I prefer to go a bit less than the "5x" pixel sizing that gets spruiked ad infinitum & I don't know what you mean by increasing the gain significantly...perhaps you mean that because of the greater image scale you have to work at with the ADC means you need more gain for the same histogram..?
In any case a couple of things - make sure that you increase the integration time for the ADC display balls if you use that approach, it stops them ricocheting around like crazed pin-balls. 
I've posted plenty of examples of how to utilise just the barlow's lens element minus the body to reduce any specific barlow's amplification factor - using a T2 male-female adaptor in the train only requires the lens element to be "floating" and held via the aforementioned device's compression band clamps.
Here's my extrapolation of the Televue 2x barlow's response where with just the lens element it can provide almost down to 1.25x without any deleterious optical effects. There are of course specific lower-amplification barlows available as alternatives...
Btw we've found that an ADC can still provide correction with Jupiter in Sthn. Oz this year at 55° or so...
If you look at our current thread you will see the imaging train I use - this has a custom Siebert 1.5x barlow but you can hold a "floating" barlow lens element in that T2 male-female adaptor that is connected to the rear of the EFW shown - a main concern is to have rotational capabilities for the camera as well as for the ADC for initially setting it level.
Mars definitely benefits from using an ADC in Oz for us folks nowadays! 
This old thread of mine that someone revived recently is probably worth a good look to give you some ideas. https://www.cloudyni...owers-anyone/