DOI,IST REx ID,Title of publication
10.1080/15257770.2017.1287378,21157,"Comparison of X-ray crystal structures of a tetradecamer sequence d(CCCGGGTACCCGGG)2 at 1.7 Å resolution"
10.1515/crelle-2014-0122,256,Improvements in Birch's theorem on forms in many variables
10.1093/imrn/rnx116,169,Twisted Linnik implies optimal covering exponent for S3
10.1093/imrn/rnx252,172,Strong approximation and a conjecture of Harpaz and Wittenberg
10.1093/mnras/stx1269,17616,"Lighthouse in the dust: infrared echoes of periodic emission from massive black hole binaries★"
10.1017/s1743921317000734,17629,A statistical method for detecting gravitational recoils of supermassive black holes in active galactic nuclei
10.1093/mnras/stx2469,17630,A drop in the pond: The effect of rapid mass-loss on the dynamics and interaction rate of collisionless particles
10.1093/mnras/stx3134,17632,On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening
10.1093/mnras/stx2524,17633,Interactions between multiple supermassive black holes in galactic nuclei: A solution to the final parsec problem
10.1038/s41550-017-0075,17667,Rapid formation of massive black holes in close proximity to embryonic protogalaxies
10.1093/mnras/stx167,17668,Beyond Jcrit: A critical curve for suppression of H2-cooling in protogalaxies
10.1103/physrevd.95.123503,17673,Validity of the Born approximation for beyond Gaussian weak lensing observables
10.1093/mnras/stx909,17696,What is the maximum mass of a Population III galaxy?
10.1093/mnras/stx1130,17698,On the orbital evolution of supermassive black hole binaries with circumbinary accretion discs
10.3847/1538-4357/835/2/165,17706,Rapid and bright stellar-mass binary black hole mergers in active galactic nuclei
10.1103/physrevd.96.023004,17707,Electromagnetic chirp of a compact binary black hole: A phase template for the gravitational wave inspiral
10.1103/physrevd.96.023513,17708,Geometry and growth contributions to cosmic shear observables
10.1038/s41467-017-00851-7,17711,Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers
10.1103/physrevd.96.063014,17712,Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal
10.1038/s41559-017-0373-6,7725,Predation drives local adaptation of phenotypic plasticity