Prism is an Astronomical image processing
and sky Atlas software that I have been writing since 1992. This
software is sold worldwide, have a look to some testimonials and users
links about PRiSM : 1, 2,
3, 4,
5
It is made of 488.000 Delphi line code, and features hundred of functions
to prepare and to take the best benefits of your astronomical observations.
The current release is V7 first released in May, 17th 2008
This
link explains how to preprocess your images by removing the Flat,
Dark and offset. It
like a cookbook that anyone should know.
How
to deal with images from planets distorted by the seeing ? This
unique feature of Prism helps you to recover from it.
Automatic
observation is fundamental for repetitive observations, and helps
to observe even if you have to work early the next day. Check
out here out PRISM is able to make them.
This
is the link where you can register to the mailing list to share
information. This is a forum that can help you to overcome problems
related to PRISM and share your experience.
You can send
email to this mailing list to report bugs and become a Prism
beta tester.
PAP98
is an old version of PRISM, that can be loaded here. It comes
with all the features for free.Just download
and install !
This
page recommands the nicest script editor that can be used to
edit PRiSM script . Color syntax is supported.
This explains
how the Prism's hardware DLL files are handled.
A kind of tutorial
that guides you to preprocess images from digital cameras and obtain
nice deep sky images, from Raw images from SLR cameras such as
Nikon, CANON EOS 10D or 20D.
PRISM and ASCOM
How to install ASCOM platform and hardware drivers
Observations
I'
am fond of astronomical observations. I have built my
own telescope (250mm), running a 1x1K thinned CCD camera. I
am observing at IAU 214 site various kind of objects. I try to find
ideas to overcome the problem of life family and light pollution,
non compliant to observations. Sometimes I am using telescopes belonging
to other people(Valmeca), and to other institution like ESO's telescopes
This
link relates all the result we got with a CCD camera and a 200mm
telescope during the famous August 99 Total solar eclipse in France.
English version here.
It
describes an observing run achieved with the Valmeca 60 cm telescope,
at Puimichel, France. This is the report presented thru these pages.
This
is the image gallery of nice objects I could record with my T250mm
telescope, despite my observing site is not so good for deep sky
observation. Keep hopping..
Image
gallery of observed object with other telescope than the T250 can
be found fellowing this link. You'll find here images from the VLT,
for instance...
Color
image gallery of targets recorded with the T250. Most are very famous
objects of the sky. All recorded in my garden surrounded by lights.
Halpha
filter for deep sky imaging makes possible to record faint structures
of nebulae with full moon ! Have a look here to understand why.
Color
imaging can be really nice when using OIII and Halpha filters. It
allows to record objects with more accurate colors.
Calibrating
exposure time a of given CCD and set of filter is mandatory to get
color images that are properly Signal to Noise Ration balanced.
The Landolt star catalog was used.
These
pages are related to the limiting magnitude you can reach with your
telescope. Selected fields that show stars up to magnitude 26 can
be used to figure out whether a star is actual or not in your image
and test your telescope capabilities.
Remarkable
images of the whole SKY with a thinned 1x1K CCD and photo lens.
As a foreground, the Gemini South telescope in Cerro Pachon.
This
page discuss about the light pollution from human activities and
how it increases the Sky background in CCD images. Discussion undertaken
to optimize the amount of images per exposures versus Signal to
Noise Ratio.
This
is useful to know all the units employed in professional Astronomy,
their meanings and their scope is explained in this pages. Page
always updated ...
CCD observations in suburb site
This is a 4Mb PDF file demonstrating that CCD imaging is possible even under a mediocre suburb light polluted site (In french).
Engarouines observation runs
This sections relates observing runs that where carried out at Engarouines observatory held by L.Bernasconi. This is a very nice place!
DIMM seeing monitor software
The DIMM aims at measuring the seeing (or turbulence) condition in a given observation site. The following page presents a DIMM dedicated software that uses a Webcam and performs measurement 10 times per second.
Telescope
making is a very nice hobby when the weather is not suitable for
observing. It allows you to build your telescope for a real cheap
price and to control the whole system. I have been making telescopes
for 16 years, like Schmidt Cameras up to 300mm, Newton telescope
up to 400mm. This involve the knowledge of mechanics, optics, electronic
and computer programming.. a real challenge where improvment is
always possible due to technology changes.
This
page is the index to many pages that are describing all the constructions
phases of a 250 mm telescope. This telescope have to fulfill the
requirement of being able to observe alone over the whole night.
Currently, this is the telescope I am employing mostly.
I have purchased
in nov 2003 an Intes Alter M703 telescope. This is the main entrance
to get all the pages related to it : test and use with CCD camera
and wabcams.
These
are Powerpoint slides presented during the Aude 2001 Seminar (French
Pdf file). This aims at presenting concept for remote automatic
observation, and how to avoid the unreliable gas factory that a
remote telescope could be if design phase and thoughts are not undertaken.
G11 have mount have been tested here. Installed drives are MCMT II system.
