The noise you are seeing is noise caused by dark current. I downloaded all of your images, and checked them out in PixInsight, an advanced astrophotography processing tool.
As far as I can tell, you do not have any many pixels. Stuck pixels tend to be significantly brighter than the background noise in a dark frame all the time regardless of exposure time or thermal status. I did see a very small handful of such pixels...values around 3500 ADU when the background noise averaged around 513 ADU (ISO 800 dark).
The thing about dark current is it is an additional signal added to your image signal. As a signal, it includes it's own random (gaussian) noise. In a 450 second exposure at higher ambient temperatures, you could easily accumulate a dark current signal in the range of several hundred ADU. If your dark current was 300 ADU, it's noise would be SQRT(300) ADU, or 17.32. That is additional random noise, on top of read noise and photon shot noise, and separate from the increase in hot pixels (which are different from stuck pixels, as they change with exposure time and thermal factors.)
None of this is unusual. The use of long exposure noise reduction (LENR) will take another 450s exposure after the image exposure, with the shutter closed, and subtract that from the image frame. That will usually remove hot pixels and stuck pixels, however it will actually also usually increase random noise, making the image noisier (even if the characteristic is better).
If you wish to get the best results possible with your night imaging, you could take the astrophotography approach. Generate a master dark frame, and subtract that yourself, rather than using LENR. A master dark frame is generated by taking a bunch of frames, say 25 or 36, and stacking them together with an averaging algorithm. This single master dark could then be used to subtract the dark current and it's noise from your nighttime images. It can be reused, so long as the temperatures of your images is within a few degrees of your master dark, so you waste less time on-scene waiting for LENR to take an additional exposure after each and every frame.
By averaging 25 dark frames together, you reduce the random noise by a factor of 5. Average 36, and you reduce it by a factor of 6. Average 100, you reduce it by a factor of 10. The lower the random noise in your master dark, the lower your random noise will be in your "calibrated" image frames. This will give you the best noise characteristics possible in your images, removing the hot and stuck pixels, the bias signal, as well as any dark signal offset.