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To: fitsbits at fits.cv.nrao.edu
Date: 28 Feb 1999 19:56:41 GMT
From: pikovsky at rz.uni-potsdam.de ( Arkady Pikovsky)
Message-ID: <7bc71p$dcu at zeppelin.rz.uni-potsdam.de>
Organization: University of Potsdam
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Subject: Scan to fits
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Hi there !
Does software exist (public domain preferred :) ) to
save scanned images into FITS format (Windows NT) ?

[if possible reply by e-mail]

Thanks

--
--------
A. Pikovsky

pikovsky at rz.uni-potsdam.de

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.                     **** CFITSIO v2.0 Release ****

This is an update on the latest features that have been added to version
2.0 of the CFITSIO library for reading and writing FITS files, which is
available at

     http://heasarc.gsfc.nasa.gov/fitsio

1.  Any table column, regardless of the datatype, can be read as a
character string.  The format of the returned string is determined by the
TDISPn display format keyword if it exists, otherwise a default format 
based on the datatype of the column is used.

2.  A subsection of a FITS image can be opened by appending the starting
and ending pixel numbers (and optionally, a pixel increment) for each
dimension to the filename with the IRAF-style syntax: 

   filename.fits[xstart:xend:xstep, ystart:yend:ystep]

For example, "myfile.fits[1:512:2, 2:512:2]" will open a 256x256 pixel
image consisting of the odd numbered columns and the even numbered rows of
the input image.

3.  Added transparent support for the ESO HIERARCH keyword convention for
keyword names longer than 8 characters or that contain ASCII characters not
allowed in normal FITS keywords.  Thus, CFITSIO can effectively read and
write keywords like:

     heliocentric_correction = -45.5   / velocity
     HST WFPC2 Exposure Time = 1200.0  / exposure time in seconds
     heater:temp:#34 = 0.8  / degrees C

These types of keywords are stored in the FITS header using the HIERARCH
keyword convention that fully conforms to the FITS Standard.

4.  Added new support routines for dealing with World Coordinate System
keywords, which makes it easier to call Doug Mink's WCSlib routines for
converting between plate and sky coordinates. 

5.  Added support for opening images or arrays that are contained in a
single cell of a binary table, with the syntax:

     "filename.fits[extname; col_name(row_number)]" 

where 'extname' is the name of the table extension, 'col_name' is the name
of the column and 'row_number' is the number of the row in the table that
contains the array.  This array is opened so that it appears to the
application program as though it is opening a FITS image in the primary
array.

6.  Added 2 new routines to read any consecutive string of bits as an
unsigned integer from a Bit 'X' or Byte 'B' column.

7.  Added support for VMS-style directories in the input file name 
(e.g. "disk:[user.subdir]myfile.fits").

8.  Added supporting project files and instructions for building CFITSIO
under Windows NT with the Microsoft Visual C++ compiler.

9.  Made major improvements to both the C and Fortran User's Guides.  These
Guides are available on line at:
 C: http://legacy.gsfc.nasa.gov/docs/software/fitsio/c/c_user/cfitsio.html
 Fortran:
    http://legacy.gsfc.nasa.gov/docs/software/fitsio/c/f_user/fitsio.html

As a reminder, version 2.0 of CFITSIO also supports these features:

1.  CFITSIO can read IRAF format image files (.imh files) as well as
    FITS files. Thus, any program that uses CFITSIO to do image analysis
    of FITS images can directly read IRAF images as well.

2.  FITS files on the internet can be directly read by providing the
    full FTP or HTTP URL as the input file name.

3.  Input FITS files can be filtered or modified at run-time based on a
    user-supplied expression that is appended to the name of the input
    file.  This allows users, at run time, to:

  a) select a subset of the rows in a table which satisfy an 
     arbitrarily complex boolean expression

  b) create new table columns whose values are calculated 
     as a function of other columns and/or keywords in the table

  c) create a virtual FITS image by binning/histogramming
     the values in one or more table columns.  This is most often 
     used to create an image by binning a list of X and Y coordinates
     for each event in a table.

4.  The data input and output routines in CFITSIO has been optimized 
    to achieve high throughputs, with typical rates of 5 - 10 MB/s
    on current generation machines.

Many people and institutions have contributed to these new features in
CFITSIO:  Please refer to the User's Guides for the list of
acknowlegements.
-- 
____________________________________________________________________
Dr. William Pence                          pence at tetra.gsfc.nasa.gov
NASA/GSFC Code 662         HEASARC         +1-301-286-4599 (voice)     
Greenbelt MD 20771                         +1-301-286-1684 (fax)

From owner-fitsbits at kochab.cv.nrao.edu  Fri Mar  5 09:38:26 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Thu, 04 Mar 1999 20:49:40 +0000
From: Duncan Munro <dmunro at sfu.ca>
Message-ID: <36DEF1E4.7125 at sfu.ca>
Organization: SFU ARO
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Reply-To: dmunro at sfu.ca
Subject: Re: Scan to fits
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you could use Xfree86, GIMP, Xscanimage, SANE and Linux or OS/2 to scan 
into the GIMP and save the scan as a fits file. Alternatively you could 
use PMview ((NT?) or OS/2) and a scanner driver to do the same. I don't 
think PMview supports 16bit fits files though.

