The 35th annual conference on Astronomical Data Analysis Software & Systems 2025 in Görlitz, Germany

The Euclid satellite is an ESA mission that launched in July 2023. Euclid targets to observe an area of 14,000 deg^2 with two instruments, the Visible Imaging Channel (VIS) and the Near IR Spectrometer and imaging Photometer (NISP) down to VIS=24.5mag (10 sigma). Ground based imaging data in griz from surveys such as the Dark Energy Survey and Pan-STARRS complement the Euclid data to enable...

BlueMUSE is a new blue-optimized, medium spectral resolution, panoramic integral field spectrograph being developed for ESO's VLT. While building on the legacy of the much requested MUSE instrument, its blue wavelength coverage to the atmospheric cutoff (~350 nm) will make it unique. In Galactic, extragalactic, and high-redshift domains, BlueMUSE will enable new science not possible with...

Most traditional data reduction pipelines are on run an investigators local machine or remote machines requiring a manual touch to be executed. This approach leads to data discoverability and reproducibility issues. Additionally, observatory sites are also often remote and one of the major challenges is facilitating data transfer from site to site. Data Central's Apache NiFi system aims to...

Bayesian imaging of astrophysical measurement data shares universal properties across the electromagnetic spectrum: it requires probabilistic descriptions of possible images and spectra, and instrument responses. To unify Bayesian imaging, we present the the Universal Bayesian Imaging Kit (UBIK). Currently, UBIK allows X-ray satellite data imaging for Chandra and eROSITA and soon radio...