The Assembly History of Disk Galaxies. I. The Tully-Fisher Relation to z ≃ 1.3 from Deep Exposures with DEIMOS

Creators: Miller, Sarah H.; Bundy, Kevin; Sullivan, Mark; Ellis, Richard S.; Treu, Tommaso

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Abstract

We present new measures of the evolving scaling relations between stellar mass, luminosity and rotational velocity for a morphologically inclusive sample of 129 disk-like galaxies with z_(AB) < 22.5 in the redshift range 0.2

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© 2011 The American Astronomical Society. Received 2011 February 18; accepted 2011 August 15; published 2011 October 25. S.H.M. thanks the Rhodes Trust, the Oxford Astrophysics Department, New College, Oxford, and the California Institute of Technology for supporting her work. M.S. and R.S.E. acknowledge financial support from the Royal Society. We thank S. Moran, N. Miller, G. Mikelsons, and K. Chiu for considerable initial assistance with the organization of this data set. We thank C. Peng for supplying us with galfit 3.0 and acknowledge useful discussions with A. Benson, A. Brooks, A. Bunker, M. Bureau, M. Cappellari, R. Davies, H. Flores, F. Hammer, S. Kassin, L. Miller, and M. Puech. The referee, B. Weiner, is acknowledged for his constructive comments in the improvement of this paper. The spectroscopic data was secured with the W. M. Keck Observatory on Mauna Kea. We thank the observatory staff for their dedication and support. The authors recognize and acknowledge the cultural role and reverence that the summit of Mauna Kea has always had with the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

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