▄▓ ▓▄
▄▄▄█▀▀ ▓▄ ▄▓ ▀▀█▄▄▄
▄█▓▀▀ ▓█ ▓▀▀▄▄▄▄▄ ░ ░ ▄▄▄▄▄▀▀▓ █▓ ▀▀▓█▄
▐▓▌ ▓ ░░▒▓█▓▓█ █▒▓▒█ █▓▓█▓▒░ ▓ ▐▓▌
▀▄ ░░ ▓ ░░░▓▓░░░░ █ █ ░░░▓▓░░░░▓ ░░ ▄▀
█ ░░ ▄▄▄▄▄ ▀▀▓▀▀ ▓ ░▓ ░░ ▓█
█ ░ ▄▓███▒░▐▓░ ░▓▀█▓░░ ▀ ░░░░░ ▄▄▓ ░░ █
█░ █▓███▒▒░░░ ░░▐ ░ ░▓▓ ▓ ▓■▄▓▓▄░░ ░█
█░ ▓▓██▓▒░░ ░▓░ ░ ▄▄▄▄ ▓ ▓ ░ ▓ ▓ ░██▀▀▀██▄ ░ █
█░ ▓███▓▒░░ ▄███████▄ ▄ ░▓ ▓██ ░▒▓██▄░ █
▓░▐███▓▒░░ ▐▒ ██▓▒░ ▀█░▓▓▐█ ░▒▓██▄▄ ■▓█▄ ▓
█░ ██▓▒▄ ▄▄▓▒ ▓▒░▀███▄▄ █▐▓▌█ ░░▒▓█▓▓██▄▄▄██▓ █
█ ▄██░ ▀█████▀▓ ▒░ ▀▀██▄█▌█▀ ▌█▀ ░▓▓██▀ ▒▓▓█ █
█░ ▐██▓▒░ ░▒█ ▄ ▓█████▐▐▌▐ ▄ ▐░██ ░▒▓██ █
█ ░▀▀██▄ ▒▓██ ▓ ▐▄▄░ ██▌▀██▀█░█▌ ░░█▄ ▄█▓ █
█ ░░ ▄██████████▓ ▀██▄██▄ ░▓██▄▓▓▀▓ ░ █▓███████▓░ █
█ ▄▄▄▄▄▄ ░ ░ ░ ▓ █▓█▀ ██▀ ▓ ▓ ▓▀▀ ▄▄▄▄▄▄ █
▄█▀ ▀▓▄ ▓▓▓▀ ▀ ▓▓▓▓░ ▄▓▀ ▀▀█▄
▀ ▄▓▀▀▀▀▀▀▀▓▄ ▄▓▀▀▀▀▀▀▀▓▄ ▀
▐▓▌▓▓▄█▀▓▄ █▓▓▒░ ░▒▓▓█ ▄▓▀█▄▓▓▐▓▌
█░▓▐ ▐▓▐▌ ░ ░ ▐▌▓▌ ▐▌▓░█
▀▓▄█▀ ▄▓▄▀ ░ ░ ▓ ▓ ░ ░ ░▀▄▓▄ ▀█▄▄▀
▄██▀▀░ ░ ░ ▓ █ ▓ ░ ░ ░ ▀▀██▄
▐██▌ ░ ░ ░ ░ ▓ ▓ ░ ░ ░ ░ ░▐▓█▌
▓██▄ ▓ ░ ▄▄▄■▓■▄▄▄▄ ▓░▄▓██
▀▀███▄█▀ ▀█▄███▀▀
▄ ▄▄▄▄▄▄▄▓ │ ▓▄▄▄▄▄▄▄ ▄
▀▀▄ │ ▄▀▀
░▐▓ ──GAMMA─RAY─BURST── ▓▌░
▄█▀ │ ▀█▄
▄▄▄█▀▀ │ ▀▀█▄▄▄
▄██▀▀ ▀▀██▄
▐▓▌▀ ▀▐▓▌
▀ P R O U D L Y P R E S E N T S ▀
MEDIA.CYBERNETICS.AUTOQUANT.X.V2.1.3_X86-GRB
_ __ ___ ____ _____ ______ _______ ____________________________
DATE.......: 07/02/2009
SUPPLIER...: GRB
CRACKER....: GRB
PACKER.....: GRB
TYPE.......: Crack
PROTECTION.: HASP
SIZE.......: 18x.5.00MB
URL........: http://www.mediacy.com/index.aspx?page=AutoDeblurVisualize
▄ ▄ ▄ ▄
▀▀▄ ▄▀▀
░▐▓ RELEASE NOTES ▓▌░
▄█▀ ▀█▄
▄▄▄█▀▀ ▀▀█▄▄▄
▄██▀▀ ▀▀██▄
▐▓▌▀ ▀▐▓▌
▀ ▀
All microscopes are limited by the laws of
physics, and these laws state that when
light passes through a medium, that light
will bend. This is one of the most common
causes of haze and blur in microscopy
images. Deconvolution can correct this
problem, not only removing the haze and
blur, but restoring vital detail to datasets.
AutoDeblur« offers the most powerful
deconvolution tools available for life
science research. Retrieve better data
from your images using the most complete
suite of 2D and 3D algorithms available.
It offers an advanced Blind Deconvolution
algorithm which is both iterative and
