Results 21 to 30 of about 69 (56)
Abstract With the ongoing transition for geodetic Very Long Baseline Interferometry (VLBI) from the use of legacy S/X telescopes to the VLBI Global Observing System (VGOS), it is necessary to connect the new VGOS network to the existing legacy S/X telescopes.
Rebekka Handirk +10 more
wiley +1 more source
Cross‐Polarization Gain Calibration of Linearly Polarized VLBI Antennas by Observations of 4C 39.25
Abstract Radio telescopes with dual linearly polarized feeds regularly participate in Very Long Baseline Interferometry. One example is the VLBI Global Observing System (VGOS), which is employed for high‐precision geodesy and astrometry. In order to achieve the maximum signal‐to‐noise ratio, the visibilities of all four polarization products are ...
F. Jaron +14 more
wiley +1 more source
Prototype System for Unmanned Reference Point Determination at the Sub‐Millimeter Level
Abstract The determination of reference points for telescopes is crucial for obtaining the local‐tie vector for a multi‐technology co‐located station. Traditional methods suffer from labor‐intensive fieldwork, long execution cycles, and systematic errors due to the incident angle of the total station's laser beam on the prism. In this paper, we propose
Zhibin Zhang +7 more
wiley +1 more source
A Modular Approach for the Design of Quadruple Ridged Flared Horn Antenna Feeds
This paper presents the methodology followed for the design of a quad-ridged flared horn (QRFH) feed for the VLBI Global Observing System (VGOS) antennas.
Oscar Garcia-Perez +6 more
doaj +1 more source
Optimizing VGOS observations using an SNR-based scheduling approach
The geodetic and astrometric very long baseline interferometry (VLBI) community is in the process of upgrading its existing infrastructure with the VLBI Global Observing System (VGOS). The primary objective of VGOS is to substantially boost the number of
Matthias Schartner +8 more
doaj +1 more source
Irregularities in the Earth’s rotation speed are quantified by the difference between Universal Time (UT1) and Coordinated Universal Time (UTC).
Arnab Laha +6 more
doaj +1 more source
Optimal distribution of VLBI transmitters in the Galileo space segment for frame ties. [PDF]
Wolf H, Böhm J.
europepmc +1 more source
The Australian mixed-mode observing program. [PDF]
McCallum L +9 more
europepmc +1 more source
Inter-Comparison of UT1-UTC from 24-Hour, Intensives, and VGOS Sessions during CONT17. [PDF]
Raut S +5 more
europepmc +1 more source
Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination. [PDF]
Böhm S +8 more
europepmc +1 more source

