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phasecurvefit #285

@nstarman

Description

@nstarman

Submitting Author: (@nstarman)
All current maintainers: (@nstarman, @jnibauer)
Package Name: phasecurvefit
Construct paths through phase-space points, with JAX.
Repository Link: https://github.com/GalacticDynamics/phasecurvefit
Version submitted: v0.1.0
EiC: @crhea93
Editor: TBD
Reviewer 1: TBD
Reviewer 2: TBD
Archive: TBD
JOSS DOI: TBD
Version accepted: TBD
Date accepted (month/day/year): TBD


Code of Conduct & Commitment to Maintain Package

Description

Filamentary structures are ubiquitous in the physical sciences, ranging from coherent streams of stars called stellar streams to elongated structures in turbulent fluids, plasmas, and the interstellar medium. In the context of stellar streams, a common preprocessing step is ordering observational or simulation data to derive the mean path of the stream's trajectory through phase-space.

phasecurvefit is an open-source Python package for constructing such orderings and paths by walking along the local phase-space flow using. There are two core components: the first is walk_local_flow which builds an approximate ordering and trajectory but which might miss some of the data; and the second is a fast-to-train autoencoder that imputes the full ordering and trajectory.

Scope

  • Please indicate which category or categories.
    Check out our package scope page to learn more about our
    scope. (If you are unsure of which category you fit, we suggest you make a pre-submission inquiry):

    • Data retrieval
    • Data extraction
    • Data processing/munging
    • Data deposition
    • Data validation and testing
    • Data visualization1
    • Workflow automation
    • Citation management and bibliometrics
    • Scientific software wrappers
    • Database interoperability

Domain Specific

  • Geospatial
  • Education

Community Partnerships

If your package is associated with an existing community please check below:

While this package does not directly interface with Astropy, it easily interoperates with it, through unxt, which brings Astropy to JAX.

  • For all submissions, explain how and why the package falls under the categories you indicated above. In your explanation, please address the following points (briefly, 1-2 sentences for each):

    • Who is the target audience and what are scientific applications of this package?

The target audience is scientists with data or simulations of stellar streams, or similar filamentary structures like elongated structures in turbulent fluids, plasmas, and the interstellar medium. Current scientific applications of this package, not by the submitters, are analyses of Milky Way stellar streams data, fitting the path of the stream for orbit and membership likelihood analyses.

  • Are there other Python packages that accomplish the same thing? If so, how does yours differ?

Not to our knowledge. Our code, written in JAX, not only fits stream-like structures in phase space, it does so differentiably e.g. for use in gradient-utilizing inference pipelines.

  • If you made a pre-submission enquiry, please paste the link to the corresponding issue, forum post, or other discussion, or @tag the editor you contacted:

Technical checks

For details about the pyOpenSci packaging requirements, see our packaging guide. Confirm each of the following by checking the box. This package:

  • does not violate the Terms of Service of any service it interacts with.
  • uses an OSI approved license.
  • contains a README with instructions for installing the development version.
  • includes documentation with examples for all functions.
  • contains a tutorial with examples of its essential functions and uses.
  • has a test suite.
  • has continuous integration setup, such as GitHub Actions CircleCI, and/or others.

Publication Options

JOSS Checks
  • The package has an obvious research application according to JOSS's definition in their submission requirements. Be aware that completing the pyOpenSci review process does not guarantee acceptance to JOSS. Be sure to read their submission requirements (linked above) if you are interested in submitting to JOSS.
  • The package is not a "minor utility" as defined by JOSS's submission requirements: "Minor ‘utility’ packages, including ‘thin’ API clients, are not acceptable." pyOpenSci welcomes these packages under "Data Retrieval", but JOSS has slightly different criteria.
  • The package contains a paper.md matching JOSS's requirements with a high-level description in the package root or in inst/. Yes, in the PR 📝 docs: JOSS paper GalacticDynamics/phasecurvefit#3, which will be merged on acceptance
  • The package is deposited in a long-term repository with the DOI: 10.5281/zenodo.18714341

Note: JOSS accepts our review as theirs. You will NOT need to go through another full review. JOSS will only review your paper.md file. Be sure to link to this pyOpenSci issue when a JOSS issue is opened for your package. Also be sure to tell the JOSS editor that this is a pyOpenSci reviewed package once you reach this step.

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This option will allow reviewers to open smaller issues that can then be linked to PR's rather than submitting a more dense text based review. It will also allow you to demonstrate addressing the issue via PR links.

  • Yes I am OK with reviewers submitting requested changes as issues to my repo. Reviewers will then link to the issues in their submitted review.

Confirm each of the following by checking the box.

  • I have read the author guide.
  • I expect to maintain this package for at least 2 years and can help find a replacement for the maintainer (team) if needed.

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Footnotes

  1. Please fill out a pre-submission inquiry before submitting a data visualization package.

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