Duncan


Arkady Pikovsky wrote:
> 
> Hi there !
> Does software exist (public domain preferred :) ) to
> save scanned images into FITS format (Windows NT) ?
> 
> [if possible reply by e-mail]
> 
> Thanks
> 
> --
> --------
> A. Pikovsky
> 
> pikovsky at rz.uni-potsdam.de

From owner-fitsbits at kochab.cv.nrao.edu  Sun Mar  7 14:31:43 1999
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Date: 5 Mar 1999 14:16:05 -0800
From: sla at ucolick.borg (Steve Allen)
Message-ID: <7bpl35$a35$1 at dei.ucolick.org>
Organization: UCO/Lick Observatory
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Subject: OBJECT keyword redux
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Last April in response to the call for comments on NOST 100-1.2 Don
Wells proposed that the value of the OBJECT keyword should conform to
the recommendations of the Designations Task Group of IAU Commission
5.

This led to a lively discussion in s.a.f that lasted through June
where two camps emerged.  One camp effectively agreed that the use of
the OBJECT keyword should be tightened for the sake of archival
applications.  The other camp objected that the original loose
definition of the OBJECT keyword had already led to development of
software and observer habits which could not easily be changed to
conform with a tightened definition.

The discussion ended without a clear consensus.

We are now about to deploy the new observing user interface whose
prototype was mentioned last year.  It has the ability to modify an
object name provided by the observer so as to generate a single FITS
card which contains a synopsis of several other important FITS cards.
The prototype used the OBJECT keyword as the location for this
information, principally because this has been the keyword which
is listed by IRAF when it scans a directory full of files.  Our
decision on whether to continue to "abuse" the OBJECT keyword
is imminent.

I would like to re-open this can of worms.  Are there any further
thoughts on the matter of how the OBJECT keyword should be used?  Or
is the issue moot because the NOST panel will be changing the
recommendations for OBJECT?
-- 
Steve Allen          UCO/Lick Observatory       Santa Cruz, CA 95064
sla at ucolick.borg     Voice: +1 831 459 3046     FAX (don't): +1 831 459 5244
WWW: http://www.ucolick.borg/~sla               PGP public keys:  see WWW
Junk mail is irrelevant -- my return address has been assimilated.

From owner-fitsbits at kochab.cv.nrao.edu  Wed Mar 10 13:09:12 1999
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Date: Wed, 10 Mar 1999 13:00:23 -0500
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Subject: Re: OBJECT keyword redux
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Steve Allen wrote:
> 
> I would like to re-open this can of worms.  Are there any further
> thoughts on the matter of how the OBJECT keyword should be used?  Or
> is the issue moot because the NOST panel will be changing the
> recommendations for OBJECT?

There has been no significant change to the definition of the OBJECT
keyword in the latest version of the NOST FITS Standard (which
incidentally, is expected to be publicly released within a couple weeks):
"Object Keyword - The Value field shall contain a character string giving a
name for the object observed".  The NOST panel decided it was out of scope
of its charter to introduce new restrictions or rules for the value of the
OBJECT keyword or to define a new reserved keyword such as IAUDESIG,
without the prior general agreement of the FITS community.

-Bill Pence
____________________________________________________________________
Dr. William Pence                          pence at tetra.gsfc.nasa.gov
NASA/GSFC Code 662         HEASARC         +1-301-286-4599 (voice)     
Greenbelt MD 20771                         +1-301-286-1684 (fax)

From owner-fitsbits at kochab.cv.nrao.edu  Thu Mar 11 14:53:28 1999
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Subject: HIERARCH keywords in CFITSIO
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Here is some information about support for the HIERARCH keyword convention
in CFITSIO, for those who may be interested:

--------------------------------------------------------------------------

At the request of ESO scientists, the CFITSIO library (available at
http://legacy.gsfc.nasa.gov/fitsio) has been enhanced to support their 
convention for hierarchical FITS keyword names.  A typical keyword using 
this convention looks like:  

HIERARCH ESO INS FOCU POS = -0.00002500 / Focus position

Basically, this convention uses the FITS keyword 'HIERARCH' to indicate that this
convention is being used.  Then the actual keyword name begins in column 10 and
can be composed of a number of subfields.  In this example, 'ESO' indicates the
domain of the keyword, 'INS' is the catagory, and 'FOCU' and 'POS' are subsystems
to which the keyword applies. The equals sign marks the end of the keyword name
and is followed by the usual value and comment fields just as in ordinary FITS
keywords. Further details of this convention are described at
http://arcdev.hq.eso.org/dicb/dicd/dic-1-1.4.html (search for HIERARCH).

