The high optical brightness of the BlueWalker 3 satellite. [PDF]
Nandakumar S +39 more
europepmc +1 more source
Exploring nine simultaneously occurring transients on April 12th 1950. [PDF]
Villarroel B +8 more
europepmc +1 more source
Dynamical Mass of the Ophiuchus Intermediate-mass Stellar System S1 with DYNAMO-VLBA
We report dynamical mass measurements of the individual stars in the most luminous and massive stellar member of the nearby Ophiuchus star-forming region, the young tight binary system S1.
Jazmín Ordóñez-Toro +10 more
doaj +1 more source
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Caleb M +21 more
europepmc +1 more source
A VLBI Software Correlator for Fast Radio Transients
One major goal in fast radio burst science is to detect fast radio bursts (FRBs) over a wide field of view without sacrificing the angular resolution required to pinpoint them to their host galaxies.
Calvin Leung +16 more
doaj +1 more source
The Celestial Frame and the Weighting of the Celestial Pole Offsets in the Computation of VLBI-Based Corrections for the Main Lunisolar Nutation Terms. [PDF]
Puente V, Folgueira M.
europepmc +1 more source
From reference frames to relativistic experiments: Absolute and relative radio astrometry
25 pages, 7 figures--Presented at JENAM meeting in Budapest, 27-30 August ...
openaire +2 more sources
Submillimeter Observations of the White Dwarf Pulsar AR Sco
AR Scorpii, the so-called white dwarf (WD) pulsar, contains a rapidly rotating magnetic WD ( P _spin = 117.0564 s) interacting with a cool, red dwarf (RD) companion in a 3.56 hr orbit. It is a strong radio source with an inverted spectral index between 1
Paul E. Barrett, Mark A. Gurwell
doaj +1 more source
The Very Long Baseline Interferometry Global Observing System (VGOS), a global network of stations equipped with small-diameter, fast-slewing antennas and broadband receivers, is primarily utilized for geodesy and astrometry.
Jiangying Gan +5 more
doaj +1 more source
Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination. [PDF]
Böhm S +8 more
europepmc +1 more source

