This indicates that these LSB galaxies follow the same clustering properties as their giant counterparts and are parts of the greater structure of the group. Although they do not fill the gaps, they certainly widen the filamentary structure of the universe. With such high numbers, I conclude that these galaxies contribute to the total light of the cluster at least as much as the bright members. Considering that my data is still limited and my sample is not complete to extremely faint objects, the contribution I calculate is a conservative number with the tendency to increase. Our view of the universe from a telescope is confined in a conical volume.
Nearby objects are few due to the volume being small nearby and increasing with distance.
As a parenthesis here, this is the reason why nearby extragalactic astronomy is more difficult than distant extragalactic astronomy. Also, objects that are nearby maybe so large on the sky that we see right through them. Another interesting result was the detection of a large concentration of LSB galaxies around the isolated galaxy NGC1291. This may well be an LSB cluster, and there are scenaria that suggest isolated galaxies are accompanied by LSB satellites. This is an important issue as it explores LSB galaxies in environments different to the cluster environment I have been researching.