This specific use of the HIERARCH convention is probably of limited interest 
outside of ESO itself, but it has been implemented in CFITSIO in a general way 
so that a much broader range of keyword names are now supported, including names
up to 67 characters in length, and names containing other ASCII text characters 
that would otherwise not be allowed in a standard keyword name.  For example, 
all the following keywords can now be read or written with CFITSIO.

12345678901234567890123456789012345678901234567890123456789012345678901234567890
HIERARCH LongKeyword = 47.5 / This keyword has > 8 characters, and mixed case
HIERARCH XTE$TEMP = 98.6 / This keyword contains the '$' character
HIERARCH Earth is a star = F / This keyword contains embedded spaces
HIERARCH ThisIsOneOfTheLongestPossibleKeywordsAllowedWhenUsingThisConvention = 9

Application programs do not need to specify the 'HIERARCH' part of the keyword
name when reading or writing keywords with CFITSIO (although it may be specified
if desired).  When writing a keyword, CFITSIO first checks to see if the keyword
name is legal as a standard FITS keyword (no more than 8 characters long and
containing only letters, digits, or a minus sign or underscore). If so it writes
it as a normal FITS keyword, otherwise it uses the hierarch convention to write
the keyword.   As shown in the last example above, the maximum keyword name
length is 67 characters, (leaving only 1 space for the value field!).  A more
practical limit would be about 40 characters, which would leave enough room for
most keyword values.  Currently CFITSIO returns an error if there is not enough
room for both the keyword name and the keyword value on the 80-character card,
except for string-valued keywords which are simply truncated so that the closing
quote character falls in column 80.  Note that this hierarch convention can be
combined in CFITSIO with the HEASARC long string value convention to produce
keywords with both long keyword names and long string values extending over
multiple keywords (the keyword name must all fit on the first card however). In
the current implementation, CFITSIO preserves the case of the letters when
writing the keyword name, but it is case-insensitive when searching for a
keyword.  Thus, the first keyword in the examples above could be read by looking
for the keyword 'LONGKEYWORD' or 'Longkeyword', or any other combination of upper
and lower case. The current implementation allows any ASCII text character (ASCII
32 to ASCII 126) in the keyword name except for the '=' character.  A space is
also required on either side of the equal sign, but in principle this could be
relaxed to provide room for 2 more characters in the other keyword fields.

Obviously, this convention should be used sparingly, or not at all in FITS files
that are intended to be imported into other data systems that don't support this
convention.  On the otherhand, this convention will enable some new applications
that require longer keywords to use the FITS format. 

- Bill Pence
____________________________________________________________________
Dr. William Pence                          pence at tetra.gsfc.nasa.gov
NASA/GSFC Code 662         HEASARC         +1-301-286-4599 (voice)     
Greenbelt MD 20771                         +1-301-286-1684 (fax)

From owner-fitsbits at kochab.cv.nrao.edu  Fri Mar 12 09:46:17 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Fri, 12 Mar 1999 06:09:23 GMT
From: dmunro at sfu.ca (Duncan Munro)
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Organization: Simon Fraser University
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Subject: Fitsblink 2.28 Xfree86-OS/2 Port
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The latest version of the Fitsblink for Xfree86-OS/2 (and others) is
available at:

http://kronos.ijs.si/~jure/fitsblink/fitsblink.html

Here are a few of its features:

>Fitsblink is a program for analysis of astronomical images, especially of asteroids and comets. It has the following features: 

>     On-screen comparison of the FITS images. It can load and display a number of images, each with its own grey level correction and translation relative to other
>     images. The images can be alternately displayed with an adjustable time delay between them; 
>     fitsblink can load images in FITS, compressed FITS (.fts.Z) or gzipped FITS (.fts.gz) formats; 
>     if the header contains correct WCS keywords, it will show the celestial coordinates at the cursor position; 
>     images can be displayed in grey level or color mode; 
>     Fitsblink can create star lists, import star lists, match star lists with GSC and USNO SA catalogs; 
>     after successful match with a catalog it is possible to do astrometry and mail results in MPC format. 

Duncan Munro

From owner-fitsbits at kochab.cv.nrao.edu  Mon Mar 15 16:27:33 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Mon, 15 Mar 1999 14:56:31 -0500
From: Tom McGlynn <tam at silk.gsfc.nasa.gov>
Message-ID: <36ED65EF.88196A87 at silk.gsfc.nasa.gov>
Organization: NASA Goddard Space Flight Center -- Greenbelt, Maryland USA
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Subject: Web Page Describing FITS Libraries
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Periodically this group gets a request for pointers
to a FITS library which will meet the requester's
needs.  I thought it might be useful to have a
single Web page that provided pointers to FITS libraries
available in various languages.  I've put one
in the HEASARC Web site at

   http://heasarc.gsfc.nasa.gov/docs/heasarc/fits/fits_libraries.html

It provides a tabular overview of all the libraries, a
capsule summary of the capabilities of the
packages and links to where each package can be downloaded.

