Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations

@article{Kourkchi2020Cosmicflows4T,
  title={Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations},
  author={E. Kourkchi and R. Tully and G. Anand and H. Courtois and A. Dupuy and J. Neill and L. Rizzi and M. Seibert},
  journal={arXiv: Astrophysics of Galaxies},
  year={2020}
}
This study is a part of the Cosmicflows-4 project with the aim of measuring the distances of more than ~10,000 spiral galaxies in the local universe up to ~15,000 km/s. New HI linewidth information has come primarily from the Arecibo Legacy Fast ALFA Survey. Photometry of our sample galaxies has been carried out in optical (SDSS u, g, r, i, z) and infrared (WISE W1 and W2) bands. Inclinations have been determined using an online graphical interface accessible to a collaboration of citizen… Expand
$H_0$ tension without CMB: beyond $\Lambda$CDM
Cosmicflows-4: The Catalog of ~10000 Tully-Fisher Distances

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