This page relates M703 Intes tests
Telescope
optics
Telescope
optics is a very attractive field, as well as designing using ray
tracing software like Zemax,
manufacturing the parts and make the sky test. I have been involved
in this field since 1985. Schmidt plates, correctors, main mirror
are fields that I enjoy to polish.
Shows
here, the set of BVRI filter to be chosen to carry out nice
color images and photometric observations. Considerations
concerning the CCD are presented.
This
is the information to design a Wynne corrector for Newton
telescopes intrinsically affected by coma. The use of such
corrector should be mandatory for telescope above a diameter
of 300mm...
In
1992, I wrote a book to explain how to achieve a complete
Schmidt camera. This book describes how to cut the Schmidt
plate and all other details. This is scanned files that have
been compressed downto 3.7Mo.
Turbulence
affects high resolution imaging, this link explains how. Also
relation with the use of webcams in astronomy is discussed
as well as optical mirror quality versus turbulence trade-offs
Shack
Hartmann is a powerfull setup to test and tune accurately telescope
optics. This page explains the principle and a shows a setup
that has been assembled and tested.
I
have written a Shack Hartmann real time software that allowed
me to carry out measurments and to reduce them "in a
real time fashion".
This
is a fascinating field : the CCD detectors used for Astronomy. Say
that 20 years ago, a film had quantum efficiency of 2%, whereas
the CCD has now up to 95%. CCD has revolutionized the way of doing
Astronomy, allowing amateurs using a 20cm telescope to compete with
4m telescopes when they were using photographic plates. This field
is the field where I am working professionally..
This
section provides a comparison between the Kodak Kaf1602E and Marconi47-10
CCD for deep sky imaging in Astronomy. This link gives hints to
make you mind up about these two great devices.
The
Chungara CCD controller is a low noise system able to read out many
kid of CCD. It uses the ethernet interface to transfer the data
to the computer. This is an home made design achieved with B.Gaillard.
This
page is a test review about the Maxcam47-10 from FLI. It shows the
pros and cons of such a camera. This test has been written to be
the most objective. Pictures of the camera parts can be seen.
This
is a presentation held during the Aude seminar in 2000 (French Pdf
file). It explains how this interface for transferring pixels to
a PC can be applied to the Audine
camera.
This
THE official web site of the Ethernaude project : The ethernet interface
for the Audine camera.
This
link is a compilation of all the Marconi (E2V or EEV) devices in
a nutshell. You'll find here also all the datasheet in PDF format
of these devices.
Electronics
Designs
Electronic
design is part of telescope making, it starts by driving RA/DEC
axis of telescopes, proceed to assistance to focusing, to drive
a dome, to drive a CCD camera, etc etc.. Electronic is nowadays
unavoidable to point the telescope towards an invisible target,
achieve automated telescope. This section will provide general purpose
designs, as well design related to telescope driving.
Sometimes
RS232 serial cables are too long and the signal can be too weak.
This page explains how to overcome this issue by the use of a simple
design.
This
section provides all the information related to a custom- made Embedded
Ethernet Interface that can be used with a CCD camera to transfer
data to a WINNT based OS PC. This design can be used for all application
requiring high speed data transfer to a PC.
This
shows how a set of general purpose high power switches can be driven
by the Embedded Ethernet interface. The goal of such a design is
to enable the PC to switch on/off devices remotely. This is a basic
brick for an automated remote observatory. This design
can open-close a dome, switch on the telescope drives, telescope
CCD, etc etc...
MCMT
is system that turns your telescope into a goto telescope. Based
only on step motors. Telescope up to 600mm can to point everywhere
in the sky. Have a look, it worth to be seeing.
Digital
focusing is an important milestone to achieve in order to run automatic
telescope. This link presents a design based on stepping motor and
ethernet link.
The
current EOS remote control system provided for performing astronomical
images is insufficient . This page shows a system developped
for the purpose of achieving long exposures images, and allow
direct and total control from a PC.
Weather
and climate
What
could be Astronomy without any basic knowledge of weather forecast
and climate ? Since weather is an important component of astronomical
observation, it disserved its whole section.
Whole
Europe Suniness data is quite impossible to find. So based on satellite
images I have made my own statistics for year 2001. This pages explain
also the method to achieve these results. New : Good statistics here
This
sections shows a whole set of charts related to France climate and
its suniness. This is the data compiled by meteo France for many
years.
This is the link
to DRSD UK meteorology, this is the web site that shows the nicest
satellite images and compute your own statistics. Also this is one
is not so bad : meteosurf
Photography
That's
an hobby I would have loved to make it my job...may be I am too
bad, and/or not brave enough.. Photography section will show pictures
from the trips I have made around the world. If you want to use
the picture, please, be kind to ask permissions and credits to use
it for your own purpose...
By
clicking here, you will access the index web page to all other sections
related to my pictures.
Direct
link to the Observatory photo pages.
Updated by Cyril Cavadore (Janv 1st 2007), ,
all right reserved. Ask for authorization to use images and documents.
To know more about me and my professionnal resume, have
a look here.