So far this has only the libraries that I was personally
aware of or that were easily findable on the Web.  I'd be very
happy to add more libraries -- and to correct errors
in the descriptions.  I've been trying to emphasize
libraries that are usable independently of a particular
software environment, and which are easily downloadable.

Since it started with the libraries I know of, it's strongly
biased to libraries developed at the HEASARC [including the two
I'm responsible for], but I'm hoping to get pointers to alternatives
and I'll be happy to add them.

Note that all of this is 'without warranty'.  I'm simply providing
pointers to what others have placed on the Web.  I've not personally
used most of the libraries so I cannot vouch for their quality.
Even a buggy library may be helpful to someone starting from scratch.

I'd be especially interested in filling gaps in the language coverage.
E.g., I don't know of any Ada or Pascal FITS libraries.

Any suggestions for how this might be improved are welcome.


		Regards,

		Tom McGlynn
		NASA/HEASARC

From owner-fitsbits at kochab.cv.nrao.edu  Tue Mar 23 14:23:03 1999
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Date: Tue, 23 Mar 1999 14:18:50 -0500 (EST)
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From: Eric Greisen <egreisen at valen.cv.nrao.edu>
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Subject: New drafts of WCS papers
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Mark and I have been working to implement the understandings of the
last ADASS in Illinois in the form of 3 wcs papers.  The drafts of
papers I and III are now available for comment.  The long Paper II on
celestial coordinate projections needs a bit more work, although Mark
has made great progress.

Paper I: Representations of World Coordinates in FITS

     ftp://ftp.cv.nrao.edu/NRAO-staff/egreisen/wcs.ps

Paper III: Representations of Spectral Coordinates in FITS

     ftp://ftp.cv.nrao.edu/NRAO-staff/egreisen/scs.ps

are in PostScript form for printers with modern PostScript fonts (as
expected by A&A Supp).  They have no long figures.

I invite comment, preferably directed to me rather than filling the
fitbits with detail at this stage of the proceedings.  Of course, wider
comment will need to be made later and you may feel it appropriate
even now.  The spectral paper has a hole marked "HERE" where
suggestions for dealing with complex optical instruments might be
made.  One thought is that optical images that have spectra of
numerous objects overlayed on an RA-dec image may not even be amenable
to a FITS representation at that stage of their processing.  They may
only e suitable for tables of spectra at a later stage of analysis.
AS a radio astronomer, I do not know about such things and need your
help.

Thanks,

Eric W. Greisen (egreisen at nrao.edu)

and

Mark Calabretta (mcalabre at atnf.csiro.edu)

From owner-fitsbits at kochab.cv.nrao.edu  Fri Mar 26 12:02:48 1999
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Date: Fri, 26 Mar 1999 12:01:04 -0500 (EST)
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From: Eric Greisen <egreisen at valen.cv.nrao.edu>
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Subject: new draft
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Peter Teuben has read wcs.ps and reported a few typos and made some
suggestions.  These are reflected in a new draft to be found at
     ftp://ftp.cv.nrao.edu/NRAO-staff/egreisen/wcs.ps

The changes are an additional sentence at the end of the section on
CUNITj concerning the number of characters needed and changes to Table
2 and to the description of Table 2.  A numerically concrete example
is now given and the choice of parameters described.  Sadly, the paper
now folds about an inch onto page 10.

I invite people to consider wcs.ps and scs.ps at the above address and
send their ideas on to me.

Thanks, Eric

From owner-fitsbits at kochab.cv.nrao.edu  Sat Mar 27 00:18:45 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Fri, 26 Mar 1999 22:24:27 GMT
From: ttruong at cfa.harvard.edu (Trieu Truong)
Message-ID: <36fc0822.1653745 at cfanews.harvard.edu>
Organization: Harvard University
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Subject: FITS to GIF/TIFF/etc.
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Hello.

I'm a newbie to FITS and was hoping someone might be kind enough to
tell me if there is PC software that will allow me to manipulate FITS
files and convert them to GIF/JPEG/TIFF/etc. files so that I can put
the pics up on the Web.  I've tried FTOOLS, but that didn't allow me
to save the files as anything but postscript files, and Photoshop (my
main image editor) couldn't read the .ps files.  Please please help.

TIA

ps. I am aware of MIRA from Axiom Research.  Is this my only option?

