_id,doi,title
13359,10.1016/j.chempr.2020.11.025,Dissipative self-assembly: Fueling with chemicals versus light
13360,10.1002/9783527821990.ch9,"Controlling Self‐Assembly of Nanoparticles Using Light"
13453,10.3847/1538-4357/ac29c5,Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi
13454,10.3847/1538-4357/ac27ae,Pre-explosion properties of Helium star donors to thermonuclear supernovae
13455,10.1051/0004-6361/202140506,Different to the core: The pre-supernova structures of massive single and binary-stripped stars
13456,10.3847/1538-4357/ac0af6,Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization
13457,10.1051/0004-6361/202140507,The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population
13458,10.3847/2041-8213/ac0b42,Binary-stripped stars as core-collapse supernovae progenitors
13459,10.3847/1538-3881/abf144,The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy
13995,10.1126/sciadv.abj8121,Attosecond interferometry of shape resonances in the recoil frame of CF4
13996,10.1021/acs.nanolett.1c02145,All-optical probe of three-dimensional topological insulators based on high-harmonic generation by circularly polarized laser fields
13997,10.1103/physreva.103.023101,Strong-field physics in three-dimensional topological insulators
14097,10.48550/arXiv.2111.15608,Science with the ultraviolet explorer (UVEX)
14117,10.1109/jproc.2021.3058954,Toward causal representation learning
14176,,Neighborhood contrastive learning applied to online patient monitoring
14177,,On disentangled representations learned from correlated data
14178,,On the transfer of disentangled representations in realistic settings
14179,,Self-supervised learning with data augmentations provably isolates content from style
14180,,Dynamic inference with neural interpreters
14181,10.24963/ijcai.2021/322,Boosting variational inference with locally adaptive step-sizes