Aims. We derive the stellar mass function (SMF) of quiescent and star-forming galaxies at z ≤ 0.2 using 12-band (five broad plus seven narrow) photometry from the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3) over 3284 deg 2, where the narrow bands improve photometric-redshift and stellar property precision relative

Progress in understanding accreting black holes remains hampered by a lack of sensitive coordinated multiwavelength observations. In particular, the mid-infrared (MIR) regime remains ill-explored except for jet-dominant states. Here, we present comprehensive follow-up of the black hole X-ray binary GX 339─4 during a bright disc-dominated state in

Context. Following its nominal mission, the Hayabusa2 spacecraft is cruising toward two new targets as part of its extended mission, Hayabusa2# (SHARP: Small Hazardous Asteroid Reconnaissance Probe). The spacecraft will fly by the near-Earth asteroid (98943) Torifune in 2026 and rendezvous with another near-Earth asteroid, 1998 KY 26, in 2031. 1998

Modifications to Newtonian dynamics at low accelerations have long been proposed as an alternative to dark matter to explain galaxy rotation curves. More recently, similar corrections have been invoked to interpret anomalies in Cavendish-type laboratory experiments and in the dynamics of wide binary stars, although the latter remain affected by

Context. Superluminous supernovae (SLSNe) are a rare class of transients with peak luminosities 10─100 times greater than those of standard core-collapse supernovae (SNe). The mechanisms powering their extreme brightness remain debated, with circumstellar medium (CSM) interaction, or energy injection from a central engine like a magnetar wind