From owner-fitsbits  Thu Jan 15 15:03:41 1998
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To: fitsbits at fits.cv.nrao.edu
Date: Thu, 15 Jan 1998 14:54:23 -0500
From: Doug Mink <dmink at cfa.harvard.edu>
Message-ID: <34BE696F.46ECBB0A at cfa.harvard.edu>
Organization: Harvard University University Information Systems
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Subject: SAOimage 1.21 FITS and IRAF image display released
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SAOimage 1.21, which displays FITS and IRAF .imh images in
the X11 window environment, has just been released.  The major
changes since version 1.20 include adding the ability to read
.imh files written by IRAF 2.11 as well as FITS files and .imh
files written by earlier versions of IRAF.  It should be capable
of reading .imh files independent of the architecture of the
machines on which the images were written or are being displayed.
A bug which kept Digitized Sky Survey WCS coordinates from being
precessed from J2000 to B1950 has also been fixed.  Problems using
the most recent versions as IRAF imtools have been fixed as well.

DATE-OBS is now accepted in the new FITS standard ccyy-mm-dd as
well as the old dd/mm/yy format, although this is only used
to compute the epoch used in converting between J2000 and B1950
coordinates.

Online documentation can be found at

http://tdc-www.harvard.edu/software/saoimage.html

and source code and binary executables for Solaris, SunOS, and
Digital Unix can be found at

ftp://cfa-ftp.harvard.edu/pub/gsc/SAOimage/

-Doug Mink
 Telescope Data Center
 Harvard-Smithsonian Center for Astrophysics
 Cambridge, Massachusetts USA


From owner-fitsbits  Mon Jan 26 09:44:35 1998
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To: fitsbits at fits.cv.nrao.edu
Date: Mon, 26 Jan 1998 10:14:06 +0100
From: Philippe Martinole <martinol at clr40ae.edf.fr>
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Subject: Re: FitsAnimator
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CcdBazar wrote:
> 
> FitsAnimator is a freeware that converts your
> Fits images directly to animated Gif !!!
> http://wwwperso.hol.fr/~pbuttani/ccdbazar/
> 
> Philippe.

I'm the programmer of the freeware Fits Animator.

It's very kind of my friend Philippe to speak
of Fits Animator in this ng but some things
have to be said.

Fits Animator loads images in three formats :
- The Cpa used by the PAP
- The Pic used by Qmips32
- The Fits format

With the Pic and the Cpa, there is no problem
because the thresholds choosen by the observer
are saved in the file with the image.
With most Fits Images, you can adjust the
thresholds in Fits Animator but it will be
less user friendly.
The french programs for amateurs (PAP,Qmips32 
and AIM) use the keywords THRESH and THRESL in
Fits files to save the thresholds.

Hope Fits Animator will be usefull.

Philippe

Ccd Bazar              :
http://wwwperso.hol.fr/~pbuttani/ccdbazar/index.html
Pises Atlas - Prism 97 : http://pages.pratique.fr/~ccavador/
Page Web d'AIM         : http://www.micronet.fr/~phmarty/


From owner-fitsbits  Mon Jan 26 09:44:03 1998
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Date: Sun, 25 Jan 1998 21:38:05 +0100
From: "CcdBazar" <philippe.buttani at hol.fr[Philippe.Buttani]>
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Subject: FitsAnimator
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FitsAnimator is a freeware that converts your
Fits images directly to animated Gif !!!
http://wwwperso.hol.fr/~pbuttani/ccdbazar/

Philippe.





From owner-fitsbits  Thu Jan 29 11:13:16 1998
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To: fitsbits at fits.cv.nrao.edu
Date: Wed, 28 Jan 1998 22:45:42 +0000
From: Damien <DG.Guillaume at ulst.ac.uk>
Message-ID: <34CFB516.6AD763F0 at ulst.ac.uk>
Organization: Ulster University
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Subject: AML, a new format for astronomy based on SGML
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The main goal of FITS was to provide a standard exchange format
for astronomy. With some advantages, especially its flexibility,
it really became used by everybody in astronomy.
However, it is still limited to some data, and is
completly ignoring (as far as I know) astronomical articles or
data on single astronomical objects (amongst many other).
Also, it has become a bit outdated as an exchange format (strange
80 characters lines in the header, no structure, ...)

This is why I started the creation of a new exchange format
for astronomy, within my thesis on information retrieval in
astronomy. It is based on SGML and as such is much more flexible,
readable by any SGML/XML browser/parser, and is appropriate
to the web.
AML is now supporting 4 astronomical data types, but is in
no way restrictive: astronomical objects, articles, tables
and images. Because only characters may be used in SGML,
and because it is easier to manage metadata this way, the big binary
files (such as tables or images) are external to the AML files,
and are referenced in AML as images are referenced in HTML.
I began the creation of an AML browser on the web (a Java applet),
so that anyone can easily read these files.

