R CrA     3 sources in R CrA are identified as new detections: sources R CrA 2,
R CrA      6 and 7. Source R CrA 2 lies close to R CrA 1, separated by 30", but 
R CrA      shows sufficiently different spectral characteristics that it 
R CrA      cannot be a ghost of this source. It is therefore considered to be 
R CrA      a real source, probably a YSO. Both R CrA 6 and 7 lie in a region of
R CrA      nebulosity between the bright sources HH100-IR (R CrA 5) and R CrA 
R CrA      (which lies just outside the image frame). These are not considered
R CrA      to be ghost images, but may well represent peaks in the nebulous 
R CrA      emission rather than true YSOs. It should also be noted that this 
R CrA      region of the R CrA cloud was not included in the ISOCAM survey of 
R CrA      Olofsson et al. (1999, Cat. <J/A+A/350/883>), due to detector 
R CrA      saturation, so it is not unreasonable to expect new detections here.
rho Oph E A large number of ghost images were found here and after they were 
rho Oph E  removed 1 unidentified source remained: {rho} Oph E 4. However, 
rho Oph E  this is the faintest source in the survey, with a flux rising to 
rho Oph E  just 0.17Jy at 16{mu}m, so is probably a peak in the nebulosity 
rho Oph E  rather than an "new'' YSO. 
Ser B     2 sources in Ser B were not identified with previous observations: 
Ser B      Ser B 4 and 7. Both these sources lie near to SVS20 and so could be
Ser B      ring-like ghost images associated with it. However they also lie in
Ser B      a previously identified region of nebulous emission (Kaas,
Ser B      1999AJ....118..558K) and so may instead be peaks in this 
Ser B      nebulosity. It is impossible to resolve this ambiguity completely,
Ser B      but in either case these 2 sources are probably not "new'' YSOs.