DOI,IST REx ID,Title of publication
10.1007/s10686-021-09712-0,17525,High angular resolution gravitational wave astronomy
10.1007/s10686-021-09709-9,17534,Unveiling the gravitational universe at μ-Hz frequencies
10.1093/mnras/stab1978,17574,The impact of baryons on cosmological inference from weak lensing statistics
10.1093/mnras/stab1856,17577,"Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries’"
10.1103/physrevd.104.103022,17578,Nucleosynthetic signatures of primordial origin around supermassive black holes
10.3847/2041-8213/abd4d3,17583,Eccentric black hole mergers in active galactic nuclei
10.1093/mnras/stab2315,17585,Signatures of hierarchical mergers in black hole spin and mass distribution
10.1093/mnras/stab2893,17586,Binary black hole signatures in polarized light curves
10.3847/2041-8213/ac2cc1,17589,"Black hole mergers of AGN origin in LIGO–Virgo’s O1–O3a observing periods"
10.3847/2041-8213/abdd1c,17592,Equilibrium eccentricity of accreting binaries
10.1007/s10714-021-02889-x,17593,The effect of mission duration on LISA science objectives
10.3847/1538-4357/ac106d,17598,Gravitational wave backgrounds from coalescing black hole binaries at cosmic dawn: An upper bound
10.1093/mnras/stab692,17610,Forming massive seed black holes in high-redshift quasar host progenitors
10.1142/S0129055X20600065,7685,The excitation spectrum of the Bose gas in the Gross-Pitaevskii regime
10.1142/s0129055x20600090,7900,Bosonic collective excitations in Fermi gases
10.1007/s00222-021-01041-5,7901,Correlation energy of a weakly interacting Fermi gas
10.1007/s00454-020-00206-y,7905,Sheaf-theoretic stratification learning from geometric and topological perspectives
10.1007/s11590-020-01603-1,7925,New inertial relaxed method for solving split feasibilities
10.1007/s00446-020-00380-5,7939,Fast approximate shortest paths in the congested clique
10.1007/s11081-020-09544-5,8196,New strong convergence method for the sum of two maximal monotone operators