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. Author manuscript; available in PMC: 2020 Feb 4.
Published in final edited form as: Publ Astron Soc Jpn Nihon Tenmon Gakkai. 2018 Apr 11;70(2):10.1093/pasj/psx083. doi: 10.1093/pasj/psx083

Table 2.

Frequency bands of the Kashima observatory

channel k frequency (MHz) minimum-maximum original bandwidth (MHz) effective bandwidth (MHz) after filterization (Δvk)
ch0 1404–1436 32 20.48
ch1 1570–1602 32 16.00
ch2 1596–1628 32 -
ch3 1622–1654 32 -
ch4 1648–1680 32 24.83
ch5 1674–1706 32 21.82
ch6 1700–1732 32 23.23
(ch7) (1702–1734) (32) -

The frequency range between ch0 and ch1, 1436–1570MHz, is avoided so as to minimize the radio frequency interference (RFI) from cellphone base stations. Only the right-hand circular polarized signals were received. In the coherent dedispersion process for each channel, the timing of the voltage data is adjusted to that for the maximum frequency of the channel.