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20022009
most citedPLUMED: a portable plugin for free-energy calculations with molecular dynamics

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6 papers · 1 filter

astro-ph.CO200948 cited

Color Distributions, Number and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations

Stijn Wuyts, Marijn Franx, Thomas J. Cox +9

We present a comparison between the observed color distribution, number and mass density of massive galaxies at 1.5 < z < 3 and a model by Hopkins et al. that relates the quasar an…

astro-ph.CO2009108 cited

The Rest-Frame Optical Luminosity Function of Cluster Galaxies at z<0.8 and the Assembly of the Cluster Red Sequence

Gregory Rudnick, Anja von der Linden, Roser Pello +12

We present the rest-frame optical luminosity function (LF) of red sequence galaxies in 16 clusters at 0.4<z<0.8 drawn from the ESO Distant Cluster Survey (EDisCS). We compare our c…

astro-ph.CO200927 cited

Interpretation and implication of the non-detection of GeV spectrum excess by Fermi gamma-ray Space Telescope in most GRBs

Yi-Zhong Fan

Since the launch of the Fermi Gamma-ray Space Telescope on 11 June 2008, significant detections of high energy emission have been reported only in six Gamma-ray Bursts (GRBs) until…

astro-ph.CO200958 cited

Frequency and properties of bars in cluster and field galaxies at intermediate redshifts

Fabio D. Barazza, Pascale Jablonka, Vandana Desai +15

We present a study of large-scale bars in field and cluster environments out to redshifts of ~0.8 using a final sample of 945 moderately inclined disk galaxies drawn from the EDisC…

astro-ph.CO200935 cited

The Building the Bridge survey for z=3 Ly-alpha emitting galaxies II: Completion of the survey

L. F. Grove, J. P. U. Fynbo, C. Ledoux +4

(Abridged). We aim at bridging the gap between absorption selected and emission selected galaxies at z~3 by probing the faint end of the luminosity function of star-forming galaxie…

astro-ph.CO200988 cited

The optical afterglows and host galaxies of three short/hard gamma-ray bursts

P. D'Avanzo, D. Malesani, S. Covino +17

Short GRBs are commonly thought to originate from the merging of double compact object binaries but direct evidence for this scenario is still missing. Optical observations of shor…