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The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co

Context. Elements heavier than Li are produced in the interiors of stars. However, for many elements the exact production sites and the timescales on which they are dispersed into the interstellar medium are unknown. Having a clear picture on the origins of the elements is important for our ability to trace and understand the formation and chemical evolution of the Milky Way and its stellar popula

Blocking technique for emulating very large polyelectrolytes

A new Monte Carlo method for computing thermodynamical properties of very large polyelectrolytes is presented. It is based on a renormalization group relating the original polymer to a smaller system, where, in addition to the naively rescaled forces, a corrective nearest-neighbor interaction originating from the short distance Coulomb cutoff is introduced. The method is derived for low T but is i

Guide-lupin-proceedo-confirm-delivery

Lupin Guide: Confirm delivery Support: https://www.staff.lu.se/ Lupin Proceedo Confirm delivery Tabel of Contents Confirm delivery .......................................................................................................... 1 Awaiting order response confirmation ........................................................................ 2 Waiting for order confirmation .................

https://www.ekonomiwebben.lu.se/sites/ekonomiwebben.lu.se/files/2025-03/guide-lupin-proceedo-confirm-delivery.pdf - 2026-05-24

Exoplanet atmospheres at high resolution through a modest-size telescope : FeII in MASCARA-2b and KELT-9b with FIES on the Nordic Optical Telescope

Ground-based, high-resolution spectrographs are providing us with an unprecedented view of the dynamics and chemistry of the atmospheres of planets outside the Solar System. While there are a large number of stable and precise high-resolution spectrographs on modest-size telescopes, it is the spectrographs at observatories with apertures larger than 3.5 m that dominate the atmospheric follow-up of

Prototype Open Event Reconstruction Pipeline for the Cherenkov Telescope Array

The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory currently under construction. It will improve over the current generation of imaging atmospheric Cherenkov telescopes (IACTs) by a factor of five to ten in sensitivity and it will be able to observe the whole sky from a combination of two sites: a northern site in La Palma, Spain, and a southern one in Paranal, Chile.

Properties of the -513 km/s Ejecta in the Spectrum of Eta Carinae

In the spectral region 2400-3160A of Eta Carinae, we have identifiedapproximately 500 absorption lines each with up to twenty velocitycomponents.The -512 km/s component is truely unique as 1) the typicalline width is <3 km/s, 2) the identified lines are in Fe I, Fe II, VII and Ti II, and 3) the lines originate from lower levels up to 2000cm-1 above the ground level. We have measured the velocity c

Theoretical oscillator strengths for Sr II and Y III, with application to abundances in the HgMn-type star chi Lupi

Oscillator strengths for selected transitions of Sr II and Y III have been determined using ab initio multiconfiguration Hartree-Fock techniques. The importance of including an accurate treatment of the core-valence correlation is emphasized. The results are used to determine the abundances of Sr and Y in the chemically peculiar star chi Lupi from HST/GHRS Echelle spectra. Overabundances of 2.09 d

W production in an improved parton-shower approach

In the description of the production properties of gauge bosons (W±, Z0, γ*) at colliders, the lowest-order graph normally is not sufficient. The contributions of higher orders can be introduced either by an explicit order-by-order matrix-element calculation, by a resummation procedure or by a parton-shower algorithm. Each approach has its advantages and disadvantages. We here introduce a method t

Gränslös nyfikenhet

Människans nyfikenhet när det gäller vårt Universum är närmast oändlig. I tusentals år har vi tittat uppåt och undrat om himlen helt enkelt är gudarnas domän eller om det kan finns varelser där ute i oändligheten som liknar oss.I denna visning reser vi från Jorden ut genom vårt Solsystem, besöker Solen och de åtta planeter som kretsar runt den, innan vi åker vidare mot stjärnor och galaxer. GalaxeIn this show we travel from the Earth to the edge of the Universe, discovering planets, stars and galaxies along the way.

Provocerade uppsägningar - om samspelet mellan materiella och processuella rättsregler

Sedan lagen om anställningsskydd trädde i kraft har kravet på saklig grund för uppsägning varit ett återkommande debatterat ämne inom arbetsrätten. Att arbetsgivaren behöver saklig grund när denne säger upp en arbetstagare är kanske inte så konstigt. Att en arbetsgivare kan behöva saklig grund när arbetstagaren säger upp sig själv är däremot ett mer svårgreppbart koncept. En uppsägning som formell

Att arkivera studentlivet - En studie om Lunds studentnationers bevarande av arkivmaterial

The purpose of this study is to give an insight into the archival management of six student nations at Lund University, as well as the general view of the archive amongst the members who are responsible for the student nation archives. The majority of the student nations are well over 300 years old, but there have been few or no studies about the student nations archives, a knowledge gap this stud

Variational auto-encoders with Student’s t-prior

We propose a new structure for the variational auto-encoders (VAEs) prior, with the weakly informative multivariate Student’s t-distribution. In the proposed model all distribution parameters are trained, thereby allowing for a more robust approximation of the underlying data distribution. We used Fashion-MNIST data in two experiments to compare the proposed VAEs with the standard Gaussian priors.

The Meridian S02E01 : The James Webb Space Telescope & an unexpected boat ride

In this first episode of the second season Nic and Rebecca invite Ori Fox to the podcast to discuss the newly launched JWST. Ori is an instrument scientist at the pace Telescope Science Institute (STSI) working on the Mid-Infrared Instrument (MIRI) which is one of four instruments on the James Webb Space Telescope. In this second season of the Meridian we are also bringing you some field reporting

A statistical model for quark fragmentation into mesons with emphasis on vector meson contributions

This paper is the first part of a program to deal with the relative importance of the different effects in a colour dipole field when the field energy is transformed into hadrons according to a statistical scheme with the sole constraints coming from energy and momentum conservation and the requirements of scaling. In this paper we treat the meson distributions from quark fragmentation with partic

The vector and scalar form factors of the pion to two loops

We calculate the vector and scalar form factors of the pion to two loops in Chiral Perturbation Theory. We estimate the unknown O(p6) constants using resonance exchange. We make a careful comparison to the available data and determine two O(p4) constants rather precisely, and two O(p6) constants less precisely. We also use Chiral Perturbation Theory to two loops to extract in a model-independent m