From owner-fitsbits at kochab.cv.nrao.edu  Sun Mar 28 20:47:40 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Sun, 28 Mar 1999 15:50:10 +0100
From: Patrick Chevalley <pch at geneva.crosswinds.net>
Message-ID: <36FE3392.7083D45A at geneva.crosswinds.net>
Organization: AstroPC
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Subject: Re: FITS to GIF/TIFF/etc.
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If you use Photoshop there is a plugin for working with FITS file.
You can find it at : http://www.fan.net.au/~eddiet/fitsplug.html

I have a utility ( AstroIma ) in my QuickCam page that can view FITS 
images and then save it in BMP format, but it is only in French.
http://www.astrosurf.org/astropc/qcam


Patrick Chevalley

http://www.astrosurf.org/astropc

From owner-fitsbits at kochab.cv.nrao.edu  Mon Mar 29 10:03:53 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Mon, 29 Mar 1999 16:39:55 +0200
From: "Martino Nicolini" <tecnico at artiglio.it>
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Organization: Customer of Flashnet S.p.A. - http://www.flashnet.it
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Subject: Re: FITS to GIF/TIFF/etc.
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Hello,

Astroart is a new 32bit software for astronomical image processing and
analysis (for Windows95-98 and NT (TM)). It supports FITS file format (you
can easly edit the header) as well as 20 commercial CCD formats like SBIG,
HiSIS, Starlight, Pixcell, Seti 245, Cookbook, Lynxx, Electrim or a generic
free format for particular cameras; some other nice features are a true real
time zoom and 3D window.
It has advanced filters like a new adaptive algorithm, gaussian high pass,
convolution and deconvolution (Lucy-Richardson and Maximum Likelihood)
rotational gradient (Larson-Sekanina) and many others...
Using a simple drag&drop you can manipolate groups of images with the
advanced tools in the PreProcessing window (in just a few seconds you can
calibrate for dark, flat and bias and align and sum a set of images); create
your own macros for many pourposes etc.
Another very powerful feature is the easy astrometric and photometric
calibration with an integrated Star Atlas based on the G.S.C. catalogue: it
fully support the WCS (World Coordinate System) with standard FITS keywords
so you can correctly read sky coordinates in your images also with other
UNIX based and advanced software like IRAF, MIDAS, XEPHEM etc. now on Linux
platform.

After our efforts in developing and producing this big package, we decided
to share with the CCD astronomical amateur community a freeware-demo version
(in english and italian), available at:

http://www.sira.it/msb/astroart.htm

Only the advanced features are not supported, but you can load, display,
read the WCS etc. in every kind of images and, above all, it does not expire
with the time: enjoy it forever!

The freeware-demo version will allow you to save FITS images only in the BMP
format

Best regards,

MSB
Fabio Cavicchio and Martino Nicolini
Ravenna, Italy.


Trieu Truong ha scritto nel messaggio
<36fc0822.1653745 at cfanews.harvard.edu>...
>Hello.
>
>I'm a newbie to FITS and was hoping someone might be kind enough to
>tell me if there is PC software that will allow me to manipulate FITS
>files and convert them to GIF/JPEG/TIFF/etc. files so that I can put
>the pics up on the Web.  I've tried FTOOLS, but that didn't allow me
>to save the files as anything but postscript files, and Photoshop (my
>main image editor) couldn't read the .ps files.  Please please help.
>
>TIA
>
>ps. I am aware of MIRA from Axiom Research.  Is this my only option?
>


From owner-fitsbits at kochab.cv.nrao.edu  Mon Mar 29 13:39:15 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Mon, 29 Mar 1999 17:47:27 GMT
From: dunmunro at direct.ca (Duncan Munro)
Message-ID: <36ffb9d8.14837494 at news.direct.ca>
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Get Fitsview. It is a freeware fits viewer which allows you to save
into the bmp format.

you can get it at:

http://www.cv.nrao.edu/fits/os-support/

Duncan

On Fri, 26 Mar 1999 22:24:27 GMT, ttruong at cfa.harvard.edu (Trieu
Truong) wrote:

>Hello.
>
>I'm a newbie to FITS and was hoping someone might be kind enough to
>tell me if there is PC software that will allow me to manipulate FITS
>files and convert them to GIF/JPEG/TIFF/etc. files so that I can put
>the pics up on the Web.  I've tried FTOOLS, but that didn't allow me
>to save the files as anything but postscript files, and Photoshop (my
>main image editor) couldn't read the .ps files.  Please please help.
>
>TIA
>
>ps. I am aware of MIRA from Axiom Research.  Is this my only option?
>

From owner-fitsbits at kochab.cv.nrao.edu  Mon Mar 29 15:05:13 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Mon, 29 Mar 1999 15:02:32 -0500
From: Doug Mink <dmink at cfa.harvard.edu>
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Trieu Truong wrote:
> I'm a newbie to FITS and was hoping someone might be kind enough to
> tell me if there is PC software that will allow me to manipulate FITS
> files and convert them to GIF/JPEG/TIFF/etc. files so that I can put
> the pics up on the Web.

