_id,doi,title
13451,10.3847/1538-4357/aca295,A panchromatic study of massive stars in the extremely metal-poor local group dwarf galaxy Leo A
13452,10.1093/mnras/stac2598,"The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities"
13994,10.1103/physrevx.12.011013,Ultrafast renormalization of the on-site Coulomb repulsion in a cuprate superconductor
11951,10.1038/s41467-022-32559-8,A direct excitatory projection from entorhinal layer 6b neurons to the hippocampus contributes to spatial coding and memory
12130,10.1038/s41467-022-34723-6,Specification of female germline by microRNA orchestrated auxin signaling in Arabidopsis
12154,10.3390/sym14102182,First and second sound in two-dimensional bosonic and fermionic superfluids
12208,10.1038/s41467-022-33931-4,On the nanoscale structural evolution of solid discharge products in lithium-sulfur batteries using operando scattering
12209,10.1038/s41567-022-01787-6,Morphogen gradient orchestrates pattern-preserving tissue morphogenesis via motility-driven unjamming
12217,10.1038/s41467-022-32806-y,Spatiotemporal dynamics of self-organized branching in pancreas-derived organoids
12249,10.1063/5.0107059,Computing chemical potentials of solutions from structure factors
12259,10.1063/5.0102904,Crises and chaotic scattering in hydrodynamic pilot-wave experiments
12277,10.1103/physrevx.12.031041,Geometry adaptation of protrusion and polarity dynamics in confined cell migration
12938,10.1039/d2cp03921d,"From vibrational spectroscopy and quantum tunnelling to periodic band structures – a self-supervised, all-purpose neural network approach to general quantum problems"
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"
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