SEPIA system temperature
The Swedish-ESO PI receiver for APEX (SEPIA) 345 GHz receiver is being built for the APEX Observatory. It covers the frequency ranges between 272 and 376 GHz. It is set-up to cover channel spacings from 62.5 kHz to 0.18 GHz. It has a receiver temperature that rises from 90 K to 216.5 K. (See Meledin et al. 2022 for more details.)
Here in the AtLAST sensitivity calculator, we use it as an exemplar of a heterodyne instrument capable of working at these frequencies.
In this module, we calculate the system temperature used in the overall sensitivity equation. For a SEPIA like system, the system temperature is calculated as:
where
\(\eta_\mathrm{eff}\) is the forward efficiency of the telescope
\(\mathfrak{t}\) is the atmospheric transmittance, defined as \(\mathfrak{t} = \textrm{exp}^{(-\tau_{atm})}\)
\(T_\mathrm{rx}\) is the receiver temperature
\(T_\mathrm{sky}\) is the sky temperature (in terms of a Rayleigh-Jeans brightness temperature) calculated from the model grid described in Weather Calculations
\(T_\mathrm{amb}\) is the ambient temperature
Here, \(O(\nu, T)\) converts a physical temperature to a Rayleigh-Jeans brightness temperature
Through consultation with the developers of the SEPIA instrument, we assume a receiver temperature that remains constant between observing frequencies of 272 and 330 GHz and then rises up to the maximum frequency of 376 GHz:
These values are used in the \(T_{sys}\) equation above, which is in turn used to calculate the System Equivalent Flux Density used in the overall sensitivity (or integration time) calculation.