FAST low frequency pulsar survey
نویسندگان
چکیده
منابع مشابه
The VLA Low-frequency Sky Survey
The Very Large Array (VLA) Low-frequency Sky Survey (VLSS) has imaged 95% of the 3π sr of sky north of δ = −30◦ at a frequency of 74 MHz (4 meter wavelength). The resolution is 80 (FWHM) throughout, and the typical RMS noise level is 〈σ〉 ≈ 0.1 Jy/beam. The typical point-source detection limit is 0.7 Jy/beam and so far nearly 70,000 sources have been catalogued. This survey used the 74 MHz syste...
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ژورنال
عنوان ژورنال: Proceedings of the International Astronomical Union
سال: 2012
ISSN: 1743-9213,1743-9221
DOI: 10.1017/s174392131300001x