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The four main findings about the age and abundance structure of the Milky Way bulge based on microlensed dwarf and subgiant stars are: (1) a wide metallicity distribution with distinct peaks at [Fe/H] = -1.09, -0.63, -0.20, +0.12, +0.41; (2) a high fraction of intermediate-age to young stars where at [Fe/H] > 0 more than 35 % are younger than 8 Gyr, (3) several episodes of significant star formati
A method of diagnosing, predicting, or prognosticating about a disease that includes obtaining experimental data, wherein the experimental data is high dimensional data, filtering the data, reducing the dimensionality of the data through use of one or more methods, training a supervised pattern recognition method, ranking individual data points from the data, wherein the ranking is dependent on th
A method of diagnosing, predicting, or prognosticating about a disease that includes obtaining experimental data, wherein the experimental data is high dimensional data, filtering the data, reducing the dimensionality of the data through use of one or more methods, training a supervised pattern recognition method, ranking individual data points from the data, wherein the ranking is dependent on th
A method of diagnosing, predicting, or prognosticating about a disease that includes obtaining experimental data, wherein the experimental data is high dimensional data, filtering the data, reducing the dimensionality of the data through use of one or more methods, training a supervised pattern recognition method, ranking individual data points from the data, wherein the ranking is dependent on th
A method of diagnosing, predicting, or prognosticating about a disease that includes obtaining experimental data, wherein the experimental data is high dimensional data, filtering the data, reducing the dimensionality of the data through use of one or more methods, training a supervised pattern recognition method, ranking individual data points from the data, wherein the ranking is dependent on th
The main purpose of this thesis is to present and analyse the Swedish sixteenth-century Catholic priest Andreas Servius’ prayer book Någre Christilige och Catholische böner printed in the Silesian city of Neisse year 1593. The general questions of the study are: which where the main sources of the prayers found in this prayer book? What characteristics typical for the period’s piety can be found i
Very-low-energy highly charged ions have been produced by use of white and monochromatic x rays from a wiggler line at the Stanford Synchrotron Radiation Laboratory to generate vacancy cascades following inner-shell photoionization. Recoil-ion energies have been determined and are shown to correspond essentially to room temperatures, even for high charge states. Promising applications to study of
The purpose with this paper is to put forward the complexity with employees’ identification with an organizations brand and the organization overall. We wish to examine the effects of internal employer branding, both through mainstream perspectives as well as through normative control. We hope to contribute with empirical support and deepen the knowledge for the impact that the brand has for the e
https://www.keg.lu.se/en/article/meet-glyn-williams - 2026-05-31
The LUSEM Mentorship Programme was concluded recently with mingling and valuable experience exchanges, between student mentees and alumni mentors. The programme offers LUSEM students and professionals the opportunity to exchange valuable experiences and ideas. Students thrive and get inspired by their mentors, through guidance and practical insight into the career world. Mentors get the opportunit
https://www.lusem.lu.se/article/career-and-leadership-inspiration-through-lusem-mentorship-programme - 2026-05-31
We present multiple-epoch radial-velocity observations for 104 stars in a field of the intermediate-age open cluster IC 4651 to . Only 13 stars (13%) of the full sample are field stars. From the 44 single member stars we find a mean radial velocity of , and the 12 single red-giant members yield a true radial-velocity dispersion of . Of the 19 giant members, 7 (37%) are spectroscopic binaries with
This article is over 5 years old, and the information may therefore be outdated. LUCSUS new postdoctoral researcher, Eric Hoddy, aims to develop a better understanding of the governance of climate change adaptation in informal urban settlements. In this short interview, he highlights what sustainability challenges he finds most interesting, what he likes about working at LUCSUS so far, and what he
Context. Gaia's Early Third Data Release (EDR3) does not contain new radial velocities because these will be published in Gaia's full third data release (DR3), expected in the first half of 2022. To maximise the usefulness of EDR3, Gaia's second data release (DR2) sources (with radial velocities) are matched to EDR3 sources to allow their DR2 radial velocities to also be included in EDR3. This pre
