI). But some of them have flux density sufficiently high for monitoring of their apparent position.
Oleg Titov   +12 more
doaj   +1 more source

A Concept of Precise VLBI/GNSS Ties with Micro-VLBI

open access: yes, 2023
AbstractWe present here a concept of measuring local ties between collocated GNSS and VLBI stations using the microwave technique that effectively transforms a GNSS receiver to an element of a VLBI network. This is achieved by modifying the signal chain that allows to transfer voltage of the GNSS antenna to a digitizer via a coaxial cable.
Leonid Petrov   +5 more
openaire   +1 more source

VLBI Observations of the Nucleus of Centaurus A [PDF]

open access: yesSymposium - International Astronomical Union, 1982
VLBI observations of the nucleus of Centaurus A have been made at three southern hemisphere observatories. Since Centaurus A is the nearest active galaxy, VLBI investigations are important because the physical processes in the nucleus can be studied in greater linear detail than in other similar galaxies.
R. A. Preston   +7 more
openaire   +1 more source

VLBI Activities in Japan and a Projected Space-VLBI Program [PDF]

open access: yesSymposium - International Astronomical Union, 1988
There are three institutes in Japan that are equipped with VLBI facilities. Of these, Nobeyama Radio Observatory started VLBI experiments with astrophysical and astrometric interests. The Institute of Space and Astronautical Science, the Nobeyama Radio Observatory, and the Radio Research Laboratory collaborated with JPL and other institutions for this ...
openaire   +1 more source

Japanese VLBI Project — Vera [PDF]

open access: yesSymposium - International Astronomical Union, 1988
The Japanese VLBI project VERA (VLBI for the Earth Rotation study and Astrometry) is being designed. It will be dedicated to regular monitoring of the Earth's rotation and astrometry. VERA will be composed of two antennas spanning about 2300km and a correlator of multi-station capability. The diameters of the antennas are 35m and 15m.
Mitsumi Fujishita, Tadayoshi Hara
openaire   +1 more source

An Experiment on Radio Location of Objects in the Near-Earth Space with VLBI in 2012

open access: yesOpen Astronomy, 2013
An experiment on radar location of space debris objects using of the method of VLBI was carried out in April, 2012. The radar VLBI experiment consisted in irradiation of some space debris objects (4 rocket stages and 5 inactive satellites) with a signal ...
Nechaeva M.   +20 more
doaj   +1 more source

Space VLBI [PDF]

open access: yesSymposium - International Astronomical Union, 2001
Space VLBI enables high angular resolution and high dynamic range imaging through an extension of ground-based VLBI. The TDRSS space VLBI experiments in the 1980s were followed by the first space VLBI imaging mission, VSOP, in the 1990s. The new century holds the promise of the VSOP-2 and ARISE missions, which aim for more sensitive, higher angular ...
openaire   +1 more source

First proof of concept of remote attendance for future observation strategies between Wettzell (Germany) and Concepción (Chile) [PDF]

open access: yes, 2010
Current VLBI observations are controlled and attended locally at the radio telescopes on the basis of pre-scheduled session files. Operations have to deal with system specific station commands and individual setup procedures.
Hase, H   +9 more
core  

MSWD: A Hybrid Machine‐Learning Framework for Slant Wet Delay Modeling

open access: yesJournal of Geophysical Research: Atmospheres, Volume 131, Issue 12, 28 June 2026.
Abstract Space geodetic techniques such as Global Navigation Satellite Systems (GNSS) and Very Long Baseline Interferometry (VLBI) are limited by direction‐dependent tropospheric delays, with slant wet delay (SWD) being the most variable component and a major error source.
Zhenyi Zhang, Benedikt Soja
wiley   +1 more source

Shanghai VLBI Correlator [PDF]

open access: yes, 2013
This report summarizes the activities of the Shanghai VLBI Correlator during ...
Fengchun Shu   +5 more
core   +1 more source

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