DOI,IST REx ID,Research Group,Title of publication
10.1016/j.ress.2019.106665,6918,KrCh,An efficient algorithm for computing network reliability in small treewidth
10.1126/sciadv.abc8895,8986,JiFr,Functional innovations of PIN auxin transporters mark crucial evolutionary transitions during rise of flowering plants
10.3390/ijms21165727,8283,JiFr,"AcoMYB4, an Ananas comosus L. MYB transcription factor, functions in osmotic stress through negative regulation of ABA signaling"
10.1038/s41467-020-18269-z,8529,JoFi,Converting microwave and telecom photons with a silicon photonic nanomechanical interface
10.1103/prxquantum.1.020315,9114,JoFi,Bidirectional electro-optic wavelength conversion in the quantum ground state
10.1364/optica.386613,21640,,Accelerating recurrent Ising machines in photonic integrated circuits
10.1364/oe.403192,21637,,"Fullwave Maxwell inverse design of axisymmetric, tunable, and multi-scale multi-wavelength metalenses"
10.1515/nanoph-2020-0579,21642,,"End‐to‐end nanophotonic inverse design for imaging and polarimetry"
10.1051/0004-6361/201834565,11499,,"Exploring He II λ1640 emission line properties at z ∼2−4"
10.1051/0004-6361/201834471,11505,,"Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE"
10.1051/0004-6361/201833075,11507,,Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator
10.3847/1538-4357/ab3102,11514,,The ALMA spectroscopic survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
10.3847/1538-4357/ab2f81,11515,,Resolved UV and [C ii] structures of luminous galaxies within the epoch of reionization
10.3847/1538-4357/ab2881,11516,,A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE
10.3847/1538-4357/ab1c5b,11517,,On the elevation and suppression of star formation within galaxies
10.1093/mnras/stz2149,11535,,"The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities"
10.1093/mnras/stz030,11540,,"The origin of scatter in the star formation rate–stellar mass relation"
10.1093/mnras/sty2779,11541,,"On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components"
10.3389/fspas.2019.00046,11613,,Revisiting the impact of stellar magnetic activity on the detectability of solar-like oscillations by Kepler
10.1051/0004-6361/201834780,11614,,FliPerClass: In search of solar-like pulsators among TESS targets