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information_for_astronomers:rx:p200mm [2015/06/23 11:12] akraus |
information_for_astronomers:rx:p200mm [2024/06/14 11:08] (current) akraus |
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This system is used for sensitive continuum, VLBI (especially 18cm), spectroscopy, and pulsar observations. Be aware, that this band may be influenced by RFI. It can be used in combination with a multi channel polarimeter of 8x4 MHz band width, and a total 40 MHz wide channel. | This system is used for sensitive continuum, VLBI (especially 18cm), spectroscopy, and pulsar observations. Be aware, that this band may be influenced by RFI. It can be used in combination with a multi channel polarimeter of 8x4 MHz band width, and a total 40 MHz wide channel. | ||
+ | Interferences are heavily present in these bands, unfortunately also around the 1720 MHz OH transition. | ||
==== Calibration Information ==== | ==== Calibration Information ==== | ||
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**Comments:** | **Comments:** | ||
* Strong interferences can occur in this frequency regime, eg. between 1.50 and 1.64 GHz! | * Strong interferences can occur in this frequency regime, eg. between 1.50 and 1.64 GHz! | ||
- | * There are two values for the noise cal, different by about 4dB. See the table below to learn which receiver version uses which value. | + | * There are two values for the noise cal, different by about 6dB. See the table below to learn which receiver version uses which value. |
==== Version description for OBSINP ==== | ==== Version description for OBSINP ==== |