Restoration of the Tully–Fisher Relation by Statistical Rectification

Abstract

I employ the Lucy rectification algorithm to recover the inclination-corrected distribution of local disk galaxies in the plane of absolute magnitude ( M _i ) and H i velocity width ( W _20 ). By considering the inclination angle as a random variable with a known probability distribution, the novel approach eliminates one major source of uncertainty in studies of the Tully–Fisher relation: inclination angle estimation from axial ratio. Leveraging the statistical strength derived from the entire sample of 28,264 H i -selected disk galaxies at z M _i > −22: ${M}_{i}={M}_{0}-2.5\beta \ [\mathrm{log}({W}_{20}/250\mathrm{km}/{\rm{s}})]$ , with M _0 = −19.77± 0.04 and β = 4.39 ± 0.06. At the brighter end ( M _i M _i > −23, while σ ( M _i ) decreases from ∼0.8 in slow rotators to ∼0.4 in fast rotators. The statistical rectification method holds significant potential, especially in the studies of intermediate-to-high-redshift samples, where limited spatial resolution hinders precise measurements of inclination angles.

Keywords

• Astrostatistics
• Scaling relations
• Disk galaxies
• Galaxy rotation
• Galaxy luminosities