21-22 September 2020
Max Planck Institute for Radio Astronomy
Europe/Berlin timezone
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Session 1:

Place

Location: Max Planck Institute for Radio Astronomy
Address: Auf dem Huegel 69 53123 Bonn GERMANY
Room: Lecture Hall 0.02
Date: 21 Sep 13:00 - 14:40

Description

Future plans for existing telescopes. Chair: Dr. A. Navarrini

Timetable | Contribution List

Displaying 4 contributions out of 4
Session: Session 1:
IRAM operates two millimetre observatories on two sites: the NOEMA interferometer located in the French Alps at 2500m altitude with currently 11 antennas of 15m diameter and the 30m telescope in southern Spain, Pico Veleta (3000m). They observe in the 70-373 GHz frequency range. We'll summarise the current receivers status and performance, and present the plans for the near and far future. In part ... More
Presented by Dr. christophe RISACHER on 21/9/2020 at 11:25
Session: Session 1:
ASTRON operates the pan-European Low -Frequency Array (LOFAR), a unique instrument that will complement phase one of the Square Kilometre Array (SKA), planned for construction in the coming three to five years. After nearly a decade of scientific operations, LOFAR science output is still ramping up. However, to keep the telescope at the forefront of science, a staged upgrade programme LO ... More
Presented by Dr. Albert-Jan BOONSTRA on 21/9/2020 at 11:50
Session: Session 1:
It is universally recognised that a well-funded and carefully targeted development programme is essential to maintain the scientific competitiveness of any observatory. The purpose of the SKA Observatory Development Programme (SODP) is to enhance the scientific productivity of the Observatory by: adapting to changes in the scientific landscape and priorities, enabling new science, restoring descop ... More
Presented by Mr. Luca STRINGHETTI on 21/9/2020 at 11:00
Session: Session 1:
A new digital back-end architecture for the Very Long Baseline Array (VLBA) is being developed at NRAO. The system will consist of several main components that are interconnected through a 100 Gbps Ethernet switch. A pair of dual-channel IF samplers will be placed in the VLBA receiver cabin, producing four VDIF streams at 2048 Gsps and with greater than 8 bits per sample quanitzation. These "di ... More
Presented by Dr. Walter BRISKEN on 21/9/2020 at 12:15
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