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DESI EDR: Calibrating the Tully–Fisher Relationship with the DESI Peculiar Velocity Survey

  • K. Douglass*
  • , S. BenZvi
  • , N. Uberoi
  • , C. Howlett
  • , C. Saulder
  • , K. Said
  • , R. Demina
  • , J. Aguilar
  • , S. Ahlen
  • , G. Aldering
  • , D. Bianchi
  • , D. Brooks
  • , T. Claybaugh
  • , A. Cuceu
  • , T. M. Davis
  • , K. S. Dawson
  • , A. De la Macorra
  • , A. Font-Ribera
  • , J. E. Forero-Romero
  • , E. Gaztañaga
  • S. Gontcho A Gontcho, G. Gutierrez, C. Hahn, K. Honscheid, M. Ishak, R. Joyce, T. Kisner, A. Kremin, M. Landriau, M. E. Levi, J. Lucey, P. Martini, A. Meisner, R. Miquel, J. Moustakas, N. Palanque-Delabrouille, W. J. Percival, F. Prada, G. Rossi, E. Sanchez, D. Schlegel, M. Schubnell, J. Silber, D. Sprayberry, G. Tarlé, B. A. Weaver, R. Zhou, H. Zou
*Corresponding author for this work

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Abstract

We calibrate the Tully–Fisher relation (TFR) with data from the DESI Peculiar Velocity (PV) Survey taken during the Survey Validation (SV) period of the DESI galaxy redshift survey. Placing spectroscopic fibers on the centers and major axes of spatially extended spiral galaxies identified in the 2020 Siena Galaxy Atlas using the DESI Legacy Surveys, we measure the rotational velocities at 0.33R 26 for 1155 (1128 + 27 dwarf) spiral galaxies observed during SV. Using 39 spiral galaxies observed in the Coma cluster, we find a slope for the TFR of −8.32 ± 0.15 AB mag in the r band, with a scatter about the TFR of 1.12 ± 0.03 AB mag. We calibrate the zero-point of the TFR using galaxies with independent distances measured using type Ia supernovae (SNe Ia) via the cosmological distance ladder. From the SN Ia distances, we measure a zero-point of − 19.21−0.31+0.30 AB mag in the r band. We produce a public catalog of the distances to these 1128 spiral galaxies observed during DESI SV as part of the DESI PV Survey with our calibrated TFR. This is, to our knowledge, the first catalog of TFR distances produced with velocities measured at a single point in the disk.

Original languageEnglish
Article number20
Number of pages14
JournalAstrophysical Journal
Volume1001
Issue number1
Early online date2 Apr 2026
DOIs
Publication statusPublished - 10 Apr 2026

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