constrained.
Unlike other deconvolution products,
AutoDeblur does not require the manual
calibration and measurement of the point
spread function (PSF). Instead, it
constructs the PSF directly from the
collected data set. AutoDeblur works with
widefield epi-fluorescence, DIC,
transmitted-light brightfield and most
Confocal microscopes including two-Photon
and spinning disk.
In addition to the full complement of
algorithms, AutoDeblur offers several other
advantages as well. It is based on a
multiDimensional platform, capable of
handling 3D time-series datasets. Instead
of loading each time point one at a time,
and processing them through a batch
process, they can be loaded and processed
as a single dataset.
Another advantage of AutoDeblur is the
ability to load a nearly limitless number
of channels, freeing you from the
constraints of the world of RGB. You also
have full control over the display of each
channel - choose from the lists of custom
colors, wavelengths, dyes, or color mapping
to best display your dataset.
Let AutoDeblur show you what you 've been
missing in your images, because better data
means better science.
▄ ▄ ▄ ▄
▀▀▄ ▄▀▀
░▐▓ RELEASE INFOS ▓▌░
▄█▀ ▀█▄
▄▄▄█▀▀ ▀▀█▄▄▄
▄██▀▀ ▀▀██▄
▐▓▌▀ ▀▐▓▌
▀ ▀
1. extract
2. install
3. replace in program files
*:\Program Files\Media
Cybernetics\AutoQuant X2
4. Gamma Ray Burst is Shining.
▄ ▄ ▄ ▄
▀▀▄ ▄▀▀
░▐▓ GROUP INFO ▓▌░
▄█▀ ▀█▄
▄▄▄█▀▀ ▀▀█▄▄▄
▄██▀▀ ▀▀██▄
▐▓▌▀ ▀▐▓▌
▀ ▀
Gamma-ray bursts (GRBs) are the most luminous electromagnetic events
occurring in the universe since the Big Bang.
Since GRBs in metal-rich galaxies like the Milky Way are rare, mass
extinctions due to GRBs may only happen once per billion years.
Dedicated To Quality And Not To Quantity
G R E E T I N G S
to N0NE
J O I N - W A N T E D
Looking for:
Experienced keygenners
Experienced unpackers
Experienced crackers
and
AFFIL SITES
NOT RENTED - NO US NO DE
C O N T A C T
Take a look at the Milky Way
email: NoWay Hose
www : Sure
irc : Sure
__________________ _________________ _________________ __________________
!DZr 01.01.2K9!