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20032007
most citedThe UV properties of E+A galaxies: constraints on feedback-driven quenching of star formation

137 citations · 395 across the 7 of their papers we have counts for

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astro-ph200777 cited

Galaxy Mergers at z>1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive Galaxies

R. E. Ryan, S. H. Cohen, R. A. Windhorst +1

We present a measurement of the galaxy merger fraction and number density from observations in the Hubble Ultra Deep Field for 0.5<z<2.5. We fit the combination of broadband data a…

astro-ph2007

AGN feedback from Jet-ISM/IGM interactions

V. Antonuccio-Delogu, J. Silk

We study the propagation of relativistic jets originating from AGNs within the Interstellar/Intergalactic Medium of their host galaxies, and use it to build a model for the suppres…

astro-ph2007137 cited

The UV properties of E+A galaxies: constraints on feedback-driven quenching of star formation

S. Kaviraj, L. A. Kirkby, J. Silk +1

We present the first large-scale study of E+A (post-starburst) galaxies that incorporates photometry in the ultraviolet (UV) wavelengths. We find that the starburst that creates th…

astro-ph200736 cited

Observational biases in Lagrangian reconstructions of cosmic velocity fields

G. Lavaux, R. Mohayaee, S. Colombi +3

Lagrangian reconstruction of large-scale peculiar velocity fields can be strongly affected by observational biases. We develop a thorough analysis of these systematic effects by re…

astro-ph200768 cited

Sterile neutrinos as subdominant warm dark matter

A. Palazzo, D. Cumberbatch, A. Slosar +1

In light of recent findings which seem to disfavor a scenario with (warm) dark matter entirely constituted of sterile neutrinos produced via the Dodelson-Widrow (DW) mechanism, we…

astro-ph200741 cited

Cluster abundances and S-Z power spectra: effects of non-Gaussianity and early dark energy

S. Sadeh, Y. Rephaeli, J. Silk

In the standard Lambda CDM cosmological model with a Gaussian primordial density fluctuation field, the relatively low value of the mass variance parameter (sigma_8=0.74{+0.05}{-0.…