Results 101 to 110 of about 758 (152)
VGOS Phase Cal Performance at High Frequencies
Since 2019, VGOS observations have routinely been carried out using the same frequency setup with a range from 3 to 10.7 GHz. Employing a network of European VGOS stations, we carried out experiments testing four alternative frequency setups covering the
Bernhart, Simone +1 more
core +2 more sources
FUKASE, Satoshi, MARUYAMA, Fumio
openaire +2 more sources
With the VLBI Global Observing System (VGOS) being the next step in the development of geodetic Very Long Baseline Interferometry (VLBI), it is necessary to connect the new VGOS network to existing legacy S/X telescopes. Specially designed short-baseline
Handirk, Rebekka,
core
Going to School on a Robot: Robot and User Interface Design Features That Matter. [PDF]
Ahumada-Newhart V, Olson JS.
europepmc +1 more source
New VLBI2010 scheduling strategies and implications on the terrestrial reference frames. [PDF]
Sun J +5 more
europepmc +1 more source
Satellite estimation of global air sea CO<sub>2</sub> flux from 2000 to 2020. [PDF]
Ji Y +5 more
europepmc +1 more source
Impact of the terrestrial reference frame on the determination of the celestial reference frame. [PDF]
Karbon M, Belda S, Nilsson T.
europepmc +1 more source
Combining legacy S/X and broadband VGOS VLBI networks by mixed-mode observations
American Geophysical Union Meeting (AGU23), 11-15 December 2023, San FranciscoA network of VLBI stations has been observing in the legacy S/X frequency bands for more than 40 years.
Cappallo, Roger J. +8 more
core
Observing APOD with the AuScope VLBI Array. [PDF]
Hellerschmied A +5 more
europepmc +1 more source
Microwave-Assisted Desilication as a Route to Hierarchical Y Zeolites: Linking Pore Architecture, Acidity, and Catalytic Stability in VGO Cracking. [PDF]
Fals J +4 more
europepmc +1 more source

