From nobody Mon May  4 11:03:20 1998
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From: Andreas Haerpfer <ah@staufen.cip.physik.uni-muenchen.de>
Newsgroups: sci.astro.research
Subject: Re: [?] LateX .bib files for astrophysics papers
Date: 4 May 1998 08:26:34 -0500
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sina@css-b-359.umd.edu (Ramin Sina) writes:

> Hi all, I was wondering if there are  bibliography files for papers in 
> astrophysics which can be used with latex. If yes, where can I find them?
> I am in particular looking for a .bib file with many enteries for cosmic ray 
> papers.

Hi,

I doubt that you will find any comprehensive and ready to use bibtex
files which are at least halfways up to date.  However, you may create
them at your own by using the ADS abstract service at

	http://adswww.harvard.edu

Follow the links `Abstracts' -> `Astronomy and Astrophysics Abstract
Service' to a query form where you can specify authors, title words,
text keywords and a lot more.  On the bottom of the query results'
page you can select `Return BIBTEX reference list' and then say
`Retrieve all references' -- that's it.

The only thing that perhaps remains to do is to adapt the original
labels to your personal needs.

BTW: a search for the keywords `cosmic' && `ray' yielded 8112 hits!

Hope that helps.

Andi

-- 
Andreas Haerpfer  <Andreas.Haerpfer@physik.uni-muenchen.de>
PGP fingerprint:  87 6D F8 06 AD 4A AA B3  6D 6B E2 63 61 61 DA BB
*** This message was entirely written with recycled electrons ***

From nobody Tue May  5 14:30:48 1998
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From: gei@head-cfa.harvard.edu (Guenther Eichhorn)
Newsgroups: sci.astro.research
Subject: Re: [?] LateX .bib files for astrophysics papers
Date: 5 May 1998 08:50:24 -0500
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You can build bibliographies in different formats with the Astrophysics
Data System Abstract Service:

<URL:http://adsabs.harvard.edu/ads_abstracts.html>

The ADS allows you to output the reference lists in several formats,
including bibtex and the reference format for LaTex.

The ADS allows you to search the astronomical literature (as well as
literature on Astronomic Instrumentation).  The Astronomy database
contains over 400,000 references, the Instrumentation database over
500,000).  The returned references contain links to a number of other
information providers (eg. on-line journals, data centers, object
databases, scanned journal articles).

This service is a NASA funded project, and access is free world-wide. 
We have mirror sites in France and Japan to improve access times for
non-US users.  I am currently discussing another mirror site in Chile.

If you have any questions about the ADS, please contact us at:

<mailto:ads@cfa.harvard.edu>

Guenther
---------------------------------------------------
Dr. Guenther Eichhorn        |  gei@cfa.harvard.edu
Project Scientist            |  Phone: 617-495-7260
Astrophysics Data System     |  Fax:   617-496-7577
Smithsonian Astrophysical Observatory

From nobody Thu May 14 11:04:58 1998
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From: Peter R Newman <see.my@web.pages>
Newsgroups: sci.astro.research
Subject: Re: Velocity components
Date: 12 May 1998 08:43:06 -0500
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Randy Stegemeyer wrote about his radio telescope:

First, a big well done on what you have so far!

>
>      What I want to do now is to correct the doppler shifts for the
> motion of the earth moving around the sun, and for the rotation of the
> earth itself.  I find all kinds of information on coordinate systems
> and converting between them, but I have not found any formulas for
> actually calculating the velocity components in various directions.
[snip]
>      If someone could direct to a reference, or provide the formulas
> themselves,

The book "Observational Astronomy" by D. Scott Birney (1991, Cambridge
University Press) gives a fairly complete guide to the reduction of
radial velocities on pages 216-223.  This is a good undergraduate level
text in general, although primarily aimed at optical observations.

Also, I think any edition of the Astronomical Almanac (a US Naval
Observatory/HMSO publication) will give the equations you need, plus all
the constants, but I don't have a copy to hand to check.

Good luck, and do continue to publish your results!

