DOI,IST REx ID,Research Group,Title of publication
10.48550/ARXIV.2108.06686,10912,GaTk,Quantifying the coexistence of neuronal oscillations and avalanches
10.1016/j.devcel.2021.10.008,11052,MaHe,Identification of long-lived proteins in the mitochondria reveals increased stability of the electron transport chain
10.1007/s11357-021-00426-x,11053,,The San Diego Nathan Shock Center: Tackling the heterogeneity of aging
null,11436,DaAl,Asynchronous optimization methods for efficient training of deep neural networks with guarantees
10.1007/s00454-021-00299-z,11446,,Vanishing of all equivariant obstructions and the mapping degree
null,11452,DaAl,Distributed principal component analysis with limited communication
null,11453,TiVo,Online learning of neural computations from sparse temporal feedback
null,11458,"GradSch,DaAl",AC/DC: Alternating Compressed/DeCompressed training of deep neural networks
null,11463,DaAl,M-FAC: Efficient matrix-free approximations of second-order information
null,11464,DaAl,Towards tight communication lower bounds for distributed optimisation
10.1051/0004-6361/202140876,11498,,Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
10.1051/0004-6361/202039887,11500,,The MUSE Extremely Deep Field: The cosmic web in emission at high redshift
10.3847/1538-4357/ac01d7,11512,,"Measuring the average molecular gas content of star-forming galaxies at z = 3–4"
10.1093/mnras/stab2762,11522,,Lyman-α transmission properties of the intergalactic medium in the CoDaII simulation
10.1093/mnras/stab1304,11523,,The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: What makes a galaxy a Lyman α emitter?
10.1093/mnras/stab1218,11524,,"The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ∼ 2 to z ∼ 6"
10.1093/mnras/stab796,11525,,Constraining the cosmic UV background at z > 3 with MUSE Lyman-α emission observations
10.1093/mnras/staa3277,11526,,Revealing the impact of quasar luminosity on giant Lyα nebulae
10.1038/s41550-021-01415-y,11585,,Differences in galaxy colours are not just about the mass
10.3847/1538-3881/ac166a,11604,,"TESS Data for Asteroseismology (T’DA) stellar variability classification pipeline: Setup and application to the Kepler Q9 data"