Mohammadi F, Uhler C, Wang C, Yu J. Generalized permutohedra from probabilistic graphical models. SIAM Journal on Discrete Mathematics. 2018;32(1):64-93. doi:10.1137/16M107894X

Leopold NK, Pickl P. Mean-field limits of particles in interaction with quantised radiation fields. In: Vol 270. Springer; 2018:185-214. doi:10.1007/978-3-030-01602-9_9

McCloskey A, Ibarra A, Hetzer M. Tpr regulates the total number of nuclear pore complexes per cell nucleus. Genes &; Development. 2018;32(19-20):1321-1331. doi:10.1101/gad.315523.118

Fleischer JG, Schulte R, Tsai HH, et al. Predicting age from the transcriptome of human dermal fibroblasts. Genome Biology. 2018;19. doi:10.1186/s13059-018-1599-6

Matthee JJ, Sobral D, Gronke M, Paulino-Afonso A, Stefanon M, Röttgering H. Confirmation of double peaked Ly;1 emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe. Astronomy &; Astrophysics. 2018;619. doi:10.1051/0004-6361/201833528

Khostovan AA, Sobral D, Mobasher B, et al. The clustering of H ;2 + [OIII] and [OII] emitters since z c 5: Dependencies with line luminosity and stellar mass. Monthly Notices of the Royal Astronomical Society. 2018;478(3):2999-3015. doi:10.1093/mnras/sty925

Sobral D, Matthee JJ, Darvish B, et al. The nature of luminous Ly ;1 emitters at z c 2–3: Maximal dust-poor starbursts and highly ionizing AGN. Monthly Notices of the Royal Astronomical Society. 2018;477(2):2817-2840. doi:10.1093/mnras/sty782

Sobral D, Santos S, Matthee JJ, et al. Slicing COSMOS with SK: The evolution of typical Ly;1 emitters and the Ly;1 escape fraction from z c 2 to 6. Monthly Notices of the Royal Astronomical Society. 2018;476(4):4725-4752. doi:10.1093/mnras/sty378

Carniani S, Maiolino R, Amorin R, et al. Kiloparsec-scale gaseous clumps and star formation at z = 5–7. Monthly Notices of the Royal Astronomical Society. 2018;478(1):1170-1184. doi:10.1093/mnras/sty1088

Matthee JJ, Schaye J. Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and ;1-enhancement. Monthly Notices of the Royal Astronomical Society: Letters. 2018;479(1):L34-L39. doi:10.1093/mnrasl/sly093

Gandolfi D, Barragán O, Livingston JH, et al. TESS’s first planet: A super-Earth transiting the naked-eye star <0 Mensae. Astronomy &; Astrophysics. 2018;619. doi:10.1051/0004-6361/201834289

Bugnet LA, García RA, Davies GR, et al. FliPer: A global measure of power density to estimate surface gravities of main-sequence solar-like stars and red giants. Astronomy &; Astrophysics. 2018;620. doi:10.1051/0004-6361/201833106

Van Eylen V, Dai F, Mathur S, et al. HD 89345: A bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2. Monthly Notices of the Royal Astronomical Society. 2018;478(4):4866-4880. doi:10.1093/mnras/sty1390

Bugnet LA, García RA, Davies GR, Mathur S, Hall OJ, Rendle BM. FliPer: Classifying TESS pulsating stars. arXiv. doi:10.48550/arXiv.1811.12140

Henzinger MH, Noe A, Schulz C, Strash D. Practical minimum cut algorithms. ACM Journal of Experimental Algorithmics. 2018;23:1-22. doi:10.1145/3274662

Dütting P, Henzinger MH, Starnberger M. Valuation compressions in VCG-based combinatorial auctions. ACM Transactions on Economics and Computation. 2018;6(2). doi:10.1145/3232860

Goranci G, Henzinger MH, Thorup M. Incremental exact min-cut in polylogarithmic amortized update time. ACM Transactions on Algorithms. 2018;14(2). doi:10.1145/3174803

Bhattacharya S, Henzinger MH, Italiano G. Dynamic algorithms via the primal-dual method. Information and Computation. 2018;261(08):219-239. doi:10.1016/j.ic.2018.02.005

Goranci G, Henzinger MH, Peng P. Dynamic effective resistances and approximate schur complement on separable graphs. In: 26th Annual European Symposium on Algorithms. Vol 112. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2018. doi:10.4230/LIPICS.ESA.2018.40

Goranci G, Henzinger MH, Leniowski D. A tree structure for dynamic facility location. In: 26th Annual European Symposium on Algorithms. Vol 112. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2018. doi:10.4230/LIPICS.ESA.2018.39