Images taken on October 11th 2002 by Steve Havas, and processed by myself.
R filter
median of images 1 to 8 & 10 ( 300 s exposures ), R filter:
sum of images 1 to 8 & 10 ( 300 s exposures ), R filter:In the following image (from the median image), the arrow is drawn from the position of 10/04 new object to a possible candidate.
Notice that this candidate is very doubtful for being quite close to the noise.
Comparing to the coordinates given by the Zetas:
The movement of the new candidate doesn't correspond: it is moving up instead of moving down.
Effect of the 'seeing'.
Comparing Red DSS (on the right) to the median image (on the left):
One can see how the image of a punctual source (star) is spread out in a spot whose size is the 'seeing', in arcsec. Star 1 appears fainter, and star 2 becomes almost indistinguishable from noise.That is why Nibiru may be almost indistinguishable from noise for the moment.
Original 'fits' files from S. Havas: >download .tar.gz<
