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Brevmall 2 Award decision regarding procurement of XXX AWARD DECISION Registration number Date General information Lund University, institution/department X, has executed a procurement of xxx. The procurement was executed as a simplified procedure with prior publication pursuant to the Swedish Public Procurement Act (2016:1145). The contract notice was published XX-XX-XX in (state database for pub
Brevmall 2 Award decision regarding procurement of XXX AWARD DECISION Registration number Date General information Lund University, institution/department X, has executed a procurement of xxx. The procurement was executed as a procurement below threshold with notice obligation pursuant to the Swedish Public Procurement Act (2016:1145). The contract notice was published XX-XX-XX in (state database
Exhange student - Bachelor level Where do you come from?I study Industrial and Organisational Psychology in Utrecht at Utrecht University in the Netherlands. Why did you choose to come to the Department of Service Management and Service Studies?I have chosen to enrol in the course Leadership in Service Organizations (15 credits) during my exchange at Lund University. When I read the summary of the
https://www.ses.lu.se/en/education/exchange-student/bachelor-level-courses/nathalie-stolwijk - 2026-05-25
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
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
Discover how the master’s programme in Pharmaceutical Technology combines industry-focused learning, hands-on projects and an international study environment, through the experience of student Sorosh.
Have you ever wondered what astronomers do?The Lund Culture Night is being celebrated during IAUs 100 Hours of Astronomy, and to celebrate this we release a new episode of our podcast; The Meridian. In this second episode of the podcast Nic and Rebecca - a couple of curious and energetic astronomy PhD students - invite Josefin Martell to the mic and chat to him about impact craters. Thereafter theIn this second episode of the podcast Nic and Rebecca invite Josefin Martell to the mic and chat to her about Impact Craters. Thereafter they take a closer look at one of their favourite astronomical objects: Dimidium.
We present the first spatially resolved (∼0.5 kpc) measurements of the molecular gas depletion time τ depl across the disk of the interacting spiral galaxy NGC 2276, a system with an asymmetric morphology in various star formation rate (SFR) tracers. To estimate τ depl, we use new NOEMA observations of the 12CO(1-0) emission tracing the bulk molecular gas reservoir in NGC 2276, and extinction-corr
Professor, Vice President Håkan Wiklund, Mid Sweden University Dr. Håkan Wiklund is currently professor in Quality Technology and Management at Mid Sweden University, Sweden. He received his PhD in Production Engineering at Linköping University and he became professor in Quality Technology and Management at Luleå University of Technology almost 20 years ago. Today he is deputy vice chancellor at M
https://www.ses.lu.se/en/sites/ses.lu.se.en/files/professor_hakan_wiklund_photo_short_bio_0.docx - 2026-05-27
This section contains examples of information that can be good to inform your students about before a digital exam. The information itself is a compilation of several faculties' and departments' information to students and we have divided it into different time periods. As soon as possible, you need to inform about the date and time, tools and software, if there is monitoring and how personal dat
https://www.education.lu.se/en/teaching-tips/digital-examination/build-and-conduct-assessment/inform-your-students - 2026-05-25
22 to 26 April 2026 Welcome to a new edition of INTONAL Festival at IAC!For the 2026 edition, we have shaped a curatorial framework that brings together our 15-years tradition of acousmonium practice and a focus on South and Central American sound scenes. This perspective unfolds through a dedicated talk and curated concerts, with music spatialized live on our 40+ speaker system.The talk will feat
https://www.iac.lu.se/intonal/intonal-2026-acousmatic-concerts-iac - 2026-05-25
The Cherenkov Telescope Array (CTA) observatory is the next generation of ground-based imaging atmospheric Cherenkov telescopes (IACTs). Building on the strengths of current IACTs, CTA is designed to achieve an order of magnitude improvement in sensitivity, with unprecedented angular and energy resolution. CTA will also increase the energy reach of IACTs, observing photons in the energy range from
Based on observational data from the fourth internal data release of the Gaia-ESO Survey we probe the abundance structure in the Milky Way stellar disk as a function of galactocentric radius and height above the plane. We find that the inner and outer Galactic disks have different chemical signatures. The stars in the inner Galactic disk show abundance signatures of both the thin and thick disks,
The lanthanide elements (Z=57?71) are characterized by the filling of the 4f electronic subshell, which lies close in energy to the 5d and 6s subshells. As a result, the lanthanide spectra can be quite complicated in terms of the number of optical spectral lines, and in some cases their hyperfine structure and isotopic shifts are extremely large. These characteristics have great implications for a
We consider the conditions necessary for the development of an inverted population among the energy levels of free atoms in a medium exposed to radiation in spectral non- equilibrium. In particular, we focus on monochromatic radiation occurring as a result of an accidental wavelength coincidence between a pumping emission line and a pumped absorption line in two different elements. We examine espe
We present a review of some of the current major challenges in stellar cluster research, including young clusters, globular clusters, and galactic nuclei. Topics considered include: primordial mass segregation and runaway mergers, expulsion of gas from clusters, the production of stellar exotica seen in some clusters (e.g., blue stragglers and extreme horizontal-branch stars), binary populations w
Under seeing limited conditions very high resolution spectroscopy becomes very difficult for extremely large telescopes (ELTs). Using adaptive optics (AO) the stellar image size decreases proportional with the telescope diameter. This makes the spectrograph optics and hence its resolution independent of the telescope diameter. However AO for use with ELTs at visible wavelengths require deformable
