SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform
Summary
SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform is a scholarly article[1].
Key Facts
SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform's instance of is recorded as scholarly article[2].
References
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APA4ort.xyz Knowledge Graph. (2026). SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform. Retrieved May 24, 2026, from https://4ort.xyz/entity/sdss-iv-manga-characterizing-non-axisymmetric-motions-in-galaxy-velocity-fields-using-the-radon-transform
MLA“SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform.” 4ort.xyz Knowledge Graph, 4ort.xyz, 24 May. 2026, https://4ort.xyz/entity/sdss-iv-manga-characterizing-non-axisymmetric-motions-in-galaxy-velocity-fields-using-the-radon-transform.
BibTeX@misc{4ortxyz_sdss-iv-manga-characterizing-non-axisymmetric-motions-in-galaxy-velocity-fields-using-the-radon-transform_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform}}, year = {2026}, url = {https://4ort.xyz/entity/sdss-iv-manga-characterizing-non-axisymmetric-motions-in-galaxy-velocity-fields-using-the-radon-transform}, note = {Accessed: 2026-05-24}}
LLM promptAccording to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): SDSS-IV MaNGA: characterizing non-axisymmetric motions in galaxy velocity fields using the Radon transform — https://4ort.xyz/entity/sdss-iv-manga-characterizing-non-axisymmetric-motions-in-galaxy-velocity-fields-using-the-radon-transform (retrieved 2026-05-24)