I display FITS images in my viewer of choice (usually SAOimage because I
maintain it, but sometimes SkyCat, SAOtng, or ds9), adjust the contrast
(darker, smoother backgrounds compress better and make smaller GIF
images),
use xwd to dump the image to a disk file and either xv or the PBMPLUS
xwd2pnm and ppmtogif programs to make GIF files for WWW use.  I have
found the the PBMPLUS pnmscale program reduces image dimensions more
cleanly than XV does.  My latest results are at

http://tdc-www.harvard.edu/software/wcstools/imwcs/imua2.html

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

From owner-fitsbits at kochab.cv.nrao.edu  Wed Mar 31 10:42:49 1999
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To: fitsbits at fits.cv.nrao.edu
Date: Wed, 31 Mar 1999 17:37:29 +0200
From: Francois Ochsenbein <francois at simbad.u-strasbg.fr>
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I read with interest the "Representation of world coordinates
in FITS" proposal -- this convention widely used will benefit
the publication! But I was suprised to find there the
Appendix B with the OGIP conventions on units in FITS that,
as far as I know, were never approved (was WCS approved ?)

There are the following points of disagreements:

1. Compared to the IAU Style Manual:
   In table3: 
   - the radian (symbol rad) is missing
   - the Ohm sould be written with a capitalized O,
         to be consistent with its origin (physicist's name)
         and uppercase greek symbol.
   In table 4: 
   - the symbol of the year is the single-letter a (not yr)
   - the sun-based units (solar mass at least) is missing
   - the letter 'b' alone is the symbol of the barn (cross-section)
   - for the Angstroem: should be capitalized for the same reasons
     as Ohm above -- and should or not an 'e' appended after the
     'o' to reflect the original accentuation of the o ?

2. The usage of the ** for exponentiation is not really a good
   idea -- it only makes sense for fortran programmers.
   Why not a single-letter symbol like the carret (^) most
   likely familiar to many more persons ? 

3. The usage of the blank is not a good idea either, even though
   it looks more like the printed text, it complicates its
   acquisition from simple-minded software (e.g. Perl) without
   better readibility  -- "count /s" doesn't look better than
   "count/s" 

4. Some usual abbreviations like "ct" for count, or "ph" for
   photon, could be accepted .
   And some "miscellaneous" units could be useful as well like
   "beam" or "bit"

5. Finally, the usage of the trigonometric functions applied to
   units raises the question of the units of their argument and
   therefore the inconsistency with the inverse function, the degree
   being adopted instead of the radian. My personnal suggestion
   would be to drop completely the trigonometric functions applied
   to non-dimensionless units -- I never found such expression in
   the literature, and this would be bad physics anyway !

Are these conventions about units in FITS definitive ?
The documentation of astronomical catalogues available from
the data centres (ADC, CDS, ...) describe over 60,000 columns;
roughly 50% of these columns are unitless, and therefore about
30,000 columns have attached units carefully standardized
to allow automatic conversions. (description at 
http://vizier.u-strasbg.fr/doc/catstd-3.2.htx ) 
I would hesitate to change these anyway... but would appreciate
any comment / argumentation !

======================================================
Francois Ochsenbein
         Centre de Donnees astronomiques de Strasbourg
Internet: francois at astro.u-strasbg.fr
   Phone: +33 3 88 150 755
     Fax: +33 3 88 150 740
    http://cdsweb.u-strasbg.fr/CDS.html
    Post: Observatoire Astronomique
          11, rue de l'Universite
          67000 STRASBOURG, France 
======================================================

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Date: Wed, 31 Mar 1999 17:58:59 +0200 (MET DST)
From: Lucio Chiappetti <lucio at ifctr.mi.cnr.it>
To: fitsbits at fits.cv.nrao.edu
Subject: Re: wcs.ps
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On Wed, 31 Mar 1999, Francois Ochsenbein wrote:

> Appendix B with the OGIP conventions on units in FITS that,
> as far as I know, were never approved (was WCS approved ?)

a statement on the official approval status of both would be appreciated.

> There are the following points of disagreements:

I would say I agree with some points

> 3. The usage of the blank is not a good idea either, [..]
> 4. Some usual abbreviations like "ct" for count, or "ph"  [...]

I'm indifferent to other

> 1. Compared to the IAU Style Manual:
> 5. Finally, the usage of the trigonometric functions applied to

(as I would not care much for standardization of what are essentially labels,
I would expect human readability to be more important than computer
readability, and few programs needing to INTERPRET (parse) such data, but just
use them "as they are" to label plots or table captions).

But I **definitely disagree** on this one :

> 2. The usage of the ** for exponentiation is not really a good
>    idea -- it only makes sense for fortran programmers.
>    Why not a single-letter symbol like the carret (^) most
>    likely familiar to many more persons ? 

