A New Paradigm for Intellectual Property Rights in Software

A Winter 2004 article by Bradford L. Smith and Susan O. Mann of Microsoft published in The University of Chicago Law Review suggests that the development and growth of the software industry in the U.S. is a direct outgrowth of the implementation of intellectual property regimes, specifically copyright and patent, with respect to software in the late 1970s and early 1980s. This paper suggests that such patents were neither the sole nor the principal factor for the development of the software industry, that concerns about patents manifested prior to or soon after their application to software have proven true, and that patents are, in fact, not serving the interests of either the U.S. software industry or the consuming public. To that end, this paper advances recommendations for reforming the U.S. patent system as well as consideration of a new schema for protecting software

The peer-to-patent initiative : revitalizing patent examination with peer review

Every day we hear someone complain that this or that patent should not have been granted. People complain that the patent system is now a threat to existing business and innovation be- cause the patent office grants with alarming regularity patents for inventions that are neither novel nor non-obvious. People argue that the patent office cannot keep up with the job of examining the backlog of hundreds of thousands of patents and that, even if it could, the large volumes of prior art literature that need to be considered each time a patent application is received make the decision as to whether a patent should be granted or not a treacherous one

SEGUE : a spectroscopic survey of 240,000 stars with g=14-20

The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained approximate to 240,000 moderate-resolution (R similar to 1800) spectra from 3900 angstrom to 9000 angstrom of fainter Milky Way stars (14.0 10 per resolution element, stellar atmospheric parameters are estimated, including metallicity, surface gravity, and effective temperature. SEGUE obtained 3500 deg(2) of additional ugriz imaging (primarily at low Galactic latitudes) providing precise multicolor photometry (sigma(g, r, i) similar to 2%), (sigma(u, z) similar to 3%) and astrometry (approximate to 0 ''.1) for spectroscopic target selection. The stellar spectra, imaging data, and derived parameter catalogs for this survey are publicly available as part of Sloan Digital Sky Survey Data Release 7