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19972006
most citedLuminosity and stellar mass functions of disks and spheroids in the SDSS and the supermassive black hole mass function

93 citations · 93 across the 2 of their papers we have counts for

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astro-ph200693 cited

Luminosity and stellar mass functions of disks and spheroids in the SDSS and the supermassive black hole mass function

A. J. Benson, Dajana Dzanovic, C. S. Frenk +1

Using the Galactica code of Benson et al., we obtain quantitative measurements of spheroid-to-disk ratios for a sample of 8839 galaxies observed in the Sloan Digital Sky Survey. We…

astro-ph2002

Kinematics of parsec-scale structures in AGN: the 2cm VLBA Survey

E. Ros, K. I. Kellermann, M. L. Lister +5

We are investigating the kinematics of jets in active galactic nuclei on parsec scales by studying a representative population of sources. This study is being carried out using the…

astro-ph2001

Statistical Properties of DLAs and sub-DLAs

Celine Peroux, Mike J. Irwin, Richard G. McMahon +1

Quasar absorbers provide a powerful observational tool with which to probe both galaxies and the intergalactic medium up to high redshift. We present a study of the evolution of th…

astro-ph2001

Large scale star formation in galaxies. II. The spirals NGC 3377A, NGC 3507 and NGC 4394

A. Vicari, P. Battinelli, R. Capuzzo--Dolcetta +2

The identification of young star groupings (YSG) in the three spiral galaxies NGC 3377A, NGC 3507, NGC 4394 is obtained by mean of the statistical method described in Paper I. We f…

astro-ph2000

Evidence for Galaxy Formation at High Redshift

T. Shanks, N. Metcalfe, R. Fong +3

We have shown previously that galaxy counts from the UV to the near-IR are well-fitted by simple evolutionary models where the space density of galaxies remains constant with look-…

astro-ph2000

Extensive molecular gas in the tidal arms near NGC3077 - Birth of a dwarf galaxy?

Andreas Heithausen, Fabian Walter

Using the IRAM 30m radio telescope we have mapped the tidal arm feature south-east of NGC3077 where we recently detected molecular gas in the CO (J=1-0) and (2-1) transitions. We f…