----------------------------------------------------------------------------
Lucio Chiappetti - IFCTR/CNR - via Bassini 15 - I-20133 Milano (Italy)      
----------------------------------------------------------------------------
L'Italia ripudia la guerra [...] come    Italy repudiates war {...] as a
mezzo di risoluzione delle controversie  way of resolution of  international
internazionali                           controversies
                [Art. 11 Constitution of the Italian Republic]
----------------------------------------------------------------------------
For more info : http://www.ifctr.mi.cnr.it/~lucio/personal.html             
----------------------------------------------------------------------------

From owner-fitsbits at kochab.cv.nrao.edu  Wed Mar 31 11:30:58 1999
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Date: Wed, 31 Mar 1999 11:28:58 -0500 (EST)
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From: Eric Greisen <egreisen at valen.cv.nrao.edu>
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My e-mails made it clear (I thought) that these are draft proposals.
They have not been approved by anyone other than their authors.  Of
course, they have been around in some form or other for a long time
and already reflect a great deal of discussion and compromise.  Both
authors are, in fact, unhappy about bits of them but we are eager to
get some sort of agreement, so long as it is workable and correct.

The authors do not expect for the appendices to be part of the adopted
standard, although one or more of them could be.  Certainly, we expect
the pixel regularization to be included if possible in an adopted
standard, but we do not expect that the added nomenclature for tables
and the specific units suggestions to be official standards.  Instead,
they may well end up in the same category as the "heap" used with
binary tables, namely an understood but informal convention.  I
adopted most of the units suggestions of OGIP since theirs is the only
set actually documented and in wide use.  I did drop non-degrees in
units for angles and may have made other mistakes in the
transcription.  I will reply in more detail about the other comments
after I get to study them in detail.

Eric Greisen

From owner-fitsbits at kochab.cv.nrao.edu  Wed Mar 31 12:35:45 1999
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Date: Wed, 31 Mar 1999 12:35:07 -0500
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From: Don Wells <dwells at cv.nrao.edu>
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	<Pine.OSF.4.05.9903311753260.26193-100000 at poseidon.ifctr.mi.cnr.it>
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Lucio Chiappetti writes:
 > On Wed, 31 Mar 1999, Francois Ochsenbein wrote:
 > 
 > > Appendix B with the OGIP conventions on units in FITS that,
 > > as far as I know, were never approved (was WCS approved ?)
 > 
 > a statement on the official approval status of both would be appreciated.

The FITS WCS conventions beyond those described in the earliest FITS
papers have not been subject to a vote by any of the FITS committees. 
Therefore, the current NOST FITS standard does not discuss them.

Conventions on units for FITS beyond those recommended in the FITS
papers have not been subject to a vote by any of the FITS committees. 
Therefore, the current NOST FITS standard says in its section 5.3 that
units should conform to the IAU style manual and 'for angular
measurements given as floating point values and specified with
reserved keywords, degrees are the recommended units'. 

The OGIP conventions on units are an agreement among certain
high-energy astrophysics data groups. The 'wcs.ps' draft is proposing
that a version of them become a recommended practice to augment the
IAU Style Manual rules. The units conventions used by the data centers
(CDS, ADC, etc) for data tables should be regarded as another draft
proposal for FITS.  I expect that a merger of the two sets of
conventions would be best; see:

http://vizier.u-strasbg.fr/doc/catstd-3.2.htx
http://heasarc.gsfc.nasa.gov/docs/heasarc/ofwg/docs/general/ogip_93_001/ogip_93_001.html
    
The current negotiation of the WCS conventions for FITS is an
opportunity to agree on a recommended practice for interchanging
computer character string representations of units, a problem which
the IAU Style Manual did not address.

-Don
-- 
  Donald C. Wells      Scientist - GBT Project        dwells at nrao.edu
                    http://www.cv.nrao.edu/~dwells
  National Radio Astronomy Observatory                +1-804-296-0277
  520 Edgemont Road,   Charlottesville, Virginia       22903-2475 USA

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Date: Wed, 31 Mar 1999 16:17:52 -0500 (EST)
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From: Eric Greisen <egreisen at valen.cv.nrao.edu>
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To: Francois Ochsenbein <francois at simbad.u-strasbg.fr>
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Subject: Re: wcs.ps
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A revised draft of wcs.ps may be found at the usual address:
     ftp://ftp.cv.nrao.edu/NRAO-staff/egreisen/wcs.ps
It contains a change to the table of special table keywords and the
discussion of that table.  And it contains lots of changes re units.
I ask the OGIP people in particular to review these changes to see if
they are okay with you.

Francois Ochsenbein writes:
 > I read with interest the "Representation of world coordinates
 > in FITS" proposal -- this convention widely used will benefit
 > the publication! 

     Thank you; the authors agree or we would not have worked on this
paper for 7 years and much aggravation.

>  But I was surprised to find there the
 > Appendix B with the OGIP conventions on units in FITS that,
 > as far as I know, were never approved (was WCS approved ?)

     I felt that we needed at least to make recommendations for usage.
I left Appendix B's status with respect to official adoption vague to
see whether the community will be willing to accept guidance on this
issue.  But, everything in the papers wcs.ps, ccs.ps (not available
yet), and scs.ps is a proposal.  None of it is adopted as yet.

