DOI,IST REx ID,Research Group,Title of publication
10.1093/mnras/stad3853,14852,"GradSch,JoMa","Linking UV spectral properties of MUSE Ly α emitters at <i>z</i> ≳ 3 to Lyman continuum escape"
10.3847/1538-4357/acd118,13443,LiBu,"Magnetic activity evolution of solar-like stars. I. Sph–age relation derived from Kepler observations"
10.1088/1538-3873/acb6b5,13449,,Bringing stellar evolution and feedback together: Summary of proposals from the Lorentz Center workshop
10.3847/1538-4357/aca655,13450,,"Cool, luminous, and highly variable stars in the Magellanic Clouds. II. Spectroscopic and environmental analysis of Thorne–Żytkow object and super-AGB star candidates"
10.1051/0004-6361/202245650,14103,,X-shooting ULLYSES: Massive stars at low metallicity. I. Project description
10.1093/mnras/stad1977,14104,,"Observational predictions for Thorne–Żytkow objects"
10.3847/1538-4357/ac97e7,13445,,Mode mixing and rotational splittings. I. Near-degeneracy effects revisited
10.3847/1538-4357/aca295,13451,,A panchromatic study of massive stars in the extremely metal-poor local group dwarf galaxy Leo A
10.1093/mnras/stac2598,13452,,"The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities"
10.1051/0004-6361/202142302,11488,,"The MUSE eXtremely Deep Field: Individual detections of Ly<i>α</i> haloes around rest-frame UV-selected galaxies at <i>z</i> ≃ 2.9–4.4"
10.1051/0004-6361/202142187,11490,,Deciphering stellar metallicities in the early universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
10.1051/0004-6361/202141900,11497,,Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
10.3847/1538-4357/ac3509,11509,,"EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 10⁴-10⁵⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae"
10.3847/1538-4357/ac4419,11510,,"The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments"
10.3847/1538-4357/ac350b,11511,,On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation
10.3847/1538-4357/ac2c83,11601,,"The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in C1–C8 and C10–C18"
10.1051/0004-6361/202141168,11602,,Detections of solar-like oscillations in dwarfs and subgiants with Kepler DR25 short-cadence data
10.1051/0004-6361/202142956,11621,,Detecting deep axisymmetric toroidal magnetic fields in stars: The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field
10.1029/2021jd034911,12583,,The energy and mass balance of Peruvian Glaciers
10.3847/1538-4357/ac29c5,13453,,Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi