I followed up on CAN 20 and CAN 40 last night, two double stars that were included in the Cygni 100 Challenge list based on magnitudes that turned out to be infrared, so not visually observable. (See post 267 above, and following posts, for more details.)
Anyway, it sounded like fun to track them down, or at least pinpoint their approximate location, so last night I did. 
Here are the details for CAN 20, plus the rather critical notes detail from the stelledoppie listing, which I cleverly overlooked. 
CAN 20AC
20h34m +40*51'
6.90/8.60 13.8" pa 330
Notes: K (K-band or other infrared magnitudes)
I couldn't say how long I spent studying this starfield -- time has a tendency to stand still for me in such contexts.
(Guessing 45 minutes to an hour between CAN 20 and 40 together.) Here is an annotated simbad chart of the starfield.

I worked on CAN 40 before turning to CAN 20, and realized that the 20x80 Deluxe just didn't go deep enough to accurately pinpoint the CAN 40 position. No hope of seeing it visually from my driveway (visual magnitude 13.71), except perhaps with the 22-inch dob, which I still haven't gotten back in operation. Though chasing down something like this might be a motivator to get me moving on it. Anyway, I swapped the Oberwerk 20x80 out for the 25x100 (Farpoint UBM on the OB 5000 tripod), which did go deep enough so I could see guide stars to find the location of CAN 40. More on that later.
I navigated to the CAN 20 position from Gamma Cygni (aka Sadr) the center star of the Cygnus "cross" asterism, enjoying quite a pleasing view of the open cluster NGC 6910 with the 25x100 while finding my way. The arc of stars is a significant marker to orient around. No hint of the nebulosity can be seen in Bortle 7 skies, needless to say. The line of faint stars pointing north in the image leads to the position of CAN 40.
HJ 609 is a legitimate Cygni 100 Challenge double, which I observed Monday 12 September 2022 from my driveway.
HJ 609
20h33m +40*27'
8.84/9.34 26.7" pa 320*
Observed with Oberwerk 20x80 Deluxe III. A fun DS for the 20x80 under these sky conditions. Precise position must be known, but then not hard to see. Quite close but fully resolved. Both stars white. A bit challenging to hold steadily in direct vision but can be done with some effort. Easier in averted. Should be easier from a darker site.
The sky conditions that evening were not great -- 17.34-42 mpsas. In fact I ended my observing session after recording one more observation because the waning gibbous moon (92% full) made the sky so bright it wasn't worth the effort. But last night the moon wasn't a factor at all, and I recorded a sky quality measure of 18.20 mpsas, which is quite good for my location. Plus using the 25x100 made HJ 609 easy to view and striking. I regret not comparing 20x80 and 25x100 observations of it now.
There is always something more to see...
HJ 609 is in a line of faint stars leading north to the position of CAN 40, incidentally.
AG 409 did not make the Cygni 100 list because the secondary is fainter than the 9.5 magnitude cutoff. It was a delightful find last night, making the CAN 20 effort more than worthwhile (though that search on its own was enjoyable enough).
AG 409
20h33m +40*34'
9.40/9.92 9.8" pa 266*
I can just resolve this double with the 25x100. Both stars bright white. It is not far from the position for CAN 20. Wow!
To pinpoint the location of CAN 20, I worked from a quadrilateral of four stars, the brighter two forming a pointer, plus a second set of two stars making an intersecting line. The faintest of the stars in the quadrilateral grouping is 10.69 magnitude TYC 3157-1184-1.
After all of that effort, I could actually glimpse the CAN 20 primary in averted vision (TYC 3157-0581-1, 11.16 magnitude), but it was near the limit for the 25x100 from my driveway on a good night.
For scale, here is a Sky Safari chart of the CAN 20 / 40 starfield .The FOV ring represents the 2.4 degree field of the Oberwerk 25x100 Deluxe binocular. CAN 20 is annotated as TYC 3157-0581-1. CAN 40 as GAIA 2067836.... HJ 609 is annotated as SAO 49778.

One thing about making observations like this is that a mounted binocular is a must. There would have been no possible way to resolve any of these doubles or even see the field stars used to triangulate the position of CAN 20 otherwise. But even beyond that, detailed study of a starfield in this fashion requires an instrument that remains in position while consulting charts, working with Sky Safari, and writing notes. Another factor is that the more one researches and learns about a given starfield, the more one appreciates what is seen. In fact, the more one literally sees. This is the secret behind the success of Burnham's Celestial Handbook, and why it remains a favorite among amateur astronomers nearly six decades after its publication when some not insignificant percentage of the science it documents has been superseded by more recent knowledge.
I'll save my observation of CAN 40 for a later post. 
Thank you for reading my report. 
Edited by Fiske, 26 September 2022 - 05:21 PM.