In the ALMA system, no portion of the baseband or spectral window can lie outside of either the IF or RF range. This fact alone does not present any unforeseen limitations on what can be observed within the specified ranges. However, an issue arises because a spectral window has an effective bandwidth of only 15/16 (93.75%) of its total bandwidth, while no portion of its total bandwidth can lie outside of the baseband. This constrains the effective useable IF and RF ranges to:
IF_min,eff = IF_min + BW/32.0 IF_max,eff = IF_max  BW/32.0
RF_min,eff = RF_min + BW/32.0 RF_max,eff = RF_max  BW/32.0
where BW refers to the total spectral window bandwidth (as chosen from the set of 2, 1, 0.5, 0.25, 0.125, 0.0625 GHz), and the min and max IF and RF ranges are listed in the table below (all values are in GHz). You can also find this table in the ALMA Technical handbook, Table 4.1.
While there is ongoing discussion to relax this requirement, it currently restricts how close one can place a spectral window to the receiver band edge (RF) and to the baseband edge (IF). These restrictions are correctly implemented in the OT. The most obvious restriction comes in situations where you want to observe two lines at the extreme edges of the IF range. The 12CO(21) and 13CO(21) lines are a particularly important example. Here the lines are so close together that you must place both lines in the IF near the lower limit of 5 GHz. Thus, the velocity space available around the lines is quite limited, particularly when using the broadest spectral windows. As the spectral window bandwidth is reduced, the effective edge of the window gets closer to the true edge of the IF range, allowing a little more freedom. Below are three tables which define the usable range of IF for the various combinations of Band and spectral window. The specific case of 12CO(21) and 13CO(21) is shown explicitly in the Band 6 Table, including the central frequencies to use when defining spectral windows which will place these two lines equidistant from the band edges. Please note that if the redshift is different to 0, you may have to vary slightly the figures in the table.
As of the start of Cycle 6, the Band 6 IF bandwidth has been increased by 0.5 GHz to extend from 4.5 to 10 GHz. This will enable12CO,13CO and C18O J=21 to be observed simultaneously with broader spectral windows. In the Band 6 table below, for all spectral window equivalent bandwidths the spectral window central frequencies are 218.2185 GHz for 13CO 21 and 232.7185 GHz for 12CO 21.
There is also a known bug in the OT which affects spectral setups where the spectral windows are at the extreme edges of the IF. This means that the frequencies given below may have to be changed slightly (by fractions of a MHz) in order for a tuning to be found, in the sense that the spectral window should be moved away from its sideband edge. For example, the Band6 setting given below for the 117 MHzwide spectral window would work (for zero velocity) with frequencies of 220.4060 and 230.5311 GHz (a change of 100 kHz in the higherfrequency spectral window).
Spectral window 
Bands 3,4,5,7 and 8 
Bands 9 and 10 
bandwidth 
Lowest IF accessible 
Highest IF accessible 
Lowest IF accessible 
Highest IF accessible 
(MHz) 
(GHz) 
(GHz) 
(GHz) 
(GHz) 
1875 
4.0625 
7.9375 
4.0625 
11.9375 
937.5 
4.0313 
7.9688 
4.0313 
11.9688 
468.75 
4.0156 
7.9844 
4.0156 
11.9844 
234.375 
4.0078 
7.9922 
4.0078 
11.9922 
117.1875 
4.0039 
7.9961 
4.0039 
11.9961 
58.59375 
4.0020 
7.9980 
4.0020 
11.9980 
Band 6 Effective 

12CO & 13CO 21 
Spectral 

Clearance of both 
Window 
Lowest IF 
Highest IF 
lines from spectral 
Bandwidth 
accessible 
accessible 
window edge ** 
(MHz) 
(GHz) 
(GHz) 
(MHz) 
(km/s) 
1875.0 
4.5625 
9.9375 
507.000 
659.30 
937.500 
4.5313 
9.9688 
538.250* 
699.94* 
468.7500 
4.5156 
9.9844 
553.875* 
720.26* 
234.3750 
4.5078 
9.9922 
561.688* 
730.42* 
117.1875 
4.5039 
9.9961 
565.594* 
735.50* 
58.59375 
4.5020 
9.9980 
567.547* 
738.04* 
*These windows are sufficiently narrow that the lines can be centered in them.
**The velocities are computed for the higher frequency line (12CO21)
