2-6 September 2024
CJD Bonn Castell
Europe/Berlin timezone
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Session XVI: VLBI perspectives II -- Chair: Zsolt Paragi

Place

Location: CJD Bonn Castell
Address: Graurheindorfer Str. 149, 53117 Bonn
Date: 6 Sep 09:00 - 10:45

Description

30 min Invited talk on GMVA 4x15min contributed talks

Timetable | Contribution List

Displaying 6 contributions out of 6
The BRAND receiver is a new system mainly intended for the EVN that covers the remarkably broad contiguous frequency range of 1.5 GHz to 15.5 GHz. It includes all required components of the entire signal path from the cryogenic frontend, feed, amplifiers, hybrids, the 56 Gsps sampler up to the VLBI backend and is intended for VLBI and single-dish work. This band coverage offers flexibility for red ... More
Presented by Mrs. Parisa RAHIMI on 6/9/2024 at 10:15
Small and flexible VLBI arrays, as exemplified by the successful EVN-lite operational model, can produce significant scientific outcomes. INAF, the Italian National Institute of Astrophysics, operates such an interferometer, comprising three dishes with a total collecting area equivalent to an 80m radio telescope and baselines up to 950 km, supported by a software correlator in Bologna. This facil ... More
Presented by Dr. Marcello GIROLETTI on 6/9/2024 at 9:30
Presented by Anton ZENSUS on 6/9/2024 at 8:30
The next decades of radio astronomy will be dominated by large facilities of superior sensitivity. Between 1GHz and 15GHz, strong synergies can be developed between the next-generation Very Large Array (ngVLA) and the Square Kilometre Array (SKA), specifically the SKA-mid. Towards higher frequencies, the ngVLA will be able to co-observe with other frontline facilities including the EVN (at 1-43 GH ... More
Presented by Prof. Matthias KADLER on 6/9/2024 at 9:45
In 2017, the National Astronomical Research Institute of Thailand (NARIT) launched a national flagship project with the empyreal goal of capacity building and technology development through the construction of national radio telescopes for radio astronomy and geodesy. To achieve this, NARIT has established the Thai National Radio Astronomy Observatory (TNRO), in Chiangmai, the northern part of Tha ... More
Presented by Dr. Koichiro SUGIYAMA on 6/9/2024 at 10:00
The Global Millimetre VLBI Array (GMVA) represents the most extensive array for high-resolution observations at 3.5 mm wavelengths. The mm-VLBI technique has reached a state of maturity and is now delivering cutting-edge results (e.g., the combined image of the black hole shadow and the jet in Messier 87 published by Lu et al. in April 2023). A leap forward is planned with upcoming advancements, ... More
Presented by Prof. Eduardo ROS on 6/9/2024 at 7:00
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