The atomic data for absorption lines compiled by Verner et al. (1994) include data for 2249 lines having wavelengths greater than 228 Å. Shirai et al. (1996b) have completed a large single-volume tabulation of spectral-line data for highly-ionized atoms of Ti through Cu, and Kr and Mo. The energy levels of the Zn spectra (Zn I-XXX) have been compiled (Sugar and Musgrove, 1995), and a new compilation of data for the Ga spectra (Ga I-XXXI) includes classified lines and separate tables of energy levels (Shirai et al. 1996a).
The data in most of the newly published major compilations of these types are now also available via the Internet; for example, all of the above compilations except the absorption-line data are accessible at the NIST Physics Laboratory Web site, and the absorption data are included in the holdings of the ``Atomic Data for Astrophysics'' site (see below for the addresses of Web sites mentioned in this paragraph). It is also worth noting that some of the newly compiled or updated data being loaded into Internet databases may not be published in printed form. The energy-level data for the C, N, and O spectra in the NIST database for example, include some updating of the older compilations. Quite large datasets previously available only on magnetic tape or CD-ROM's have also been made available via the Internet, examples being the Kurucz CD-ROM 23 (CfA site, see Smith et al. 1996) and the ``Atomic Spectral Line List'' of R. Hirata and T. Horaguchi (CDS site, Catalogue VI/69). The ``Vienna Atomic Line Data Base'' is accessible only via e-mail (Piskunov et al. 1995).
A number of papers on atomic spectroscopic data are included in the proceedings of a workshop on Laboratory and Astronomical High Resolution Spectra (Sauval et al. 1995), and a few such papers were given at an IAU Joint Discussion on Astrophysical Applications of Powerful New Databases (Adelman and Wiese 1995). The invited papers given at the Fifth International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas, held in Meudon, France, August 1995, are scheduled for publication (Tchang-Brillet et al. 1996a). Many of the contributed papers for this colloquium were on particular spectra of astrophysical interest; these appear in a publication of the Paris Observatory (Tchang-Brillet et al. 1996b).