Searching for Transient Pulses with the ETA Radio Telescope
| dc.creator | Patterson, Cameron D. | |
| dc.creator | Ellingson, Steven W. | |
| dc.creator | Martin, Brian S. | |
| dc.creator | Deshpande, Kshitija | |
| dc.creator | Simonetti, John H. | |
| dc.creator | Kavic, Michael | |
| dc.creator | Cutchin, Sean E. | |
| dc.date | 2008-12-06 | |
| dc.date.accessioned | 2026-07-07T12:45:52Z | |
| dc.date.available | 2026-07-07T12:45:52Z | |
| dc.description | Array-based, direct-sampling radio telescopes have computational and communication requirements unsuited to conventional computer and cluster architectures. Synchronization must be strictly maintained across a large number of parallel data streams, from A/D conversion, through operations such as beamforming, to dataset recording. FPGAs supporting multi-gigabit serial I/O are ideally suited to this application. We describe a recently-constructed radio telescope called ETA having all-sky observing capability for detecting low frequency pulses from transient events such as gamma ray bursts and primordial black hole explosions. Signals from 24 dipole antennas are processed by a tiered arrangement of 28 commercial FPGA boards and 4 PCs with FPGA-based data acquisition cards, connected with custom I/O adapter boards supporting InfiniBand and LVDS physical links. ETA is designed for unattended operation, allowing configuration and recording to be controlled remotely. | |
| dc.description | 18 pages, 9 figures | |
| dc.identifier | https://arxiv.org/abs/0812.1255 | |
| dc.identifier | http://arxiv.org/abs/0812.1255 | |
| dc.identifier | ACM Trans.Reconf.Tech.Syst.1:1-19,2009 | |
| dc.identifier | doi:10.1145/1462586.1462589 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/221190 | |
| dc.subject | Astrophysics | |
| dc.title | Searching for Transient Pulses with the ETA Radio Telescope | |
| dc.type | text |