     I have reviewed both the OGIP document and the WWW page you cited
and have made a bunch of changes to wcs.ps.  Thank you for pointing me
in this direction.  I believe that every unit in your www page is now
in wcs.ps.  For specifics, see below:

 > 
 > There are the following points of disagreements:
 > 
 > 1. Compared to the IAU Style Manual:
 >    In table3: 
 >    - the radian (symbol rad) is missing

     Angular units are a problem.  The original FITS papers specified
that degrees would be used and they have been widely used for angles
projected onto images.  Coordinate descriptions purporting to obey the
proposed conventions of Paper II (ccs.ps) will be required to use
degrees throughout.  Nonetheless, wcs.ps should include 'rad' and
other standard angular measures for other uses, such as in tables.
Angles without specified units will be assumed to be in degrees.

 >    - the Ohm should be written with a capitalized O,
 >          to be consistent with its origin (physicist's name)
 >          and uppercase Greek symbol.

      Agreed - but neither your www site nor OGIP used the upper case
so I think we should stay lower.  IAU does not capitalize any of the
named units (e.g.newton) when spelling out the unit in case that
matters to anyone.

 >    In table 4: 
 >    - the symbol of the year is the single-letter a (not yr)

      Yes.  However, your www site also allows 'yr', so I have added
the IAU-standard 'a'

 >    - the sun-based units (solar mass at least) is missing

      Special mass units in general were missing and I also added all
the solar ones on your www page.

 >    - the letter 'b' alone is the symbol of the barn (cross-section)

       The IAU does not include this unit and your www page also uses
'barn' so I think we leave this one.

 >    - for the Angstroem: should be capitalized for the same reasons
 >      as Ohm above -- and should or not an 'e' appended after the
 >      'o' to reflect the original accentuation of the o ?

       The IAU does not include the unit.  I suggest angstrom because
that is what OGIP has used and your www page does not allow for it.

 > 
 > 2. The usage of the ** for exponentiation is not really a good
 >    idea -- it only makes sense for fortran programmers.
 >    Why not a single-letter symbol like the caret (^) most
 >    likely familiar to many more persons ? 

       Actually the up arrow is also tied to mark-up languages such as
TeX which, like Fortran, will become unfamiliar to people in time.
There is no reason not to allow both and I agree that the up arrow
looks more like "raising to a power".  It will be harder to typeset
with TeX (e.g. \char'136 or inside a \verb) than simple text.

 > 
 > 3. The usage of the blank is not a good idea either, even though
 >    it looks more like the printed text, it complicates its
 >    acquisition from simple-minded software (e.g. Perl) without
 >    better readability  -- "count /s" doesn't look better than
 >    "count/s" 

      You know - I rejected this when I first read it and have since
come around to think that you are right.  I have rewritten the text to
allow but strongly discourage blanks.

 > 
 > 4. Some usual abbreviations like "ct" for count, or "ph" for
 >    photon, could be accepted .
 >    And some "miscellaneous" units could be useful as well like
 >    "beam" or "bit"

     I added 'ct', 'bit', and 'beam'.  Your list does not include 'ph'
so I left 'photon' as the only one of those.

 > 
 > 5. Finally, the usage of the trigonometric functions applied to
 >    units raises the question of the units of their argument and
 >    therefore the inconsistency with the inverse function, the degree
 >    being adopted instead of the radian. My personal suggestion
 >    would be to drop completely the trigonometric functions applied
 >    to non-dimensionless units -- I never found such expression in
 >    the literature, and this would be bad physics anyway !

Again I am going from rejecting your idea to accepting it.  There are
numerous physical quantities that vary e.g wrt log(wavelength) or
cos(elevation).  In the first case, the values do depend on whether it
is log(nm) or log(m).  But the second case, cos requires an argument
in whatever units that function requires and produces a unitless
result that is independent of whatever units we thought of the
elevation in.  Therefore I have dropped all trigonometric functions
but have left log, ln, etc.

 > 
 > Are these conventions about units in FITS definitive ?
 > The documentation of astronomical catalogues available from
 > the data centres (ADC, CDS, ...) describe over 60,000 columns;
 > roughly 50% of these columns are unitless, and therefore about
 > 30,000 columns have attached units carefully standardized
 > to allow automatic conversions. (description at 
 > http://vizier.u-strasbg.fr/doc/catstd-3.2.htx ) 
 > I would hesitate to change these anyway... but would appreciate
 > any comment / argumentation !

    I have adopted all of the suggestions at this site, but one.
Write m2 does not instinctively mean m^2 or m**2 when I read it and so
I prefer the nomenclature of OGIP for exponents even though it does
require more characters.  At some point human readability must enter
this discussion.

    Many thanks for your close reading of this document and your
suggestions.  I look forward to hearing from you again...

Eric Greisen

