EAS INSTRUCTIONSElectronically transmitted abstracts have several advantages including: speed of delivery, savings in mailing, and electronic processing in the conference office eliminating typing errors.
Generally speaking, if you know how to use email, submitting your
abstract electronically is by far the easiest approach and will ensure
the highest quality reproduction in the abstract book. Your electronic
abstract will be processed upon receipt by a
In sending e-mail messages with abstracts,
please make absolutely sure that the messages are not
HTML/MIME encoded.
In the following template, replace strings of upper case
characters, ie. AUTHOR ADDRESS, with information appropriate to the
content of your abstract.
SEE NOTE 3 FOR CAPITALIZATION RULES ON
TITLES AND AUTHORS.
Please refer to the example abstracts for
clarification. (Note that lines beginning with % are "comments" and
not processed by
The above template has multiple sections, each of which require
some explanation which is given below.
If you submit an abstract electronically and you receive
confirmation of successful receipt, you need do nothing more.
DO NOT
send us an additional paper copy of your abstract.
The following information is only for those of you without the
capabilities of viewing or printing your abstract locally, to whom we
are offering the following option. After you have completed your
abstract according to the directions, email it to our special test
address:
test-hrms2010@pso.com.pl.
Upon receipt, your document
will be processed by our
If you do not have
When your abstract is ready it
should be e-mailed to
eas-hrms2010@pso.com.pl
without any added material.
While not
required, placing the word "abstract" on the subject line is a
convenient identifier.
When you fill in the template, make sure not to use characters from your national
character set, such as
ü,
ä,
ö,
ß in German names,
ç, é, è in French names,
and æ, ø, å in Danish and Norwegian names. You may have keys on your keyboard with these characters,
but our English-language
You can put pictures (i.e. graphics) in your abstract by using the
Note the graphics commands in the abstract:
Please note that we can only handle one form of document for
electronic submission, and that
For those who are interested in learning more about
compiler,
supporting all the capabilities of
-2
. However, you do not need
any real knowledge of
to submit an abstract electronically. All
you need to do is type into the template below, with any ordinary
(ASCII) text editor, the required information. To submit the abstract,
simply email the completed template to
eas-hrms2010@pso.com.pl.
Besides the template, we have several
other aids to help you make the submission process as painless as
possible. We have set up a test facility so you can see how your
abstract will appear in the Abstract Book, if you are unable to
compile it locally (see item 1 below the template). On our WWW site we
provide two helpful pages. One
(
help page) shows how to
construct the common special symbols that appear in conference
abstracts. The other page
(view Example Abstracts) gives several
example
files and a picture of how each will appear.
.)
% ------ begin electronic abstract submission template -----
% ------ Version 2.0 last modified on Tue Feb 03 1998 -----
\documentclass[12pt]{article}
\usepackage{praha}
%\category{poster}
%\category{lecture}
\timereq{MINUTES REQUIRED}
\comment{COMMENT TEXT}
\title{TITLE OF YOUR ABSTRACT}
\author{\underline{FULL NAME OF SPEAKER}, OTHER AUTHOR(S)}
\address{AUTHOR ADDRESS}
\author {FULL NAME OF AUTHOR FROM OTHER LOCATION}
\address{ADDRESS OF AUTHOR FROM OTHER LOCATION}
\begin{document}
\maketitle
TEXT OF YOUR ABSTRACT
\end{document}
% ------ end electronic abstract submission template ------
-2
commands 'documentclass' and
'usepackage' specify the style your printed abstract will have. To
preview your abstract locally you must place the file praha.sty where
your
compiler can find it (typically in the same directory as
your abstract file) before processing. If you received these
instructions by email, you will have received the style file in a
separate email message, the body of which you must save as the file
praha.sty. If you are viewing these instructions on our Web site,
download the file praha.sty from it.
If at all possible
you are encouraged to view or print your abstract locally before submission.
Remember we must treat abstracts submitted electronically, just as paper
abstracts arriving by post. In particular, iteration on accepted electronic
abstracts is a forbidden process.
-2
compiler. If that step is
successful, you will receive an email reply to that effect. You will
then be able to on the WWW a picture of
your abstract as it will appear in the program by following the
directions in the email confirmation. If your submission is rejected
by our compiler, your email reply will inform you of the failure of
your submission with information about the problem. Once you are
satisfied with your abstract's appearance, re-submit it as an
"official" abstract to
eas-hrms2010@pso.com.pl.
Please note
the following caveats: (1) The conference organizers will not look at
the "test" abstracts. (2) In the directory storing the "test" abstracts,
files older than 24 hours will be deleted at regular intervals. (3) The
conference reserves the right to shut down this service if our computer
becomes overloaded. If you need this service, plan ahead and utilize it
well in advance of the abstract submission deadline.
-2
at your location, but
DO use an
earlier LaTeX or TeX compiler, you can still do most of the previewing
locally, but a few extra words of explanation are in order. The style
file, praha.sty, uses
-2
specific code and therefore will not run
under older compilers. Correspondingly praha.sty interprets a number of
command lines in the template, e.g.,
\timereq,
\address,
etc. For
those of you with the older compilers, avoid difficulties by
previewing your abstract text with your own compiler, then just follow
a "fill-in-the-blank" approach with the command lines in the template
that your compiler does not support. The completed abstract should be
acceptable when it is processed by the
-2
compiler here. Its
appearance can be tested by the procedure described above.
command lines
"\begin{document}", and
"\maketitle",
the body of the abstract should be entered. It can take
advantage of all the special symbols, and control (superscripts,
subscripts, etc.) available in
documents, but may be a simple
text only. Examples of such material are available on either our web
site or via anonymous ftp. A single example will be found at the end
of this document.
processor does not
understand them, so please do not use them. If you do,
it is likely that the special characters will be missing in the abstract
printed in the abstract book, or that they will be replaced by other characters that make no sense
in your language. But even if you are called Bürger, Picqué, Møllendal, or pirko, do not despair!