There are of course some interactions between FITS and AML,
especially for astronomical images: as everybody is now using
FITS, the translation in the two directions must be easy.
To enable an easy translation, I just copied the FITS keywords
and put them into AML in an SGML-way. However, some improvements
may be easy to do on that basis, such as classifying FITS
header information (on the image, on the observations, and so on).

As I hope AML could become a standard format, I cannot
define it alone, and I'm now looking for people interested in
its definition. Maybe it could be seen not as a rival, but as
a new version of FITS...

More information on AML is available at:
http://www.infm.ulst.ac.uk/~damien/these/

Damien Guillaume



From owner-fitsbits  Thu Jan 29 11:16:12 1998
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To: fitsbits at fits.cv.nrao.edu
Date: Thu, 29 Jan 1998 09:17:58 +0000
From: Peter Bunclark <psb at ast.cam.ac.uk>
Message-ID: <34D04946.1808 at ast.cam.ac.uk>
Organization: Royal Greenwich Observatory
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References: <34CFB516.6AD763F0 at ulst.ac.uk>
Subject: Re: AML, a new format for astronomy based on SGML
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You can't replace FITS unless you do handle large binary images. 
Perhaps you could use FITS as your image format, which would be
referenced from AML.

Peter.

Damien wrote:
> 
> The main goal of FITS was to provide a standard exchange format
> for astronomy. With some advantages, especially its flexibility,
> it really became used by everybody in astronomy.
> However, it is still limited to some data, and is
> completly ignoring (as far as I know) astronomical articles or
> data on single astronomical objects (amongst many other).
> Also, it has become a bit outdated as an exchange format (strange
> 80 characters lines in the header, no structure, ...)
> 
> This is why I started the creation of a new exchange format
> for astronomy, within my thesis on information retrieval in
> astronomy. It is based on SGML and as such is much more flexible,
> readable by any SGML/XML browser/parser, and is appropriate
> to the web.
> AML is now supporting 4 astronomical data types, but is in
> no way restrictive: astronomical objects, articles, tables
> and images. Because only characters may be used in SGML,
> and because it is easier to manage metadata this way, the big binary
> files (such as tables or images) are external to the AML files,
> and are referenced in AML as images are referenced in HTML.
> I began the creation of an AML browser on the web (a Java applet),
> so that anyone can easily read these files.
> 
> There are of course some interactions between FITS and AML,
> especially for astronomical images: as everybody is now using
> FITS, the translation in the two directions must be easy.
> To enable an easy translation, I just copied the FITS keywords
> and put them into AML in an SGML-way. However, some improvements
> may be easy to do on that basis, such as classifying FITS
> header information (on the image, on the observations, and so on).
> 
> As I hope AML could become a standard format, I cannot
> define it alone, and I'm now looking for people interested in
> its definition. Maybe it could be seen not as a rival, but as
> a new version of FITS...
> 
> More information on AML is available at:
> http://www.infm.ulst.ac.uk/~damien/these/
> 
> Damien Guillaume


From owner-fitsbits  Thu Jan 29 16:44:46 1998
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To: fitsbits at fits.cv.nrao.edu
Date: Thu, 29 Jan 1998 22:20:10 +0100
From: Damien GUILLAUME <guillaum at newb6.u-strasbg.fr>
Message-ID: <34D0F28A.7643 at newb6.u-strasbg.fr>
Organization: CRC - Universite Louis Pasteur - Strasbourg France
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References: <34CFB516.6AD763F0 at ulst.ac.uk> <34D04946.1808 at ast.cam.ac.uk>
Subject: Re: AML, a new format for astronomy based on SGML
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> You can't replace FITS unless you do handle large binary images.

There's no reason why my system would not be able to handle large
binary images (which is the common case in astronomy).


> Perhaps you could use FITS as your image format, which would be
> referenced from AML.

Yes, it's exactly what I'm doing now. But the meta-information
is duplicated: it is both in the AML file and in the FITS header.
I can also delete the header of the FITS file, but I prefer to
give the two possiblities: pointing from AML to a FITS file,
or pointing only to the raw data. The risk is that someone
may change the FITS file with a usual image processing program
without changing the AML file accordingly. So, my software will
have to check the FITS file each time it loads a corresponding
AML file. But it's not really a problem: the AML files will always
be used with a software, for transfert, translations or browsing.

Damien


