Calibrated Tully–Fisher relations for improved estimates of disc rotation velocities
Version of Record online: 9 SEP 2011
© 2011 The Authors. Monthly Notices of the Royal Astronomical Society © 2011 RAS
Monthly Notices of the Royal Astronomical Society
Volume 417, Issue 3, pages 2347–2386, November 2011
How to Cite
Reyes, R., Mandelbaum, R., Gunn, J. E., Pizagno, J. and Lackner, C. N. (2011), Calibrated Tully–Fisher relations for improved estimates of disc rotation velocities. Monthly Notices of the Royal Astronomical Society, 417: 2347–2386. doi: 10.1111/j.1365-2966.2011.19415.x
- Issue online: 20 OCT 2011
- Version of Record online: 9 SEP 2011
- Accepted 2011 July 11. Received 2011 July 11; in original form 2011 June 7
Table 1. Basic properties of the 189 galaxies in the child disc sample.
Table 3. Best-fit parameters from i-band B+D fits for 189 galaxies in the child disc sample.
Table 4. Observations with DIS at APO 3.5m (95 galaxies).
Table 5. Rotation curve fit parameters and rotation velocity amplitudes for the child disc sample (189 galaxies).
|MNR_19415_sm_tables.zip||21K||Supporting info item|
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