Open Data Standards for Open Source Software Risk Management Routines: An Examination of SPDX

As the organizational use of open source software (OSS) increases, it requires the adjustment of organizational routines to manage new OSS risk. These routines may be influenced by community-developed open data standards to explicate, analyze, and report OSS risks. Open data standards are co-created in open communities for unifying the exchange of information. The SPDX® specification is such an open data standard to explicate and share OSS risk information. The development and subsequent adoption of SPDX raises the questions of how organizations make sense of SPDX when improving their own risk management routines, and of how a community benefits from the experiential knowledge that is contributed back by organizational adopters. To explore these questions, we conducted a single case, multi-component field study, connecting with members of organizations that employed SPDX. The results of this study contribute to understanding the development and adoption of open data standards within open source environments

Oakscan: procédé de mesure rapide et non destructif des polyphénols du bois de chêne de tonnellerie

Les polyphénols extractibles contenus dans le bois de chêne des barriques de tonnellerie sont des composés très importants car ils ont une influence sur la couleur et sur les propriétés organoleptiques des vins qu'ils enrichissent. Les analyses chimiques de laboratoire qui permettent de les mesurer sont réalisées sur des extractions, nécessitent un délai de réalisation très long et ne permettent d'analyser que des lots de matière par échantillonnage. Le procédé de mesure rapide et non destructif Oakscan® a été développé par la tonnellerie Radoux. Il se fonde sur la spectrométrie proche infrarouge et permet de mesurer la teneur en polyphénols en quelques secondes, directement sur le bois massif. Le contenu polyphénolique de chaque douelle est alors mesuré, permettant une meilleure maitrise de la matière première entrant dans la composition des fûts

The Planetary Nebula Luminosity Function at the Dawn of Gaia

The [O III] 5007 Planetary Nebula Luminosity Function (PNLF) is an excellent extragalactic standard candle. In theory, the PNLF method should not work at all, since the luminosities of the brightest planetary nebulae (PNe) should be highly sensitive to the age of their host stellar population. Yet the method appears robust, as it consistently produces < 10% distances to galaxies of all Hubble types, from the earliest ellipticals to the latest-type spirals and irregulars. It is therefore uniquely suited for cross-checking the results of other techniques and finding small offsets between the Population I and Population II distance ladders. We review the calibration of the method and show that the zero points provided by Cepheids and the Tip of the Red Giant Branch are in excellent agreement. We then compare the results of the PNLF with those from Surface Brightness Fluctuation measurements, and show that, although both techniques agree in a relative sense, the latter method yields distances that are ~15% larger than those from the PNLF. We trace this discrepancy back to the calibration galaxies and argue that, due to a small systematic error associated with internal reddening, the true distance scale likely falls between the extremes of the two methods. We also demonstrate how PNLF measurements in the early-type galaxies that have hosted Type Ia supernovae can help calibrate the SN Ia maximum magnitude-rate of decline relation. Finally, we discuss how the results from space missions such as Kepler and Gaia can help our understanding of the PNLF phenomenon and improve our knowledge of the physics of local planetary nebulae.Comment: 12 pages, invited review at the conference "The Fundamental Cosmic Distance Scale: State of the Art and Gaia Perspective", to appear in Astrophysics and Space Scienc