DOI,IST REx ID,Title of publication
10.1007/s00454-021-00299-z,11446,Vanishing of all equivariant obstructions and the mapping degree
null,11452,Distributed principal component analysis with limited communication
null,11453,Online learning of neural computations from sparse temporal feedback
null,11463,M-FAC: Efficient matrix-free approximations of second-order information
null,11464,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"
10.1051/0004-6361/202039159,11605,Magnetic signatures on mixed-mode frequencies: I. An axisymmetric fossil field inside the core of red giants
10.1051/0004-6361/202039180,11606,Probing the internal magnetism of stars using asymptotic magneto-asteroseismology
10.1051/0004-6361/202039947,11608,ROOSTER: A machine-learning analysis tool for Kepler stellar rotation periods
10.1051/0004-6361/202038654,11609,Horizontal shear instabilities in rotating stellar radiation zones: II. Effects of the full Coriolis acceleration
10.23919/ifipnetworking52078.2021.9472803,11649,On the complexity of weight-dynamic network algorithms