>download .fits< >.gzip version<
Images taken on September 21th 2002 by Steve Havas, and processed by myself.
R filter
median of images 1 to 20, R filter:
sum of images 1 to 20, R filter:All Luminance
median of images 1 to 8, all luminance:
sum of images 1 to 8, all luminance:
Median of 3 "darks": >download
.fits.gz<
Original 'fits' files from S. Havas: >download
.tar.gz<
DSS with the position given by the Zetas for September 15th 2002
(green circle). The green box show the field of the images taken on September,
21th.
ESO-DSS 1:=> Nothing new appears on September 21th images. But is Nibiru detectable in such conditions ?
ESO-DSS Red:
ESO-DSS InfraRed:
Problem of the size of Nibiru
According to these informations:
http://www.zetatalk.com/usenet/use90661.htm
on September, 15th, Nibiru's diameter is ~ 0.3 arcsec, and its swirl of dust and moons is ~ 1.2 arcsec ( = 33% the size of Uranus, see below).
Due to the faintness of the object, and the fact that its size is still lower than the 'seeing' (~ 1 arcsec), Nibiru is still very difficult to detect, and may be invisible on S. Havas' images.
