Twenty-five codes were added to the ASCL in June, 2025:
3ML: Framework for multi-wavelength/multi-messenger analysis
astromodels: Spatial and spectral models for astrophysics
Bjet_MCMC: Model multiwavelength spectral energy distributions of blazars
CAMEL: Cosmological parameters estimator
CLUES: Clustering tool for analyzing spectral data
CTD: Cumulative Time Dilation
DART-Vetter: Convolutional Neural Network to distinguish planetary transits from false positives
easyCHEM: Chemical abundances in exoplanet atmospheres calculator
excalibuhr: High-resolution spectral data reduction
Gen TSO: Graphical interface to simulate JWST exoplanet time-series observations
GRIP: Generic data Reduction for nulling Interferometry Package
hydromass: Hydrostatic mass profile reconstruction
M_-M_K-: Estimate masses and uncertainties from M_Ks (2MASS Ks + distance)
MAGIC: Automatic analysis of realistic microlensing light curves
OCSVM-Transit-Detection: One-Class SVM exoplanet transit detector
Octofitter: Bayesian inference against exoplanet and binary star data
pinc: Compute profile likelihoods in cosmology
Procoli: 1D profile likelihood extractor
pynchrotron: Synchrotron emission from cooling electrons
pyTPCI: Python version of The Pluto-Cloudy Interface
SBI++: Simulation-based (likelihood-free) inference for astronomical applications
SMART: Forward-modeling framework for spectroscopic data
TESS-cont: TESS contamination tool
TPCI: The PLUTO CLOUDY interface
VBMicrolensing: Microlensing computations for single, binary, and multiple lenses