DOI,IST REx ID,Research Group,Title of publication
10.1088/2515-7647/ae0fd1,21370,ScWa,Roadmap on deep learning for microscopy
10.1126/science.adz8603,21371,JoMa,Black holes disguised as little red dots
10.1103/16dk-5dgx,21373,MiLe,Phenomenological model of decaying Bose polarons
10.1007/978-3-032-17801-5_39,21374,HeEd,"Edge-constrained Hamiltonian paths on a point set"
10.1007/s00440-026-01468-y,21379,JuFi,On minimizing curves in a Brownian potential
10.1051/0004-6361/202557358,21380,JoMa,"J-PAS: First identification, physical properties, and ionization efficiency of extreme emission line galaxies"
10.1038/s41467-026-68660-5,21382,"ZhAl,LifeSc",Flexoelectric domain walls enable charge separation and transport in cubic perovskites
10.1126/sciadv.ady1461,21383,CaHe,Extracellular vesicles mediate stem cell signaling and systemic RNAi in planarians
10.1371/journal.pcbi.1013934,21384,MiSi,Modelling chemotaxis of branched cells in complex environments provides insights into immune cell navigation
10.48550/arXiv.2601.01255,21400,"GradSch,VlKo",A blueprint for the formalization of Seymour's matroid decomposition theorem
10.15479/AT-ISTA-21401,21401,"GradSch,ToHe",Privacy-preserving runtime verification
10.1007/s41468-026-00233-3,21407,HeEd,"Maximum persistent Betti numbers of Čech complexes"
10.1063/5.0304731,21408,"CaGo,GradSch",Simultaneous optimization of assembly time and yield in programmable self-assembly
10.1093/molbev/msag020,21409,BeVi,The evolutionary genomics of meiotic drive
10.1007/978-981-95-7127-7_26,21410,HeEd,"On the MST-ratio: Theoretical bounds and complexity of finding the maximum"
10.4230/LIPIcs.OPODIS.2025.31,21411,KrCh,Fast re-routing in networks: On the complexity of perfect resilience
10.48550/arXiv.2601.06646,21438,VeSu,Deterministic domain selection of antiferromagnets via magnetic fields
10.1103/h1m9-h3yw,21449,"JoFi,GradSch",Parametric amplification of spin-motion coupling in three-dimensional trapped-ion crystals
10.1051/0004-6361/202557675,21450,YlGo,A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
10.1051/0004-6361/202557537,21451,JoMa,The warm outer layer of a little red dot as the source of [Fe ii] and collisional Balmer lines with scattering wings