_id,doi,title
10860,10.4153/s000843952000096x,Tight frames and related geometric problems
10912,10.48550/ARXIV.2108.06686,Quantifying the coexistence of neuronal oscillations and avalanches
11053,10.1007/s11357-021-00426-x,The San Diego Nathan Shock Center: Tackling the heterogeneity of aging
11436,,Asynchronous optimization methods for efficient training of deep neural networks with guarantees
11452,,Distributed principal component analysis with limited communication
11453,,Online learning of neural computations from sparse temporal feedback
11458,,AC/DC: Alternating Compressed/DeCompressed training of deep neural networks
11463,,M-FAC: Efficient matrix-free approximations of second-order information
11464,,Towards tight communication lower bounds for distributed optimisation
11498,10.1051/0004-6361/202140876,Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
11500,10.1051/0004-6361/202039887,The MUSE Extremely Deep Field: The cosmic web in emission at high redshift
11512,10.3847/1538-4357/ac01d7,"Measuring the average molecular gas content of star-forming galaxies at z = 3–4"
11522,10.1093/mnras/stab2762,Lyman-α transmission properties of the intergalactic medium in the CoDaII simulation
11523,10.1093/mnras/stab1304,The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: What makes a galaxy a Lyman α emitter?
11524,10.1093/mnras/stab1218,"The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ∼ 2 to z ∼ 6"
11525,10.1093/mnras/stab796,Constraining the cosmic UV background at z > 3 with MUSE Lyman-α emission observations
11526,10.1093/mnras/staa3277,Revealing the impact of quasar luminosity on giant Lyα nebulae
11585,10.1038/s41550-021-01415-y,Differences in galaxy colours are not just about the mass
11604,10.3847/1538-3881/ac166a,"TESS Data for Asteroseismology (T’DA) stellar variability classification pipeline: Setup and application to the Kepler Q9 data"
11605,10.1051/0004-6361/202039159,Magnetic signatures on mixed-mode frequencies: I. An axisymmetric fossil field inside the core of red giants