Abstract
We have started programs at the Waseda Nasu Pulsar Observatory to identify EGRET γ-ray sources and to search for radio transients. The observed frequency was 1.4 ± 0.01 GHz, and eight-element spherical dish antennas were used as four pairs of interferometers, with each element 20 m in diameter. The observable region was ±5° from zenith, covering a region of sky 32° ≤ δ ≤ 42° in declination. For accurate flux measurement, we developed a receiver gain calibration system using Johnson-Nyquist noise; the system was compact, inexpensive, and easily maintained. We describe the system and recent results of radio source monitoring.
Original language | English |
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Pages (from-to) | 112-121 |
Number of pages | 10 |
Journal | Publications of the Astronomical Society of the Pacific |
Volume | 119 |
Issue number | 851 |
DOIs | |
Publication status | Published - 2007 Jan |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science