Pete
-- 
http://sa1.star.uclan.ac.uk/~prn
Happy is he who has been able to learn the causes of things - Virgil

From nobody Thu May 14 11:05:46 1998
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From: chandler@cfara1.harvard.edu (John Chandler)
Newsgroups: sci.astro.research
Subject: Re: Velocity components
Date: 12 May 1998 08:48:18 -0500
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Randy Stegemeyer (hamradio@oz.net) wrote:
:      What I want to do now is to correct the doppler shifts for the
: motion of the earth moving around the sun, and for the rotation of the
: earth itself.

What about the motion of the Sun with respect to the LSR or the LSR
with respect to the Galaxy or...  Even leaving those aside, the
question is not so simple.  You have to specify what level of
precision you want, in order to know what sorts of approximations will
be acceptable (and you probably want to use all the approximations you
can).  For example, the rotational velocity on the Earth's surface is
less than .5 km/s -- if you don't need the velocity to that level, you
can ignore the rotation entirely.

--
John F. Chandler             chandler@cfa.harvard.edu

From nobody Fri May 15 13:51:57 1998
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From: Wilfred Walsh <clarges@dempster.gaean.re>
Newsgroups: sci.astro.research
Subject: Re: [?] Automated object detection+classification in 3d data cubes?
Date: 13 May 1998 08:39:18 -0500
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Brad Gibson wrote:
> 
> I'd be interested in finding any pointers to references on the automated
> detection of objects in 3-dimensional data cubes.  


Brad,

There is a program in IDL and miriad called clfind that does this. It
originates from J. Williams at CfA I believe, who documents the program
at http://cfa-www.harvard.edu/~jpw/clfind.html. I think you need to get
the BIMA version of miriad from 
http://bima.astro.umd.edu/bima/programmer.html rather than the ATNF
version. Also, check with the Parkes multibeam guys (eg Lister) as they
must be doing something similar to find the dwarfs in their data.

Wilfred Walsh

From nobody Fri May 15 13:51:59 1998
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From: Volker Ossenkopf <ossk@zeus.ph1.uni-koeln.de>
Newsgroups: sci.astro.research
Subject: Re: [?] Automated object detection+classification in 3d data cubes?
Date: 15 May 1998 08:01:28 -0500
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Brad Gibson wrote:
> I'd be interested in finding any pointers to references on the automate=
d
> detection of objects in 3-dimensional data cubes. =20

Gaussclumps is a FORTRAN code to find objects in a 3-D data cube
(normally position and velocity) that can be approximated by Gaussians=20
in all three dimensions. I don't know whether this fits your
needs in galaxy detection.

Gaussclumps was described in detail by Stutzki & Guesten 1990,=20
ApJ 356, 513. The code with some explanations is available by
anonymous ftp at zeus.ph1.uni-koeln.de/pub/gaussclumps .

Best wishes
		Volker

---------------------------------------------------------------------
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Fax.: 0221 4705162                               Universit=E4t zu K=F6ln
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From nobody Wed May 20 14:17:24 1998
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From: Clive Page <cgp@nospam.le.ac.uk>
Newsgroups: sci.astro.research
Subject: Re: [?] Cross-correlating catalogs
Date: 20 May 1998 08:20:17 -0500
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>>Can anyone recommend tools for or literature about cross-correlating
>>astronomical catalogs?  I'd like to compare two catalogs and find
>>sources that are present in both of them, to within some specified
>>position uncertainty.  Vizier has a huge number of catalogs, but I

If you have access to ESO/MIDAS you will find it can do that on MIDAS
tables, but you have to import the data first.   The Starlink CURSA package
can do something similar, and will work directly on FITS tables.  If I
remember rightly, however, VIZIER will only export FITS ASCII tables, which
makes the computations very inefficient.  Perhaps converting to FITS binary
tables would be a useful step.  One could use FTOOLS to do that.

-- 
-- 
Clive Page,
Dept of Physics & Astronomy,        
University of Leicester.

