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19962007
most citedHow cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest

207 citations · 207 across the 1 of their papers we have counts for

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astro-ph2007207 cited

How cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest

M. Viel, G. D. Becker, J. S. Bolton +3

We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha flux power spectrum of 55 high- resolution HIRES spectra at 2.0 < z < 6.4. From…

astro-ph2001

Measuring Black Hole Masses Using Ionized Gas Kinematics

Aaron J. Barth, Marc Sarzi, Luis C. Ho +5

We describe techniques for measuring the central masses of galaxies using emission-line kinematics observed with the Hubble Space Telescope. For accurate results, it is necessary t…

astro-ph2001

The Central Regions of Early-Type Galaxies Hosting Active Galactic Nuclei as Viewed with HST/NICMOS

Swara Ravindranath, Luis C. Ho, Chien Y. Peng +2

We present preliminary results from surface photometry of a sample of early-type galaxies observed with NICMOS on board HST in the F160W (H-band) filter. Dust is found to occur mos…

astro-ph2000

Supermassive Black Holes from the SUNNS survey

Marc Sarzi, Hans-Walter Rix, Joseph C. Shields +5

We report three new accurate mass measurements for the supermassive black holes hosted by the early-type disk galaxies NGC2787, NGC4459 and NGC4596. The targets were selected from…

astro-ph2000

Variability in LINERs

J. C. Shields, H. -W. Rix, D. H. McIntosh +6

A small number of LINERs have been seen to display variable H-alpha emission with a very broad, double-peaked profile. Recent observations with the Hubble Space Telescope indicate…

astro-ph2000

Oxygen Abundance Determination in Very Metal-Deficient Giants: Permitted O I Lines Versus Forbidden [O I] Lines

Y. Takeda, M. Takada-Hidai, S. Sato +4

The abundance of oxygen was determined for selected very metal-poor G-K stars (six giants and one turn-off star) based on the high S/N and high-resolution spectra observed with Kec…