@article{https://doi.org/10.48550/arxiv.2111.03070,<br/><span class="tab"></span>
  doi = {10.48550/ARXIV.2111.03070},<br/><span class="tab"></span>
  url = {https://arxiv.org/abs/2111.03070},<br/><span class="tab"></span>
  author = {Bar,<br/><span class="tab"></span> Nitsan and Blum,<br/><span class="tab"></span> Kfir and Sun,<br/><span class="tab"></span> Chen},<br/><span class="tab"></span>
  keywords = {High Energy Physics - Phenomenology (hep-ph),<br/><span class="tab"></span> Cosmology and Nongalactic Astrophysics (astro-ph.CO),<br/><span class="tab"></span> Astrophysics of Galaxies (astro-ph.GA),<br/><span class="tab"></span> FOS: Physical sciences,<br/><span class="tab"></span> FOS: Physical sciences},<br/><span class="tab"></span>
  title = {Galactic rotation curves versus ultralight dark matter: A systematic comparison with SPARC data},<br/><span class="tab"></span>
  publisher = {arXiv},<br/><span class="tab"></span>
  year = {2021},<br/><span class="tab"></span>
  copyright = {arXiv.org perpetual,<br/><span class="tab"></span> non-exclusive license}
}