Keywords: astro-30m-emir-time-estimator

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## Frontends

Warning: Please do not quote these values in your papers. You should refer to the publications which fully describe the receivers.

- The receiver temperature is the sum of
  - The mixer temperature: Typically 50 K below 260 GHz and 70 K above;
  - The mirror losses: Typically 10 K;
  - The dichroic losses: Typically 15 K. Nota Bene: Dichroics enable dual frequency observation by frequency separation of the sky signal.
  We end up with K below 260 GHz and K above 260 GHz.
- .