Design of (2+1+2)D FFT for Interferometric Pulsar Survey

Author:

Daishido T.,Tanaka N.,Sudo S.,Suzuki M.,Saito Y.,Agehama R.,Adachi M.,Watanabe N.

Abstract

AbstractThe Following design of a Pulsar Survey System with a Huge Interferometric Array is discussed. (1) A Huge Array of 320m × 320m with 256(= 16 × 16) spherical dishes of 20m in diameter, (2) RF is 1.4 GHz, (3) Receivers are frequency modified GPS(1.57542, 1.2276GHz) ones, (4) Phase and Delay Tracking, (5) Phase Calibration using Differential GPS(GPS signal × 2 → CW), (6) (2+1+2)D FFT /256 pixel Imaging + 256 ch Filtering + Dispersion Removal and Period finding(17M point floating 2DFFT by DSP), (8) Observing time required for the same sensitivity to Arecibo τ/τA: 0.88(Timing), 0.003(Survey).

Publisher

Cambridge University Press (CUP)

Subject

General Medicine

Reference5 articles.

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Two 1.4 GHz Sky Atlases at Declination 32° to 42° in Nasu Radio-Transient Search Project;Publications of the Astronomical Society of the Pacific;2008-03

2. Quick‐Look Data Analysis in the Nasu Radio Transient Search Project;Publications of the Astronomical Society of the Pacific;2007-10

3. High and Low Galactic Latitude Radio Transients in the Nasu 1.4 GHz Wide-Field Survey;The Astronomical Journal;2007-03-01

4. A 3 Jy Radio Burst at a High Galactic Latitude;The Astrophysical Journal;2007-02-01

5. The Automatic Radio Burst Search System at Nasu Observatory;Publications of the Astronomical Society of the Pacific;2006-06

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