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M200

 
National Institutes of Health

Papers overview

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2017
2017
Characterizing the evolution of the faint end of the cluster red sequence (RS) galaxy luminosity function (GLF) with redshift is… Expand
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2015
2015
We present the discovery of two galaxy overdensities in the Hubble Space Telescope UDF: a proto-cluster, HUDFJ0332.4-2746.6 at z… Expand
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Highly Cited
2014
Highly Cited
2014
We analyse the mass–size relation of ∼400 quiescent massive ETGs (M_*/M_⊙ > 3 × 10^(10)) hosted by massive clusters (M_(200 ∼ 2–7… Expand
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2011
2011
Context: In tablet manufacturing, less attention is paid to the measurement of die-wall pressure than to force–displacement… Expand
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Highly Cited
2010
Highly Cited
2010
Context. Galaxy clusters represent valuable cosmological probes us ing tests that mainly rely on measurements of cluster masses… Expand
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Highly Cited
2007
Highly Cited
2007
We use the Millennium Simulation (MS) to measure the cross-correlation between halo centres and mass (or equivalently the average… Expand
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2007
2007
The gene encoding an epoxide hydrolase from Aspergillus niger M200 has been cloned and its sequence determined. The gene is… Expand
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Highly Cited
1999
Highly Cited
1999
We investigate the gravitational lensing properties of dark matter halos with Navarro, Frenk & White (NFW) density profiles and… Expand
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Highly Cited
1991
Highly Cited
1991
Recently, Hoke et al. (1989) and Pantev et al. (1989) demonstrated that the auditory evoked cortical magnetic field (AECMF) M100… Expand
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Highly Cited
1989
Highly Cited
1989
The waveforms of the auditory evoked magnetic field in normal-hearing individuals and patients suffering from tinnitus are… Expand
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