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Expected Source Properties (for Technical Assessment)

This panel contains three fields that are used by the ALMA Staff to doa technical review of the Phase 1 proposal. The only mandatoryparameter is the Peak Flux Density . This should be an estimateof either the flux you expect in a continuum map or the peak fluxdensity of your main spectral line of interest. If you are observingspectral lines then please enter an expected line width. If yoursource is polarized, please enter the expected magnitude ofpolarization - however, note that polarization observations are notoffered for Cycle 0.



The ALMA OT Team, 2011 May 20