High-resolution imaging is widely used to constrain false positive scenarios in exoplanet validation, but it is a finite follow-up resource that reaches only a subset of candidates, and its population-level impact on validation outcomes has not been quantified through controlled removal experiments. Using an automated pipeline built on TRICERATOPS

Context. Understanding the large-scale dynamics of molecular clouds (MCs) is crucial to constraining the processes that govern star formation and the structure and evolution of the Galaxy. While gas tracers have traditionally been used to map MC kinematics, stellar tracers such as young stellar objects (YSOs) and open clusters (OCs) provide a

We present the cross-match of galaxy clusters detected by redMaPPer using the first three years of Dark Energy Survey (DESY3RM) operations, and the first release of the eROSITA-All Sky Survey (eRASS1) taken by eROSITA onboard the Spectrum Roentgen Gamma telescope. We define a sky region ( $60^{\circ }\lt {\rm RA}\lt 90^{\circ }$ and $-58^{\circ }

Context. Several strong solar resonance lines show observable linear scattering polarization signals, holding a great potential for investigating the magnetism of the outer solar atmosphere. Accurately modeling these signals requires consideration of the detailed 3D structure of the solar atmosphere and accounting for partial frequency

We present JWST/MIRI mid-infrared integral field spectroscopy combined with ALMA CO(2--1) observations of the post-starburst galaxy ESO 420-G13, hosting a low-luminosity active galactic nucleus (AGN). The unprecedented spatial and spectral resolution of MIRI enables a detailed study of the molecular and ionised gas kinematics, excitation, and

The AM CVn class includes mass transferring, ultra-compact double white dwarf binaries with orbital periods on the timescale of minutes. A long-standing puzzle is that none of the roughly fifty ultra-compact, `verification binaries' that are easily detectable in the millihertz gravitational wave regime reside in a triple star configuration. Much