All Tables

Table 1: Summary of the initial scientific requirements and top level specifications for AMBER.
Table 2: Number of photons per frame and per channel needed for the frame to contribute to the ensemble averages, as a function of the observing mode and considering the measured and the potential (vibration-free) atmosphere+VLTI+AMBER visibility.
Table 3: Number of photons collected per 50 ms frame and per spectral channel in the K band in different observation modes.
Table 4: Current, potential, and achieved limiting magnitudes of AMBER in the K band, for $50~\mbox{ms}$ frames.