The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics

Abstract

The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics

arXiv commentAccepted to A&A

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Cited by in corpus (8)

• Stellar kinematics across the Hubble sequence in the CALIFA survey: General properties and aperture corrections
• Kinematic scaling relations of CALIFA galaxies: A dynamical mass proxy for galaxies across the Hubble sequence
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass
• The SAMI Galaxy Survey: The Low-Redshift Stellar Mass Tully-Fisher Relation
• Uncertainties in gas kinematics arising from stellar continuum modelling in integral field spectroscopy data: the case of NGC2906 observed with MUSE/VLT
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Rotation curves and dynamical masses of MaNGA barred galaxies