Cryogenic LNA Range (Radio Astronomy & Deep Space)
TTI Norte
Cryogenically-cooled low-noise amplifier portfolio spanning UHF to W-band for radio astronomy, deep-space ground stations and quantum computing applications.
Technical specifications
- W-band
- 72 - 116 GHz, ~31 K average noise temperature
- Q-band
- 31 - 50 GHz, ~14 K average noise temperature
- K-Ka band
- 18 - 32.4 GHz, ~8 K average noise temperature
- C-Ka band
- 4 - 20 GHz, ~4.7 K average noise temperature
- X band (0808)
- 8.4 - 8.5 GHz, < 3 K noise temperature
- X band (0809)
- 8 - 9 GHz, < 4 K noise temperature
- C-X band (2-18 GHz)
- ~4.8 K average noise temperature
- C-X band (0412)
- 4 - 12 GHz, 5 K average noise temperature
- C band (0506)
- 5.7 - 6.3 GHz, < 2.5 K noise temperature
- C band (0408)
- 4 - 8 GHz, < 3.5 K noise temperature
- S band (0204-B)
- 2.3 - 4.8 GHz, < 3.5 K noise temperature
- S band (0204-A)
- 2 - 4.5 GHz, < 3 K noise temperature
- UHF-S band
- 0.1 - 3.3 GHz, 4.5-5 K average noise temperature
About
Celestia TTI’s cryo-LNA range covers radio astronomy, deep-space tracking (e.g. ESA ESTRACK) and quantum computing applications, spanning UHF through W-band with noise temperatures as low as sub-2.5K depending on band. Products include single- and multi-octave designs across S, C, C-X, X, K-Ka and Q/W bands.
Documentation
- prod_cryolna_ds_x0808.pdf kosmolab.space ↗
- prod_cryolna_ds_x0809.pdf kosmolab.space ↗
- prod_cryolna_ds_cx0412.pdf kosmolab.space ↗
- prod_cryolna_ds_c0506.pdf kosmolab.space ↗
Need the full ICD, test reports or a specific revision? Ask the supplier directly.
