In the framework of the Square Kilometer Array (SKA) project, the Italian Institute for Astrophysics (INAF) has addressed several efforts in the design and prototyping of aperture arrays for low-frequency radio astronomical research. The Sardinia Array Demonstrator (SAD) is a national project aimed to develop know-how in this area and to test different architectural technologies and calibration algorithms. SAD consists of 128 prototypical dual-polarized Vivaldi antennas designed to operate at radio frequencies below 650 MHz. The antennas will be deployed at the Sardinia Radio Telescope's site with a versatile approach able to provide two different array configurations: (i) all antennas grouped in one large station or (ii) spread among a core plus few satellite stations. This paper provides an overview of the SAD project from an instrumental point of view, and illustrates its status after 2 years from its start.
Sardinia Array Demonstrator: Instrument overview and status / Bolli, P.; Comoretto, G.; Dallacasa, D.; Farooqui, M. Z.; Fierro, D.; Gaudiomonte, F.; Govoni, F.; Lingua, A.; Marongiu, P.; Mattana, A.; Melis, A.; Monari, J.; Murgia, M.; Mureddu, L.; Naldi, G.; Paonessa, F.; Perini, F.; Pisanu, T.; Poddighe, A.; Porceddu, I.; Prandoni, I.; Pupillo, G.; Rusticelli, S.; Schiaffino, M.; Schilliro, F.; Serra, G.; Tartarini, G.; Tibaldi, A.; Venturi, T.; Virone, G.; Zanichelli, A.. - STAMPA. - (2015), pp. 682-685. (Intervento presentato al convegno 2015 International Conference on Electromagnetics in Advanced Applications (ICEAA) tenutosi a Turin nel 7-11 Sept. 2015) [10.1109/ICEAA.2015.7297200].
Sardinia Array Demonstrator: Instrument overview and status
Dallacasa, D.;TARTARINI, GIOVANNI;
2015
Abstract
In the framework of the Square Kilometer Array (SKA) project, the Italian Institute for Astrophysics (INAF) has addressed several efforts in the design and prototyping of aperture arrays for low-frequency radio astronomical research. The Sardinia Array Demonstrator (SAD) is a national project aimed to develop know-how in this area and to test different architectural technologies and calibration algorithms. SAD consists of 128 prototypical dual-polarized Vivaldi antennas designed to operate at radio frequencies below 650 MHz. The antennas will be deployed at the Sardinia Radio Telescope's site with a versatile approach able to provide two different array configurations: (i) all antennas grouped in one large station or (ii) spread among a core plus few satellite stations. This paper provides an overview of the SAD project from an instrumental point of view, and illustrates its status after 2 years from its start.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
