most citedMeasurements of Strange Particle Production in Collisions at = 200 GeV

368 citations · 776 across the 8 of their papers we have counts for

collaborators

8 papers

nucl-ex200818 cited

Azimuthal dependence of pion source radii in Pb+Au collisions at 158 A GeV

CERES Collaboration, D. Adamova, G. Agakichiev +54

We present results of a two-pion correlation analysis performed with the Au+Pb collision data collected by the upgraded CERES experiment in the fall of 2000. The analysis was done…

astro-ph200666 cited

Five years of searches for point sources of astrophysical neutrinos with the AMANDA-II neutrino telescope

A. Achterberg

We report the results of a five-year survey of the northern sky to search for point sources of high energy neutrinos. The search was performed on the data collected with the AMANDA…

nucl-ex2006107 cited

Modification of the rho meson detected by low-mass electron-positron pairs in central Pb-Au collisions at 158 A GeV/c

CERES Collaboration, D. Adamova

We present a measurement of pair production in central Pb-Au collisions at 158 GeV/. As reported earlier, a significant excess of the pair yield over the ex…

astro-ph200644 cited

On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

A. Achterberg et al.

The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking…

nucl-ex200647 cited

Neutral Kaon Interferometry in Au+Au collisions at sqrt(s_NN) = 200 GeV

STAR Collaboration, B. I. Abelev

We present the first statistically meaningful results from two-K0s interferometry in heavy-ion collisions. A model that takes the effect of the strong interaction into account has…

nucl-ex2006368 cited

Measurements of Strange Particle Production in Collisions at = 200 GeV

STAR Collaboration, B. Abelev

We present strange particle spectra and yields measured at mid-rapidity in GeV proton-proton () collisions at RHIC. We find that the previously observed…