Add to ORKGIn this paper, we derive scaling relations between photometric observable quantities and disc galaxy rotation velocity Vrot or Tully-Fisher relations (TFRs). Our methodology is dictated by our purpose of obtaining purely photometric, minimal-scatter estimators of Vrot applicable to large galaxy samples from imaging surveys. To achieve this goal, we have constructed a sample of 189 disc galaxies at redshifts
The relation between galaxy luminosity L and halo virial velocity v_vir required to fit the galaxy l...
We measured the distribution in absolute magnitude - circular velocity space for a well-defined samp...
In this paper, we derive scaling relations between photometric observable quantities and disc galaxy...
In this paper, we derive scaling relations between photometric observable quantities and disc galaxy...
In this paper, we derive scaling relations between photometric observable quantities and disk galaxy...
We present calibrated scaling relations (also referred to as Tully-Fisher relations or TFRs) between...
We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] ...
The statistical properties of the Tully-Fisher relation provide important constraints for semi-analy...
We construct Tully–Fisher relationships (TFRs) in the u, g, r, i and z bands and stellar mass TFRs f...
The Tully-Fisher (TF) relation is an empirically establish correlation between the luminosity of s...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
In this paper, we investigate the statistical properties of the Tully-Fisher relation (TFr) for a sa...
We present an I-band Tully-Fisher relation (TFR) for 18 nearby S0 galaxies using kinematics derived ...
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
Observational parameters which can be used for redshift-independent distance determination using the...
The relation between galaxy luminosity L and halo virial velocity v_vir required to fit the galaxy l...
We measured the distribution in absolute magnitude - circular velocity space for a well-defined samp...
In this paper, we derive scaling relations between photometric observable quantities and disc galaxy...
In this paper, we derive scaling relations between photometric observable quantities and disc galaxy...
In this paper, we derive scaling relations between photometric observable quantities and disk galaxy...
We present calibrated scaling relations (also referred to as Tully-Fisher relations or TFRs) between...
We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] ...
The statistical properties of the Tully-Fisher relation provide important constraints for semi-analy...
We construct Tully–Fisher relationships (TFRs) in the u, g, r, i and z bands and stellar mass TFRs f...
The Tully-Fisher (TF) relation is an empirically establish correlation between the luminosity of s...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
In this paper, we investigate the statistical properties of the Tully-Fisher relation (TFr) for a sa...
We present an I-band Tully-Fisher relation (TFR) for 18 nearby S0 galaxies using kinematics derived ...
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
Observational parameters which can be used for redshift-independent distance determination using the...
The relation between galaxy luminosity L and halo virial velocity v_vir required to fit the galaxy l...
We measured the distribution in absolute magnitude - circular velocity space for a well-defined samp...
In this paper, we derive scaling relations between photometric observable quantities and disc galaxy...