hi All- To follow up on the "Rx suite" selection issue which I mentioned in the commissioning meeting this morning: we need to think through how we will rotate receivers through the year and which receivers will go in which holes in the turret. There are 8 holes 1 with d=48'' 3 d=36'' 4 d=24'' The current arrangement nominally is 48: L 36: S 24: C 24: X 24: Ku 24: K 36: Q 36: holo We are planning 4 additional receivers: Ka, W, Penn Array, and W2 (90-116 GHz). It will be desirable for these to be up for as much of the winter as feasible. Packaging on *all* of these receivers is currently negotiable. The notional Q-band tertiary is what motivated the 36'' slot for this receiver; as a possible constraint on this and other receivers this design needs more careful consideration. I propose a nominal arrangement as a starting point. In this arrangement we have a "low frequency season" (~ 01May - 01 Sep) and a "high frequency season" (the other 8 months). There will be a set of receivers up, more or less the same each year, in each season; we will plan on individual swap outs, however, to accomadate projects or blocks of them (VLBI, radar, particular LST ranges, holography, etc) "out of season". The rationale for the uneven split is that we want to be ready for good conditions when they come, wheras most lower frequency observations can easily be scheduled in advance via the above mechanism. Here's what I propose: Low Frequency Season 48: L 36: S 24: C 24: X 24: Ku 24: K 36: Holo 36: Q High Frequency Season 48: L 36: S -> W 24: C-> Ka 24: X 24: Ku -> (W2 eventually) 24: K 36: Holo -> Penn Array 36: Q One possibility which would buy some flexibility is to make one or more "mating plates" to fit 24'' Rx's in 36'' holes. I welcome any and all comments, especially from those more familiar with operational constraints and the current science demand. To be clear what I am trying to define now are receiver packaging constraints. A missing piece of the puzzle is a real tertiary design(s). -Brian