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Davide Fierro03/12/2018, 11:30Oral
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Luca Stringhetti03/12/2018, 11:45Oral
The short presentation will present what we consider to be most important technical challenges for the SKA project. Before doing that, we need to put some context around and the current status of the project. The bridging phase and the adoption process to get to a successfully System CDR will be presented. The bridging phase will cover the gap between the Element CDRs and the System CDR, its...
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Jader Monari03/12/2018, 12:10Oral
The Italian contribution within the SKA1-LOW instrument and in particular on the Low Frequency Aperture Array (LFAA) Element has been important since the conception of the Square Kilometer Array project.
The Low Frequency Aperture Array is a key component of the SKA. Combining 128 thousands of antennas into up to 2048 stations, with multiple beams and an instantaneous frequency coverage of 50...
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Pietro Bolli (INAF - OAA)03/12/2018, 12:30Oral
This contribution deals with the SKALA4-AL antenna developed by INAF in collaboration with CNR-IEIIT and the industrial partner Sirio Antenne. This dual-polarized Log Periodic Dipole Antenna optimized to operate between 50 and 350 MHz is a candidate for the SKA1-LOW telescope. The main characteristics of the antenna are: aluminium material, 50 ohm single-ended feeding, screw fastening and...
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Federico Perini (IRA - INAF)03/12/2018, 12:45SKA-related technology and HPC activities in ItalyOral
INAF/IRA has a long and well established tradition with low frequency arrays thanks to the Northern Cross radio telescope, located in Medicina (Italy). Since the beginning of the Italian adventure in the SKA project, with the participation to the SKADS EC-FP6 program, INAF/IRA has been involved, as part of its general effort, to contribute into the design of RF receivers for low frequency...
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Francesco Schilliro' (Istituto Nazionale di Astrofisica (INAF))03/12/2018, 14:00Oral
ITPM ADU is an international collaboration led by INAF team, whose goal is the realization of a digital equipment designed and produced for SKA-LFAA station signal processing. The project started in 2013 and led to the production of a digital platform consisting of 3 hardware upgrades (ITPM 1.0, 1.1 and 1.2), the processing and management firmware for LFAA and the station control software....
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Corrado Trigilio (INAF-OA Catania)03/12/2018, 14:15Oral
The Square Kilometre Array is currently completing the pre-construction phase in which two arrays of radio antennas (SKA1-Mid and SKA1-Low), observing at different frequencies, are being designed to be installed in the South Africa's Karoo region and Western Australia's Murchinson Shire. The SKA1-Mid array will consist of 133 15-m diameter dish antennas observing in the 350 MHz-14 GHz range...
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Gianni Comoretto03/12/2018, 14:40Oral
The SKA Central Signal Processor represents the largest radioastronomical correlator ever designed, including a massive real time pulsar search and pulsar timing machine.
Italian contribution to this element is described. It includes a study of the element local monitor and control, with particular emphasis to the pulsar search machine, the final optimization stag of the pulsar search, and...
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Mauro Dolci (Istituto Nazionale di Astrofisica (INAF))03/12/2018, 15:05Oral
Telescope Manager (TM) is the central element of the SKA. Its role (and responsibility) are the management of the preparation of astronomical observations, the execution of telescope operations and the control and monitoring of the overall telescope status.
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To accomplish these functions, TM was originally structured as made of of specific sub-elements: Observation Management (OBSMGT,... -
Alessandro Navarrini03/12/2018, 15:30Oral
High-sensitivity large-scale surveys are an essential tool for new discoveries in radio astronomy. A Phased Array Feed (PAF) placed at the focal plane of an antenna can increase the Field-of-View (FoV) and the mapping efficiency by fully sampling the sky. Multiple beams can be formed by adding signals from electrically small focal plane radiating elements of the array using different sets of...
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Stefania Matteoli (CNR – IEIIT)03/12/2018, 16:30SKA-related technology and HPC activities in ItalyOral
New-generation radio telescopes such as the SKA’s aperture array require advanced techniques to confirm the desired performance and calibrate the instrument. At low frequencies, the strong mutual coupling between the array elements and the interaction of the antennas with the environment can drastically alter the expected response of the elements and compromise the calibration process.
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In this... -
Maurizio Miccolis04/12/2018, 09:15Oral
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A. Possenti / R. Smareglia04/12/2018, 09:40Oral
SKA Data Challenger is only one of the IT technologies challengers in which the SKA project is involved. These imply all activities from data management, network transfer, (super)computing infrastructure to, last but not least, software pipeline development and workflow management. INAF, as Italy main actor in the SKA project, can play an important role, both in the evolution of the exascale...
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U. Becciani / G. Taffoni04/12/2018, 10:10Oral
On March 2018, INAF approved the participation to the International LOFAR Telescope (ILT) and the organization of a LOFAR-IT Consortium leaded by INAF itself aiming at coordinating at Italian level the participation to ILT.
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The University of Turin (Department of Phyiscs: DP-UniTO) has recently formalised the participation to LOFAR-IT Consortium.
A Board of the LOFAR-IT project has been... -
Marcella Massardi (INAF-IRA/Italian ARC)04/12/2018, 10:40Oral
Training and support services will provide the pillars for the future SKA endeavour.
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The AENEAS WP5 analysis identified the crucial aspects in preparing for the new frontier that is SKA: several challenges await our astronomical communities to proficiently face the opportunities offered by it. A preparatory plan based on coordinated training events that exploit current facilities and tests... -
Luca StringhettiOral
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