I think this could be the main source of your problems.
http://www.sciencedirect.com/science/article/pii/S0927776505000986
http://pubs.acs.org/doi/abs/10.1021/ac061341j
5/ Yes the detector is a DTGS and i do not have an access to an MCT detector.
In both of these papers, they use an MCT detector, which is probably why they can get away with using a microscope FT-IR, rather than grazing angle accessory. Essentially as you adjust the angle of incidence, the number of reflections varies until you reach a maximum just before the grazing angle, as you go through the grazing angle, the signal inverts sharply and hence the most sensitive region is either side of the grazing angle for a given substrate.
The graph at the end of the first page in the following link shows how the sensitivity varies as a function of angle of incidence using their Veemax accessory.
http://www.piketech.com/files/pdfs/VeeMAXIIPDS611.pdfIf you have recently purchased an accessory, it is likely you have a good rapport with the sales person. It is worth speaking to them and trying to arrange a demo of the accessory.
As I mentioned in my previous post Harrick also manufacture accessories. However, they are based in the states and you will pay a premium for them, expect them to be 2-3 more expensive than the Pike, although I believe in this case you genuinely get what you pay for.
With reference to the papers, I can't quite work out what they have done in terms of collecting the data. Have the recorded the spectra with 100-200 scans or, have they recorded 100-200 samples with x number of scans per sample?
Looking at their spectra (I like the way they have deconvoluted the amide bands) and yours, is it possible you have a very weak signal in the 1500-1800 cm^-1 region?
It looks like you have a fairly nice IR there, I would try to record the following spectra with the highest practical resolution and a minimum of 1024 scans.
Background
Substrate
Substrate + Sample.
Baseline correct, smooth and normalise all the spectra in the IR software and export as CSV or similar.
Use origin to plot the individual spectra and then use origin to subtract you references. This is where 1024 scans will help. Origin is also quite good at doing this. I haven't for origin on this computer, but if you need help here, can check and let you know the steps.
If that doesn't work, I would really follow up with Pike/Harrick, especially if you don't have access to an MCT.
Good luck
djt