Sorry, forgot to answer those other questions...
1) Can we use the other scans as well as the Excitement of science named scan.
Well you can if you like but might be good to hold fire for a bit. I plan to provide a bit of info on doing that when we've got a bit farther with the special EoS scans and the radio sky image builds up a little farther.
However if you're champing at the bit you could do a "21cm Spectral Line Observation - Simple" pointing at galactic coordinates longitude=120, latitude=0, with integration time 120s. This will show you a spectrum of atomic hydrogen in that direction. You'll see several peaks, each of which is a spiral arm of the Milky Way. See
http://webmail.jb.man.ac.uk/distance/observatory/Generic_Exercise2.pdffor some backgroud on what it all means (note the Simple observation setup hides a few of the extra details referred to in this document)
I'd prefer if you didn't do all the exercises in this document as it will take time away from other schools completing the EoS observations.
2) Now that we have some data (even though it cut off with 5 degrees left) what do we do, just look at it and make conclusions? or is there something else we could be doing as well...
Try your other longitude?
I've divvied up the range 10 to 240 degrees between everybody (including some overlap so we get multiple scans of the same bit of sky). At some point we will look to extend the scan to go outside the range of 10 degrees either side. keen shcools could help here. I just need to check that the live radio sky plotting program will handle this so hold off a bit until I'm sure we're ok on that.
3) Is it possible to do more than 1 scan in a row, if we booked say 3 or 4 time slots?
Each scan is scheduled separately in however many slots you assign it. You can always schedule two scans straight after each other. However, bear in mind that if the two pointing positions are widely separated on the sky there is a significant time taken to slew the telescope around (slew is a bit of jargon meaning move!). This can result in an observation failing to complete before the next one starts.
Hope that all makes sense,
Tim