N 442.  A bright star nearby causes a gradient in the background around the
galaxy.  External ellipses were contaminated by the star light.  The
extrapolated magnitude is not accurate enough to be included in the
comparisons.

N 943.  Galaxy with peculiar nucleus; the ellipse fitting results are not
satisfactory.

N 1120.  Ellipse fitting results have big errors in the profiles.

N 1667.  The ellipse fitting results were not satisfactory with bigger errors.
The extrapolated magnitude was not accurate enough to be used in the
comparisons.

N 2517.  A lot of stars in the frame.  Ellipse fitting results were
satisfactory in the central region of the galaxy but were contaminated by the
stars in the faintest parts.  The extrapolated magnitudes were not reliable.

M -2-22-17.  Late type galaxy with faint arms.  A lot of bright stars in the
frame.  The ellipse fitting results were not satisfactory in the external parts
due to the galaxy's shape and stars.

M -1-24-1.  Big galaxy with a bright star superposed and a nearby galaxy in the
field.  The ellipse fitting results reflected the field contamination and the
fitting stopped at mu approx. 21.0.

M -2-24-3.  Two stars nearby the galaxy in the frame.  The ellipse fitting
results were contaminated by the stars; the extrapolated magnitude was not
accurate enough.

N 3142.  A bright star caused a gradient in the background around the galaxy.
The ellipse fitting results were contaminated by the star.

M -3-26-30.  Gradients in the background.  The extrapolated magnitude was not
accurate; the curve was not flat at faint levels.

M -1-27-15.  The morphological type was obtained by eye-inspection on plates
from the Palomar Observatory Sky Survey.

M -2-28-1.  Spiral galaxy with a lot of knots.  The flatfielding was not
satisfactory in the B band.  The extrapolated magnitude was not accurate and
the ST ScI magnitude may reflect saturation problems in the scan.

M -2-29-9.  Star light caused a gradient in the background.  The ellipse
fitting could not fit well the galaxy shape.

I 2889.  Bright star in the frame contaminates the galaxy.  The ellipse
fitting results were not satisfactory and the extrapolated magnitude was not
accurate enough.

N 4403 - N 4404.  Galaxies too close.  It was impossible to mask the nearby
galaxy and the results were strongly contaminated.

M -1-32-28.  Faint, irregular galaxy.  It was difficult to fit ellipses.

N 4594.  Galaxy bigger than the frame.  The ellipse fitting stopped at bright
levels.  The results were not accurate enough.

N 5006.  Star nearby the galaxy.  The results were strongly contaminated.

N 5018.  Big galaxy.  The ST ScI magnitude may have been obtained in a
saturated image.  It was not used in the comparison with ST ScI magnitudes.

M -2-34-36.  Galaxy close to N 5094.  It was impossible to mask the nearby
galaxy and the results were strongly contaminated.

N 5584.  Bright star in field.  The ellipse fitting results were contaminated
at faint levels.

M -2-38-15.  Faint stars in the frame.  The ellipse fitting results were not
satisfactory at faint levels.

M -1-52-5.  A lot of stars in the frame, some of them are bright.  The ellipse
fitting results were contaminated by the stars.

N 6945.  Bright star contaminates the outer parts of the galaxy.  Ellipse
fitting results were not satisfactory, reflecting the star light contamination.

M -1-53-1.  Bright star nearby the galaxy.  Outer fitted ellipses were afected
by the star light.

M -1-53-22.  Bright star nearby the galaxy.  Ellipse fitting results were
contaminated by the star light.

M -2-56-7.  Faint spiral galaxy.  Ellipse fitting results were not
satisfactory.  The extrapolated magnitude was not accurate, the curve was not
flat at faint levels.

N 7717.  Bright star nearby the galaxy.  Ellipse fitting results were
contaminated by the star light.