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Max Planck Institute for Astronomy
- Heidelberg, Germany
- https://orcid.org/0000-0001-7923-2979
- Quximoz
- in/paul-boley-89250a34b
Stars
SED model grid and fitting tools for fitting SEDs of massive protostars
Command-line driven tool to create dust opacities
A pythonic interface for radio astronomy interferometry data (uvfits, measurement sets, uvh5, others)
Oimodeler is a modular modelling tool for optical interferometry
Reconstructing Hankel rAdial Profiles in centro-Symmetric Objects with Discrete rings for astrophYsics
X11/GUI utilities and applications for IRAF (xgterm, ximtool, xtapemon)
IRAF - Image Reduction and Analysis Facility
Absolute photometry and Sky Brightness with all-sky images.
Display and fit Optical (spectro-)Interferometric OIFITS data
Tutorials on the use of (Gaia) astrometry in astronomical data analysis or inference problems.
Estimate distances to stars as done for the Gaia-DR2 distance catalogue
Python version of the SED fitter from Robitaille et al., 2007, ApJS 169 328
Support for OI-FITS (optical interferometry data format) in Julia.
Contains core part of the RTS2 - RTS2 libraries, and drivers for basic devices.
A variety of python utilities focusing on numerical, scientific, and astrophysical computing