Nuclear Properties for Astrophysical and RIB Applications: Compressed Files

Each of these files for the preprint ``Nuclear Properties for Astrophysical and Radioactive-Ion-Beam Applications,'' by P. Möller, J. R. Nix, and K.-L. Kratz, has been compressed by use of the command gzip name to produce the compressed version name.gz. If these files are not decompressed automatically by your system, then use the command gunzip name.gz to transform the compressed file name.gz into the normal file name. The description for each file below refers to the normal version after decompression.

astro.tar.gz (3.73 MB). Tar file of the complete preprint, including device-independent (dvi), PostScript, and LaTeX versions of the text and table, plus PostScript files of the figures and graphs. Use the command tar xvf astro.tar to create the directory astro containing the files text.dvi, text.ps, text.tex, table.dvi, table.ps, and table.tex plus the three sub-directories figs1-16, figs17-37, and graphs with the indicated figures and graphs. The six text and table files contained in astro.tar are identical to those that can be obtained individually below, but the formats used for the figures and graphs are different. The figures and graphs are included in astro.tar as 93 separate files in three sub-directories, whereas in the format used below they are merged into three files containing multiple figures or graphs.
text.dvi.gz (80 KB). Device-independent (dvi) file produced by LaTeX of the text section of the preprint, which occupies pages 1-40; the explanation of the graphs, which occupies page 78; the explanation of the table, which occupies pages 135 and 136; and pages 137 and 138 that should be discarded. This file can be conveniently viewed on-screen by use of xpreview, xdvi, or similar dvi previewer. It can also be used on many systems to generate a PostScript file of arbitrary printer resolution.
text.ps.gz (156 KB). PostScript file in 600-dpi resolution produced by LaTeX and dvips of the text section of the preprint, which occupies pages 1-40; the explanation of the graphs, which occupies page 78; and the explanation of the table, which occupies pages 135 and 136. Print this file on a 600-dpi PostScript printer to produce the entire text section and explanations of the graphs and table.
text.tex.gz (54 KB). LaTeX file of the text section of the preprint, which occupies pages 1-40; the explanation of the graphs, which occupies page 78; the explanation of the table, which occupies pages 135 and 136; and pages 137 and 138 that should be discarded. Please note that if you process this file with your LaTeX system, you may obtain line and page breaks at different locations than occurred where the preprint was prepared. To guarantee the original appearance of the preprint, you should instead utilize either the above file text.dvi or the above file text.ps.
figs1-16.ps.gz (290 KB). Figures 1-16 of the preprint, which are in color. This file should ideally be printed on a color PostScript printer. On some color printers that are not able to print close to the edge of the paper, the page number, figure number, and running head may not be printed properly. If this occurs, the figure can be rescaled and translated by use of appropriate PostScript commands. Alternatively, this file can be conveniently viewed on-screen by use of ghostview or similar PostScript previewer. In the absence of a color printer or monitor, you can print or view this file on a black-and-white device, although the resulting grayscale is nonoptimal.
figs17-37.ps.gz (193 KB). Figures 17-37 of the preprint. Print on any black-and-white PostScript printer. Alternatively, this file can be conveniently viewed on-screen by use of ghostview or similar PostScript previewer.
graphs.ps.gz (1.37 MB). Graphs 1-56 of the preprint, containing level diagrams for representative spherical and deformed nuclei throughout the periodic system. Print on any black-and-white PostScript printer. In the event that your printer memory is not large enough to print this long file in its entirety, it can be split into separate files corresponding to smaller numbers of figures. The splits should occur between %%trailer and %!PS-Adobe-1.0. Alternatively, this file can be conveniently viewed on-screen by use of ghostview or similar PostScript previewer.
table.dvi.gz (478 KB). Device-independent (dvi) file produced by LaTeX of the table of nuclear properties, which occupies pages 135 and 136 (blank to facilitate running head and double-sided printing) and pages 137-296. This file can be conveniently viewed on-screen by use of xpreview, xdvi, or similar dvi previewer. It can also be used on many systems to generate a PostScript file of arbitrary printer resolution.
table.ps.gz (696 KB). PostScript file in 600-dpi resolution produced by LaTeX and dvips of the table of nuclear properties, which occupies pages 137-296. Print this file on a 600-dpi PostScript printer to produce the entire table.
table.tex.gz (402 KB). LaTeX file of the table of nuclear properties, which occupies pages 135 and 136 (blank to facilitate running head and double-sided printing) and pages 137-296. Please note that if you process this file with your LaTeX system, you may obtain line and page breaks at different locations than occurred where the table was prepared. To guarantee the original appearance of the preprint, you should instead utilize either the above file table.dvi or the above file table.ps.