Integrated flux for ALMA’s CO(3-2) line measurement. Superposed as black circles on Neptune’s map are the beam positions observed onto the planet and used for the spatially resolved retrievals. The

AbGradEPEC’26 Early Career Event: AbGradEPEC’26 – 6th September 2026 The Europlanet Early-Career (EPEC) Network and Astrobiology Graduates in Europe (AbGradE) are thrilled to announce the latest event in our long-standing

SFR as a function of stellar mass for equilibrium (left) and non-equilibrium (right) galaxies. The solid red line indicates the SFMS from Renzini & Peng (2015), with dashed lines showing

Pole-on views of the orbital positions of Proxima d (small black dot) and b (large black dot) during each enhanced-emission event. The telescope symbol and vertical dotted line indicate the

ShaneAO/ShARCS high-resolution imaging of HIP 18512 (left), ShaneAO/ShARCS imaging of HIP 45839 (center), and Keck/NIRC2 high-contrast imaging of HIP 45839 (right). Each image is oriented such that north is up

Spectral characterization of Chiron’s surface composition. a Comparison of the bestfit spectral model of the surface composition (red) with the measured spectrum (black). The surface is best described by an

Top and middle panels: Colour–colour diagrams (J−K vs. J−H) as a function of spectral type. The spectral types highlighted in each panel are as follows: M0-M4 (a), M5-M9 (b), L0-L4