Note: Duplicate of Sawbird LNA Bandpass Plots page.
There are a number of low-noise amplifier + filter devices available useful for radio astronomy. These are available from Nooelec (https://www.nooelec.com/store/sdr/sdr-addons/sawbird.html) as Sawbird LNAs. The gains and noise figures are reasonable. The passband characteristics are suitable for a couple of transition line targets - namely the HI 1420 MHz line and the OH maser 1612/1665/1667/1720 MHz lines.
The bandpass characteristics of three Sawbird LNAs are given below - the +HI, +IR and +GOES models are examined.
For excitation a broadband noise source is used and the bandpass output displayed on a spectrum analyser. The broadband noise source used has an output at a sufficiently low level such as to not overload the LNAs in the Sawbirds. If a higher level source was used, an appropriate amount of attenuation would need to be inserted between the source and the Sawbirds to avoid overload.
The passband is not particular flat. However, the 3 dB bandwidth (~70 MHz) is much wider than required for the spread of HI line velocities likely to be encountered. For example - a velocity range of ± 250 km/s translates to about 2.4 MHz at 1420 MHz . This bandwidth corresponds to about 1/10th of a division (1 division = 25 MHz) on the horizontal frequency scale. - 1/30th of the 3 dB bandwidth. Therefore the inflections of the passband ripple are not seen - but some local slope will be seen.
Nominally used for observing the Iridium satellites - which use the L-band frequency ranging from 1616 to 1626.5 MHz to communicate directly with ground-based users. Also in this band are the GLONASS satellites (1598 to 1605.5 MHz).
Our target OH 1612 MHz transition line is sandwiched between the two.
This OH line - generally speaking - is emitted from some of the strongest 1.6/1.7 GHz masers.
Nominally used for receiving the GOES weather satellite, this Sawbird can be used for the other three 1.6/1.7 GHz OH transition lines - 1665, 1667 and 1720 MHz.
These three transition lines - again generally speaking - are emitted at a lower flux than 1612 MHz.