Map with the observed area in the red filter (DSS1 Red from the SkyView Virtual Observatory). The small square shows the area observed with the VATT telescope to fainter magnitudes. Approximate positions of the northern part of the emission nebula Sh2-205, the centre of the dark cloud TGU H942 P7, and a part of the cloud TGU H942 P8 are labelled. The four-digit numbers designate positions of a few clouds that were identified by Dobashi (2011). The brightest star in the area is the eclipsing variable DD Cam (HD 24733). CY Cam might be the ionising star of Sh2-205.