Showing 1–20 of 79 results
/ Date/ Name
Feb 23, 2026Little Red Dots: One Photometric Tag Concealing Diverse Spectroscopic Flavors of Massive Star Formation and Black Hole ActivityFeb 5, 2026The JWST EXCELS survey: The ages and abundances of $3<z<5$ massive quiescent galaxies show that downsizing was already in place by $z\simeq4$Jan 15, 2026Topological textures and emergent altermagnetic signatures in ultrathin BiFeO3Sep 16, 2025SuNeRF-CME: Physics-Informed Neural Radiance Fields for Tomographic Reconstruction of Coronal Mass EjectionsSep 8, 2025PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5Sep 4, 2025GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave PropagationJul 16, 2025Low-energy domain wall racetracks with multiferroic topologiesMar 10, 2025JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7Oct 29, 2024Morphogenesis of Spin Cycloids in a Non-collinear AntiferromagnetSep 4, 2024Superfluid-tight cryogenic receiver with continuous sub-Kelvin cooling for EXCLAIMJul 19, 2024ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developmentsJul 10, 2024Sulphur dioxide in the mid-infrared transmission spectrum of WASP-39bJun 7, 2024The $β$ Pictoris b Hill sphere transit campaign. Paper II: Searching for the signatures of the $β$ Pictoris exoplanets through time delay analysis of the $δ$ Scuti pulsationsApr 16, 2024A 25-micron single photon sensitive kinetic inductance detectorNov 13, 2023On the hypothesis of an inverted Z-gradient inside JupiterMay 10, 2023A reflective, metal-rich atmosphere for GJ 1214b from its JWST phase curveApr 18, 2023Saturn's Interior After the Cassini Grand FinaleMar 27, 2023Science opportunities with solar sailing smallsatsFeb 28, 2023JWST-TST Proper Motions: I. High-Precision NIRISS Calibration and Large Magellanic Cloud KinematicsFeb 17, 2023Jupiter's interior from Juno: Equation-of-state uncertainties and dilute core extent