sage-archive-2023-02-01 | repository used to be the user-facing mirror

 by   sagemath Python Version: 9.7 License: Non-SPDX

kandi X-RAY | sage-archive-2023-02-01 Summary

kandi X-RAY | sage-archive-2023-02-01 Summary

sage-archive-2023-02-01 is a Python library. sage-archive-2023-02-01 has no bugs, it has no vulnerabilities and it has medium support. However sage-archive-2023-02-01 build file is not available and it has a Non-SPDX License. You can download it from GitHub.

This repository used to be the user-facing mirror of the Sage source tree. As Sage development migrated on 2023-02-01 from https://trac.sagemath.org/ to our new repository on GitHub, https://github.com/sagemath/sage, we have renamed and archived this repository.
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            kandi-support Support

              sage-archive-2023-02-01 has a medium active ecosystem.
              It has 2067 star(s) with 436 fork(s). There are 132 watchers for this library.
              OutlinedDot
              It had no major release in the last 12 months.
              There are 0 open issues and 36 have been closed. On average issues are closed in 191 days. There are no pull requests.
              It has a neutral sentiment in the developer community.
              The latest version of sage-archive-2023-02-01 is 9.7

            kandi-Quality Quality

              sage-archive-2023-02-01 has no bugs reported.

            kandi-Security Security

              sage-archive-2023-02-01 has no vulnerabilities reported, and its dependent libraries have no vulnerabilities reported.

            kandi-License License

              sage-archive-2023-02-01 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.

            kandi-Reuse Reuse

              sage-archive-2023-02-01 releases are available to install and integrate.
              sage-archive-2023-02-01 has no build file. You will be need to create the build yourself to build the component from source.
              Installation instructions, examples and code snippets are available.

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            sage-archive-2023-02-01 Key Features

            No Key Features are available at this moment for sage-archive-2023-02-01.

            sage-archive-2023-02-01 Examples and Code Snippets

            No Code Snippets are available at this moment for sage-archive-2023-02-01.

            Community Discussions

            No Community Discussions are available at this moment for sage-archive-2023-02-01.Refer to stack overflow page for discussions.

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

            Vulnerabilities

            No vulnerabilities reported

            Install sage-archive-2023-02-01

            The Sage Installation Guide provides a decision tree that guides you to the type of installation that will work best for you. This includes building from source, obtaining Sage from a package manager, using a container image, or using Sage in the cloud. This README contains self-contained instructions for building Sage from source. It assumes that you have already cloned the git repository or downloaded the sources in the form of a tarball. If you have questions or encounter problems, please do not hesitate to email the sage-support mailing list or ask on the Ask Sage questions and answers site.

            Support

            Sage attempts to support all major Linux distributions, recent versions of macOS, and Windows (using Windows Subsystem for Linux or virtualization). Detailed information on supported platforms for a specific version of Sage can be found in the section "Availability and installation help" of the release tour for this version. We highly appreciate contributions to Sage that fix portability bugs and help port Sage to new platforms; let us know at the sage-devel mailing list.
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            gh repo clone sagemath/sage-archive-2023-02-01

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            git@github.com:sagemath/sage-archive-2023-02-01.git

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