DOI,IST REx ID,Title of publication
10.3847/2041-8213/aadf3a,17627,Identifying direct collapse black hole seeds through their small host galaxies
10.3847/2041-8213/aad8ad,17640,Gravitational waves from supermassive black hole binaries in ultraluminous infrared galaxies
10.1093/mnras/sty142,17655,Self-consistent semi-analytic models of the first stars
10.1103/physrevd.97.103515,17662,Non-Gaussian information from weak lensing data via deep learning
10.1093/mnras/sty276,17679,"Low-density, radiatively inefficient rotating-accretion flow on to a black hole"
10.3847/1538-4357/aaad0f,17680,Testing the binary hypothesis: Pulsar timing constraints on supermassive black hole binary candidates
10.1093/mnras/sty1720,17687,Massive black hole and Population III galaxy formation in overmassive dark-matter haloes with violent merger histories
10.1093/mnras/sty516,17691,Testing the relativistic Doppler boost hypothesis for supermassive black hole binary candidates
10.1088/1475-7516/2018/03/049,17713,MassiveNuS: Cosmological massive neutrino simulations
10.19086/da.4375,178,Counting rational points on quadric surfaces
10.1021/jacs.8b10296,17927,Large variations in the single-molecule conductance of cyclic and bicyclic silanes
10.1021/jacs.8b06964,17928,Resonant transport in single diketopyrrolopyrrole junctions
10.1021/acs.nanolett.8b02743,17929,Near length-independent conductance in polymethine molecular wires
10.1021/jacs.8b05184,17930,In situ formation of N-heterocyclic carbene-bound single-molecule junctions
10.1038/s41586-018-0197-9,17931,"Comprehensive suppression of single-molecule conductance using destructive σ-interference"
10.1039/c7nr08737c,17932,Tuning ultrafast electron injection dynamics at organic-graphene/metal interfaces
10.1039/c7nr08354h,17933,Electronic and mechanical characteristics of stacked dimer molecular junctions
10.1021/acs.jpclett.8b00176,17934,Probing charge transport through peptide bonds
null,18,Superconcentrators of density 25.3
10.5802/jep.64,180,Statistical mechanics of the uniform electron gas
