Institution
University of Ljubljana
Education•Ljubljana, Slovenia•
About: University of Ljubljana is a education organization based out in Ljubljana, Slovenia. It is known for research contribution in the topics: Population & Liquid crystal. The organization has 17210 authors who have published 47013 publications receiving 1082684 citations. The organization is also known as: Univerza v Ljubljani.
Papers published on a yearly basis
Papers
More filters
••
TL;DR: The results show that cell survival in experiments involving electropermeabilization can be improved by decreasing the medium conductivity, and both the induced and the resting transmembrane voltage must be considered, taking into account the conductivity and the ionic composition of the extracellular medium.
197 citations
••
University of New South Wales1, University of Sydney2, Max Planck Society3, Australian National University4, Australian Astronomical Observatory5, Uppsala University6, University of Cambridge7, Macquarie University8, University of Ljubljana9, University of Notre Dame10, University of Southern Queensland11, University of Western Australia12
TL;DR: The Galactic Archaeology with HERMES (GALAH) survey as discussed by the authors is a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration and minor mergers.
Abstract: The Galactic Archaeology with HERMES (GALAH) Survey is a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration and minor mergers. Using high-resolution (R$\simeq$28,000) spectra taken with the High Efficiency and Resolution Multi-Element Spectrograph (HERMES) instrument at the Anglo-Australian Telescope (AAT), GALAH will determine stellar parameters and abundances of up to 29 elements for up to one million stars. Selecting targets from a colour-unbiased catalogue built from 2MASS, APASS and UCAC4 data, we expect to observe dwarfs at 0.3 to 3 kpc and giants at 1 to 10 kpc. This enables a thorough local chemical inventory of the Galactic thin and thick disks, and also captures smaller samples of the bulge and halo. In this paper we present the plan, process and progress as of early 2016 for GALAH survey observations. In our first two years of survey observing we have accumulated the largest high-quality spectroscopic data set at this resolution, over 200,000 stars. We also present the first public GALAH data catalogue: stellar parameters (Teff, log(g), [Fe/H], [alpha/Fe]), radial velocity, distance modulus and reddening for 10680 observations of 9860 Tycho-2 stars that may be included in the first Gaia data release.
197 citations
••
University of Paris1, University College London2, Royal Observatory of Belgium3, University of Montpellier4, University of Liège5, University of Antwerp6, University of Geneva7, Leibniz Institute for Astrophysics Potsdam8, University of Bordeaux9, University of Nice Sophia Antipolis10, Spanish National Research Council11, University of La Laguna12, University of Grenoble13, Max Planck Society14, University of Antofagasta15, Atos16, University of Edinburgh17, University of Ljubljana18, INAF19, Australian National University20
TL;DR: In this paper, the authors describe the validation and properties of the median radial velocities published in Gaia DR2, which provide a full-sky coverage and are complete with respect to the astrometric data to within 77.2% (for G ≤ 12.5 mag).
Abstract: Context. For Gaia DR2, 280 million spectra collected by the Radial Velocity Spectrometer instrument on board Gaia were processed, and median radial velocities were derived for 9.8 million sources brighter than G RVS = 12 mag.Aims. This paper describes the validation and properties of the median radial velocities published in Gaia DR2.Methods. Quality tests and filters were applied to select those of the 9.8 million radial velocities that have the quality to be published in Gaia DR2. The accuracy of the selected sample was assessed with respect to ground-based catalogues. Its precision was estimated using both ground-based catalogues and the distribution of the Gaia radial velocity uncertainties. Results. Gaia DR2 contains median radial velocities for 7 224 631 stars, with T eff in the range [3550, 6900] K, which successfully passed the quality tests. The published median radial velocities provide a full-sky coverage and are complete with respect to the astrometric data to within 77.2% (for G ≤ 12.5 mag). The median radial velocity residuals with respect to the ground-based surveys vary from one catalogue to another, but do not exceed a few 100 m s−1 . In addition, the Gaia radial velocities show a positive trend as a function of magnitude, which starts around G RVS ~ 9 mag and reaches about + 500 m s−1 at G RVS = 11.75 mag. The origin of the trend is under investigation, with the aim to correct for it in Gaia DR3. The overall precision, estimated from the median of the Gaia radial velocity uncertainties, is 1.05 km s−1 . The radial velocity precision is a function of many parameters, in particular, the magnitude and effective temperature. For bright stars, G RVS ∈ [4, 8] mag, the precision, estimated using the full dataset, is in the range 220–350 m s−1 , which is about three to five times more precise than the pre-launch specification of 1 km s−1 . At the faint end, G RVS = 11.75 mag, the precisions for T eff = 5000 and 6500 K are 1.4 and 3.7 km s−1 , respectively.
196 citations
••
TL;DR: The 2019 special issue on understanding knowledge hiding in organizations as discussed by the authors provides some context to how and why this phenomenon should be studied and provides some suggestions for future research on knowledge hiding and its implications in organizations.
Abstract: J Organ Behav. 2019;40:779–782. Summary In our introduction to this special issue on understanding knowledge hiding in organizations, we provide some context to how andwhy this phenomenon should be studied. We then describe the five articles that comprise the special issue, and we note some common themes and divergences in this collection. Our introduction concludes with some suggestions for future research on knowledge hiding in organizations.
196 citations
••
TL;DR: Analysis of BA capabilities indicates that BA capabilities strongly impact a firm’s agility through an increase in information quality and innovative capability and that both market and technological turbulence moderate the influence of firms' agility on firms' performance.
196 citations
Authors
Showing all 17388 results
Name | H-index | Papers | Citations |
---|---|---|---|
David Miller | 203 | 2573 | 204840 |
Hyun-Chul Kim | 176 | 4076 | 183227 |
James M. Tour | 143 | 859 | 91364 |
Carmen García | 139 | 1503 | 96925 |
Bernt Schiele | 130 | 568 | 70032 |
Vladimir Cindro | 129 | 1157 | 82000 |
Teresa Barillari | 129 | 984 | 78782 |
Sven Menke | 129 | 1121 | 82034 |
Horst Oberlack | 129 | 985 | 80069 |
Hubert Kroha | 129 | 1126 | 80746 |
Peter Schacht | 129 | 1030 | 80092 |
Siegfried Bethke | 129 | 1266 | 103520 |
Igor Mandić | 128 | 1065 | 79498 |
Stefan Kluth | 128 | 1261 | 84534 |
Andrej Gorišek | 128 | 951 | 67830 |