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19912026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

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611 papers · 1 filter

astro-ph2008★ 92 cited

Optimal filter systems for photometric redshift estimation

N. Benitez, M. Moles, J. A. L. Aguerri +18

In the next years, several cosmological surveys will rely on imaging data to estimate the redshift of galaxies, using traditional filter systems with 4-5 optical broad bands; narro…

astro-ph2008★ 10 cited

Detection of the second eclipsing high mass X-ray binary in M 33

W. Pietsch, F. Haberl, T. J. Gaetz +7

Chandra data of the X-ray source [PMH2004] 47 were obtained in the ACIS Survey of M 33 (ChASeM33) in 2006. During one of the observations, the source varied from a high state to a…

astro-ph2008★ 613 cited

The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements II. The Full Sample of Reverberation-Mapped AGNs

Misty C. Bentz, Bradley M. Peterson, Hagai Netzer +2

We present high-resolution HST images of all 35 AGNs with optical reverberation-mapping results, which we have modeled to create a nucleus-free image of each AGN host galaxy. From…

astro-ph2008★ 128 cited

The halo merger rate in the Millennium Simulation and implications for observed galaxy merger fractions

S. Genel, R. Genzel, N. Bouché +2

We developed a new method to extract halo merger rates from the Millennium Simulation. First, by removing superfluous mergers that are artifacts of the FOF halo finder, we find a l…

astro-ph2008★ 43 cited

Metal-Absorption Column Densities in Fast Radiative Shocks

Orly Gnat, Amiel Sternberg

In this paper we present computations of the integrated metal-ion column densities produced in the post-shock cooling layers behind fast, radiative shock-waves. For this purpose, w…

astro-ph2008★ 40 cited

Photometry and Spin Rate Distribution of Small-Sized Main Belt Asteroids

D. Polishook, N. Brosch

Photometry results of 32 asteroids are reported from only seven observing nights on only seven fields, consisting of 34.11 cumulative hours of observations. The data were obtained…