DOI,IST REx ID,Research Group,Title of publication
10.1109/BLOC.2019.8751326,6056,KrCh,Probabilistic smart contracts: Secure randomness on the blockchain
10.7554/elife.41801,6187,DaSi,A conserved major facilitator superfamily member orchestrates a subset of O-glycosylation to aid macrophage tissue invasion
10.15479/AT:ISTA:6546,6546,"DaSi,GradSch",The role of a highly conserved major facilitator superfamily member in Drosophila embryonic macrophage migration
10.15479/AT:ISTA:6849,6849,"JoCs,GradSch",The role of CCK-interneurons in regulating hippocampal network dynamics
10.15479/at:ista:7132,7132,HaJa,Design and characterization of methods and biological components to realize synthetic neurotransmission
10.1007/978-3-319-74772-9_7,10864,VlKo,Absorption and directed Jónsson terms
10.1093/bfgp/ely007,10880,CaHe,Significance of whole-genome duplications on the emergence of evolutionary novelties
10.1093/jxb/ery097,10881,JiFr,Molecular evolution and diversification of the SMXL gene family
10.1109/cvpr.2018.00956,10882,ChLa,Learning intelligent dialogs for bounding box annotation
10.29007/5z5k,10883,KrCh,Quasipolynomial set-based symbolic algorithms for parity games
10.1137/16M107894X,1092,,Generalized permutohedra from probabilistic graphical models
10.1007/978-3-030-01602-9_9,11,RoSe,Mean-field limits of particles in interaction with quantised radiation fields
10.1101/gad.315523.118,11063,,Tpr regulates the total number of nuclear pore complexes per cell nucleus
10.1186/s13059-018-1599-6,11064,,Predicting age from the transcriptome of human dermal fibroblasts
10.1051/0004-6361/201833528,11508,,Confirmation of double peaked Lyα emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe
10.1093/mnras/sty925,11549,,"The clustering of H β + [O III] and [O II] emitters since z ∼ 5: Dependencies with line luminosity and stellar mass"
10.1093/mnras/sty1088,11555,,"Kiloparsec-scale gaseous clumps and star formation at z = 5–7"
10.1093/mnras/sty782,11557,,"The nature of luminous Ly α emitters at z ∼ 2–3: Maximal dust-poor starbursts and highly ionizing AGN"
10.1093/mnras/sty378,11558,,"Slicing COSMOS with SC4K: The evolution of typical Ly α emitters and the Ly α escape fraction from z ∼ 2 to 6"
10.1093/mnrasl/sly093,11584,,"Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and α-enhancement"