Differences

This shows you the differences between two versions of the page.

--- 1420mhzfeed [2026/05/17 22:45] – [Other Documents] dsheen
+++ 1420mhzfeed [2026/05/17 23:43] (current) – [1420 MHz] dsheen
@@ Line 3: / Line 3: @@
 The 1420 MHz frontend is a receive-only system designed by Daniel Sheen (KC1EPN) for radio astronomy. It is tuned to 1420 MHz for the hydrogen emission line and incorporates custom bandpass filters to reject high power OOB signals which otherwise overload the LNAs. The LNAs used are the first generation Indium Phosphide devices designed for the deep synoptic array, and incorporate noise calibration diodes which are used for amplitude and phase calibration of the full RX chain.
-Tsys for this frontend is around 45 K within the 1420 MHz protected band (1400 - 1427 MHz), and it has a gain of about 36.3 dBi. Performance degrades rapidly outside of the band.
+Tsys for this frontend is around 45 K within the 1420 MHz protected band (1400 - 1427 MHz), and it has a gain of about 36.3 dBi (~2.9 degree beamwidth). Performance degrades rapidly outside of the band.
 {{::1420mhz_frontend_simplified.jpg?direct&800|}}
@@ Line 59: / Line 59: @@
 Calibrator control is via a dedicated control board located at the feed. This board accepts 12 V power and two opto-isolated GPIO pairs, and provides a 5 V supply for the LNA summed with the calibrator control tones. These are then combined with the RF lines from the LNAs by minicircuits bias tees.
-[[https://github.mit.edu/w1xm/ULNA_Bias_and_CTL_v2.git[Control Board Kicad Files]]
+[[https://github.mit.edu/w1xm/ULNA_Bias_and_CTL_v2.git|Control Board Kicad Files]]
 The calibrator signals for the two channels are enabled by a 3.3V active high signal on outputs 0 and 1 of the Ettus X300 radio GPIO. Setting this requires running the following commands to configure the radio correctly:
@@ Line 93: / Line 93: @@
 {{ ::measurements.zip |}}
+LNA data:
+{{ :copy_of_03oct2022_cmt_ulna_data_ganesh_to_daniel.xlsx |}}