Results 71 to 80 of about 424 (141)
Scintillation Properties of PSR B1133+16 Measured with Very Long Baseline Interferometry
The scintillation of pulsars reveals the small-scale structure of the interstellar medium. A powerful technique for characterizing the scintillating structures (screens) combines analysis of scintillation arcs and very long baseline interferometry (VLBI).
Ashley M. Stock +5 more
doaj +1 more source
First Very Long Baseline Interferometry Detections at 870 μm
The first very long baseline interferometry (VLBI) detections at 870 μ m wavelength (345 GHz frequency) are reported, achieving the highest diffraction-limited angular resolution yet obtained from the surface of the Earth and the highest-frequency ...
Alexander W. Raymond +278 more
doaj +1 more source
Blazar jets imaged with Very Long Baseline Interferometry (VLBI) - kinematics of helical trajectories in 3C273 and 3C345 [PDF]
In this work a large collection of VLBI (Very Long Baseline Interferometry) maps are presented based upon data from the VLBA (Very Long Baseline Array) for 29 sources. The maps are the result of three epochs of imaging. A kinematic study was undertaken with a view to understanding some interesting structure seen in the quasars 3C273 and 3C345 ...
openaire
RadioAstron reveals a change in the jet collimation profile of 3C 84
Context. Due to its brightness and proximity, the radio galaxy 3C 84 (optical counterpart NGC 1275 in the Perseus cluster) has been the target of extensive studies investigating the central parsec region of its active galactic nucleus.
Benke P. +7 more
doaj +1 more source
Prospects of Detecting a Jet in Sagittarius A* with Very-long-baseline Interferometry
Event Horizon Telescope (EHT) images of the horizon-scale emission around the Galactic center supermassive black hole Sagittarius A* (Sgr A*) favor accretion flow models with a jet component. However, this jet has not been conclusively detected.
Erandi Chavez +5 more
doaj +1 more source
Automated Modeling with AAP-Imfit: Astrometry and Photometry via CASA
Very long baseline interferometry (VLBI) provides the highest-resolution radio intensity maps, crucial for detailed studies of compact sources like active galactic nuclei (AGNs) and their relativistic jets.
Alfredo Amador-Portes +5 more
doaj +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
Baseline-dependent clock offsets in VLBI data analysis. [PDF]
Krásná H +4 more
europepmc +1 more source

