Format Examples | Submit | Replace | Cross Reference | Publication Note | e-mail addresses of E-print Archives |
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Text:
Your paper should be a TeX or LaTeX file with lines not longer
than 80 characters.
All nonstandard TeX macros or definitions
must be defined within the file, style files not
available at the E-prints archives
should be sent with the file.
Figures:
It is recommended to include
postscript figures
into the paper with psfig or epsfig.
Send your figure files together with the TeX file (and style files)
packed (tar-compressed and uuencoded) using the
uufiles utility.
Header:
The electronic archives need a special header
preceding the
text (+figures) file in the following format:
\\ Title: (required) Author: (required) Comments: (recommended) Report-no: (if appropriate) Subj-class: (if appropriate) Journal-Ref: (if appropriate) MSC-class: (if appropriate) \\ Abstract (or other short description, must be less than 24 lines) \\
Examples: (submission to hep-ph) \\ Title: Charmonium Production via Fragmentation at DESY HERA Authors: Bernd A. Kniehl (MPI Munich), Gustav Kramer (Hamburg) Comments: 32 pages (Latex), 12 figures (Postscript) Report-no: DESY 97-110, MPI/PhT/97-001 Journal-Ref: Phys. Rev. D56 (1997) 5820-5833 \\ (Text of abstract) \\ (submission to physics) \\ Title: A superconductive undulator with period length of 3.8 mm Authors: T. Hezel, B. Krevet, H. O. Moser, J. A. Rossmanith, R. Rossmanith, T. Schneider Subj-class: Accelerator Physics Report-no: ANKA Technical Note BES-07/97 \\ (Text of abstract) \\ (submission to math) \\ Title: Hamiltonian Dynamical Systems Without Periodic Orbits Authors: Viktor L. Ginzburg Comments: AMS-LaTeX, 16 pages Subj-class: Differential Geometry MSC-class: 58F05, 58F17, 58F22 \\ (Text of abstract) \\
Title:
Should be readable text - avoid illegible TeX sequences.
Author:
Use the form: first name(s) familyname
(first name(s) may be abbreviated by initial, followed by '.' and a blank)
seperate multiple authors by ', '
or ' and '.
Comments:
number of pages, number of figures,
(tex flavors, conference or journal,to which paper
has been submitted,...) For including an URL, see
help of E-prints archives.
Report-no:
Publication number(s) of your institution(s).
Subj-class:
for the
cond-mat ,
math
and
physics
archives.
For the cond-mat archive you may indicate
the Subj-class,
for the physics and math
archives it is obligatory .
Journal-Ref:
full bibliographic reference - only if paper has already
been published in a journal or conference proceedings,
must contain journal- or book-title, volume number,
year and page number.
MSC-class:
Mathematical
classification code for the math archive only
The abstract is used only for the listings and will not be TeXed, avoid illegible TeX sequences and unnecessary blank lines.
If a field does not apply to your paper, omit it. Do not include any extra fields. Submit
Find name and e-mail address of the
appropriate archive from
list .
The archive paper number
can be inserted directly into the TeX file
(typically on the title
page together with the local report numbers)
using the encoded form
arch-ive/yymmnnn (replace arch-ive by
the name of the selected archive).
The sequence 'yymmnnn' will be translated to the correct paper number
assigned after submission.
Example: hep-th/yymmnnn transforms to e.g. hep-th/9710323
For submission use any mail program.
The command 'put' must be placed in the ' Subject '
field of the mail program,
the header followed by the (packed) text (+figures) file in the
' Message ' area.
Example: To : hep-th@arXiv.org Cc : Attchmnt : Subject : put -----Message Text---- ( header ) ( paper )After submission, you will get an answer mail from the archive, which helps you to check the correctness of all important items. It includes the (preliminary till the next day) archive paper number, and a URL that will allow you to view the PostScript version generated, together with a username/password for viewing it. If you detect any errors, replace the paper!
Example: To : hep-th@arXiv.org Cc : Attchmnt : Subject : replace 9612121 -----Message Text---- ( new header ) ( new version of the paper)
Example: To : hep-lat@arXiv.org Cc : Attchmnt : Subject : cross hep-th/9701007 -----Message Text---- ( header )Before cross listing it is preferable to wait a day until the paper number is final.
Example: To : hep-th@arXiv.org Cc : Attchmnt : Subject : published 9701116 Phys. Rev. D56 (1997) 6684-6687 -----Message Text---- ( empty )
Be sure that all files you want to submit are in one directory.
Be careful with the choice of file names:
If you submit a file name.tex don't submit a file name.ps
too, because it will be automatically removed at the E-print archive
to allow dvips to create the Postscript file from your TeX file.
directory with files to be archived:Type [directory-name] (Enter)
files (e.g. *.ps, file1 file2 file3, or * for all):type [your file-names] (Enter) and you will be prompted for an output filename:
output file (will create name.tar.gz uuencoded as name.uu) name:Type [file-name] (Enter).
Physics astro-ph@arXiv.org (astrophysics) cond-mat@arXiv.org (condensed matter, see Subject-Classes) gr-qc@arXiv.org (general relativity / quantum cosmology) hep-lat@arXiv.org (computational and lattice physics) hep-ph@arXiv.org (high energy physics phenomenological) hep-th@arXiv.org (high energy physics formal) hep-ex@arXiv.org (high energy physics experimental) math-ph@arXiv.org (mathematical physics) nucl-ex@arXiv.org (nuclear experiment) nucl-th@arXiv.org (nuclear theory) physics@arXiv.org (partitioned, see Subject-Classes) quant-ph@arXiv.org (quantum physics) Mathematics math@arXiv.org (partitioned, see Subject-Classes) Nonlinear Sciences nlin@arXiv.org (partitioned, see Subject-Classes) Computer Science cs@arXiv.org (partitioned, see Subject-Classes)Have also a look at the complete list of available archives
Back to the DESY-Library Homepage.
Annemarie Blobel, Mar. 2004.