uvmcmcfit | Python software that uses emcee

by sbussmann Python Version: v0.1.1 License: Non-SPDX

X-Ray Key Features Code Snippets Community Discussions Vulnerabilities Install Support

kandi X-RAY | uvmcmcfit Summary

uvmcmcfit is a Python library. uvmcmcfit has no bugs, it has no vulnerabilities and it has low support. However uvmcmcfit build file is not available and it has a Non-SPDX License. You can download it from GitHub.

Detailed documentation is available at Python software to fit models to interferometric data, appropriately accounting for gravitational lensing as needed.

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Quality

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License

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Support

uvmcmcfit has a low active ecosystem.

It has 7 star(s) with 5 fork(s). There are 5 watchers for this library.

It had no major release in the last 12 months.

uvmcmcfit has no issues reported. There are no pull requests.

It has a neutral sentiment in the developer community.

The latest version of uvmcmcfit is v0.1.1

Quality

uvmcmcfit has no bugs reported.

Security

uvmcmcfit has no vulnerabilities reported, and its dependent libraries have no vulnerabilities reported.

License

uvmcmcfit has a Non-SPDX License.

Non-SPDX licenses can be open source with a non SPDX compliant license, or non open source licenses, and you need to review them closely before use.

Reuse

uvmcmcfit releases are available to install and integrate.

uvmcmcfit has no build file. You will be need to create the build yourself to build the component from source.

Installation instructions are not available. Examples and code snippets are available.

Top functions reviewed by kandi - BETA

kandi has reviewed uvmcmcfit and discovered the below as its top functions. This is intended to give you an instant insight into uvmcmcfit implemented functionality, and help decide if they suit your requirements.

Plot the test fitting
Compute the sensitivity map for a set of sources
Logarithm of the log likelihood
Return the phase center of the image
Load the UV spectrum
Compute the likelihood of a poff_model
Load parameters from an ALMA image file
Generate matplotlib plot
Generator to iterate over a set of figures
Rolls up a visibilities from a visfile
Plot the covariance
Pre - prune a PDF
Remove columns from PDF data
Convert a visw file to a wt file
Calculate the value of the statistic wgt
Calculate spectral average spectral average spectrum
Load a vispy file
Plots the best fit of the posterior PDF
Prints the parameters of the fit
Fit a uvm model to a given model
Subtracts the visibilities from the model
Zerow tz file
Load parameters from an ALMA image file
Scales the weights of vispy
Find the best fit of the posterior PDF
Evaluate the evolution of the posterior pdf
Load the UV data from a file
Generate a mask for a given image
Load the phase center of the image

Get all kandi verified functions for this library.

uvmcmcfit Key Features

No Key Features are available at this moment for uvmcmcfit.

uvmcmcfit Examples and Code Snippets

No Code Snippets are available at this moment for uvmcmcfit.

Community Discussions

No Community Discussions are available at this moment for uvmcmcfit.Refer to stack overflow page for discussions.

Community Discussions, Code Snippets contain sources that include Stack Exchange Network

Vulnerabilities

No vulnerabilities reported

Install uvmcmcfit

You can download it from GitHub.
You can use uvmcmcfit like any standard Python library. You will need to make sure that you have a development environment consisting of a Python distribution including header files, a compiler, pip, and git installed. Make sure that your pip, setuptools, and wheel are up to date. When using pip it is generally recommended to install packages in a virtual environment to avoid changes to the system.

Support

For any new features, suggestions and bugs create an issue on GitHub. If you have any questions check and ask questions on community page Stack Overflow .

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