It is inherently challenging to characterize long-period transiting exoplanets because the transit events are rare and last long. These systems provide unique insights into planetary formation, migration, the detection of exomoons, and primordial atmospheres by occupying a sparsely populated region of the exoplanet parameter space, however. The

We present the New Online Database of Symbiotic Variables (NODSV), a comprehensive and publicly accessible catalog of known and candidate symbiotic stars in the Milky Way and nearby galaxies. The database provides an up-to-date census of confirmed symbiotic binaries and systematically compiles information previously scattered across the literature

We present new JWST/MIRI integral field spectroscopy (IFS) observations of the prototypical Seyfert 2 galaxy NGC 1068. These observations, combined with archival VLT/MUSE data, allow us to investigate the outflow from the active galactic nucleus (AGN) and radio jet and its interaction with the circumnuclear multiphase gas. MIRI data trace the

We investigate the height variation of the line-of-sight (LOS) magnetic field in solar active-region (AR) plage from the upper photosphere to the upper chromosphere using cospatial ultraviolet and infrared spectropolarimetric observations from the Sunrise III stratospheric balloon flight. The Ca II K and Ca II 8542 Å lines provide complementary

Understanding the magnetic field structure of spicules is essential for developing their formation models, which are important for understanding the mass transport to the corona and coronal heating. We report the spatial distribution of spicule magnetic fields from spectropolarimetric observations with SUNRISE III/SCIP, which provides high spatial

The Transiting Exoplanet Survey Satellite (TESS) is conducting a nearly full-sky survey, enabling the photometric characterisation of millions of stars. The forthcoming PLAnetary Transits and Oscillations of stars mission (PLATO) will provide long-duration, high-precision photometry of tens of thousands of bright stars to be characterised through