In
your names
are written B\"urger, Picqu\´e, M{\o}llendal, and
{\v S}pirko, respectively, and if you write them like that in the
input file,
they will appear with the correct special characters in the printed abstract.
Each special character can be expressed in standard
in a way that
our processor can understand. Our
help page gives you the codes
for a selection of them.
environment
"filecontents" and
the macro package
"psfig". The graphical display to be
inlined in your abstract must be available as an encapsulated PostScript (.eps) file; an eps file is in ASCII format
and can be transmitted as an e-mail message. Abstract 5 of our
sample abstracts gives an example of an abstract
with a spectrum displayed in it. The file sent as an e-mail message must have the following format:
\begin{filecontents}{fig1.eps}
.
.
Here you place the entire eps file with your picture;
you must choose a name for the eps file, here it is fig1.eps.
After the "\end{filecontents}" command you place the
usual LaTeX file with the abstract.
.
.
\end{filecontents}
% ------ begin electronic abstract submission template -----
% ------ Version 2.0 last modified on Wed Nov 08 1995 -----
\documentclass[12pt]{article}
\usepackage{praha,psfig}
\category{poster}
%\category{lecture}
%\timereq{15}
%\comment{COMMENT TEXT}
\title{MEASUREMENTS OF D$_2$S$_2$ NEAR 2 THz: PRECISION
BROADBAND SPECTROSCOPY WITH COSSTA}
.
.
.
.
\vspace{3mm}
\centerline{\psfig{figure=fig1.eps,width=3.5in,height=2.5in}}
.
.
.
\end{document}
Important note:
For sending abstracts with graphic content (eps
format) we support uuencode, base64, and quoted-printable
encoding only.
was chosen for its support by
several American professional societies and widespread use by the
worldwide scientific community.
the
following resources are available:
Below is the
- A Document Preparation System -
User's Guide and Reference Manual. 2nd edition
Addison-Wesley, Reading, 1994.
Companion. Addison-Wesley, Reading, 1994.
text that produced the abstract viewable on our web
site as example Abstract 0.
% ------ begin electronic abstract submission template -----
% ------ Version 2.0 last modified on Wed Nov 08 1995 -----
\documentclass[12pt]{article}
\usepackage{praha}
%\category{poster}
\category{lecture}
\timereq{15}
\comment{Session on electronic spectra or astrophysics}
\title{CYANOPOLYYNE CATIONS AS CARRIERS OF
A SET OF DIFFUSE INTERSTELLAR BANDS}
\author{\underline{JAMES K.~G.~WATSON}}
\address{Steacie Institute for Molecular Sciences,
National Research Council of Canada,
Ottawa, Ontario, Canada K1A 0R6}
\begin{document}
\maketitle
It is proposed that a set of diffuse interstellar bands (DIBs) can
be attributed to the $\widetilde B{}^2\Pi-\widetilde X{}^2\Pi$
electronic transitions of the cyanopolyyne cations, HC$_{2n+1}$N$^+$,
based on comparisons with laboratory observations in Ne matrices
by Forney et al.$^1$ For HC$_7$N$^+$ the DIB $\lambda6614$ is
assigned as the $0_0^0$ origin band, and $\lambda\lambda6426$,
6196, 5982, and 5850 to transitions to upper-state fundamental
vibrations. The three-peaked structure of $\lambda6614$ under
high resolution$^{2,3}$ is assigned as $P$ and $R$ branches of the two
subbands $^2\Pi_{1/2}-{}^2\Pi_{1/2}$ and $^2\Pi_{3/2}-{}^2\Pi_{3/2}$,
with the central pair of branches overlapping. The $0_0^0$ band
of HC$_9$N$^+$ is assigned to $\lambda7562$, with vibrational bands
at $\lambda\lambda7358$, 6919, and 6521, while the $0_0^0$ band of
HC$_{11}$N$^+$ is assigned to $\lambda8531$, with vibrational bands
too weak to identify. These are all relatively sharp DIBs, with
full widths at half maximum (FWHMs) in the range 1.7--3.1 cm$^{-1}$.
Assignments are less satisfactory for
shorter members of the series. The $0_0^0$ bands of HC$_5$N$^+$ and
HC$_3$N$^+$ may be $\lambda\lambda5797$ and 5110, respectively,
but the former seems to have a rather narrow $PR$ separation under high
resolution, although its FWHM of 2.9 cm$^{-1}$
lies in the above range, while the latter
is much broader (FWHM = 45 cm$^{-1}$) than higher members of the
series. The first member of the series, HCN$^+$, does not have a
$\ldots\pi^3\pi^4\gets\ldots\pi^4\pi^3$ electronic transition of this type.
\vspace{1em}
\noindent
1. D.~Forney, P.~Freivogel, J.~Fulara, and J.~P.~Maier, J.~Chem.~Phys.,
102, 1510 (1995). \hfil\break
2. P.~J.~Sarre, J.~R.~Miles, T.~H.~Kerr, R.~E.~Hibbins, S.~J.~Fossey,
and W.~B.~Somerville, Mon.~Not.~Roy.~Astron.~Soc.~277, L41 (1995).
\hfil\break
3. P.~Ehrenfreund and B.~H.~Foing, Astron.~Astrophys., 307, L25 (1996).
\hfil\break
\end{document}
% ------ end electronic abstract submission template ------
praha.sty Download praha.sty file
SampleAbstr.html View sample abstracts

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