Python modules for simulating and manipulating VLBI data and producing images with regularized maximum likelihood methods. This version is an early release so please submit a pull request or email [email protected] if you have trouble or need help for your application.
The package contains several primary classes for loading, simulating, and manipulating VLBI data. The main classes are the Image, Array, Obsdata, Imager, and Caltable classes, which provide tools for loading images and data, producing simulated data from realistic u-v tracks, calibrating, inspecting, and plotting data, and producing images from data sets in various polarizations using various data terms and regularizers.
Download the latest version from the GitHub repository, change to the main directory and run:
pip install .It should install most of the required libraries automatically (astropy, ephem, future, h5py , html , networkx, numpy, pandas , matplotlib, requests, scipy, skimage).
If you want to use fast fourier transforms, you will also need to separately install NFFT and its pynfft wrapper. The simplest way is to use conda to install both:
conda install -c conda-forge pynfftAlternatively, first install NFFT manually following the instructions on the readme, making sure to use the --enable-openmp flag in compilation. Then install pynfft, with pip, following the readme instructions to link the installation to where you installed NFFT. Finally, reinstall ehtim.
Documentation is here .
Here are some ways to learn to use the code:
- Start with the script examples/example.py, which contains a series of sample commands to load an image and array, generate data, and produce an image with various imaging algorithms.
- Slides from the EHT2016 data generation and imaging workshop contain a tutorial on generating data with the VLBI imaging website, loading into the library, and producing an image. Note that this presentation used a previous version of the code -- some function names and prefixes may need to be updated.
If you use ehtim in your publication, please cite both Chael et al. 2016 and Chael et al. 2018
Let us know if you use ehtim in your publication and we'll list it here!
- High-Resolution Linear Polarimetric Imaging for the Event Horizon Telescope, Chael et al. 2016
- Computational Imaging for VLBI Image Reconstruction, Bouman et al. 2016
- Stochastic Optics: A Scattering Mitigation Framework for Radio Interferometric Imaging, Johnson 2016
- Quantifying Intrinsic Variability of Sgr A* using Closure Phase Measurements of the Event Horizon Telescope, Roelofs et al. 2017
- Reconstructing Video from Interferometric Measurements of Time-Varying Sources, Bouman et al. 2017
- Dynamical Imaging with Interferometry, Johnson et al. 2017
- Interferometric Imaging Directly with Closure Phases and Closure Amplitudes, Chael et al. 2018
- A Model for Anisotropic Interstellar Scattering and its Application to Sgr A*, Psaltis et al. 2018
- The Currrent Ability to Test Theories of Gravity with Black Hole Shadows, Mizuno et al. 2018
- The Scattering and Intrinsic Structure of Sagittarius A* at Radio Wavelengths, Johnson et al. 2018
- How to tell an accreting boson star from a black hole, Olivares et al. 2018
- Testing General Relativity with the Black Hole Shadow Size and Asymmetry of Sagittarius A*: Limitations from Interstellar Scattering, Zhu et al. 2018
- The Size, Shape, and Scattering of Sagittarius A* at 86 GHz: First VLBI with ALMA, Issaoun et al. 2019
The oifits_new code used for reading/writing .oifits files is a slightly modified version of Paul Boley's package at http://astro.ins.urfu.ru/pages/~pboley/oifits. The oifits read/write functionality is still being developed and may not work with all versions of python or astropy.
The documentation is styled after dfm's projects
ehtim is licensed under GPLv3. See LICENSE.txt for more details.