works on

From the 1 of 8.2k papers with an AI index.

output
19912026
Showing 2012Show all

249 papers · 1 filter

astro-ph.CO2012★ 9 cited

Large Size Scatter of Passively Evolving Lensed Galaxies at z~2 in CLASH

Lulu Fan, Yang Chen, Xinzhong Er +3

In a systematic search over 11 cluster fields from Cluster Lensing And Supernova survey with Hubble (CLASH) we identify ten passively evolving massive galaxies at redshift z~2.We d…

hep-ph2012★ 38 cited

The little hierarchy problem for new physics just beyond the LHC

F. Bazzocchi, M. Fabbrichesi

We discuss two possible extensions to the standard model in which an inert singlet scalar state that only interacts with the Higgs boson is added together with some fermions. In on…

hep-th2012★ 15 cited

Horava-Lifshitz gravity with detailed balance

Daniele Vernieri, Thomas P. Sotiriou

Horava-Lifshitz gravity with "detailed balance" but without the projectability assumption is discussed. It is shown that detailed balance is quite efficient in limiting the prolife…

q-bio.BM2012★ 79 cited

Comparing proteins by their internal dynamics: exploring structure-function relationships beyond static structural alignments

C. Micheletti

The growing interest for comparing protein internal dynamics owes much to the realization that protein function can be accompanied or assisted by structural fluctuations and confor…

astro-ph.CO2012★ 98 cited

Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies

Planck Collaboration, P. A. R. Ade, N. Aghanim +194

We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Surv…

astro-ph.CO2012★ 11 cited

The Planck Sunyaev-Zel'dovich vs. the X-ray View of the Coma Cluster

R. Fusco-Femiano, A. Lapi, A. Cavaliere

The Planck collaboration has recently published precise and resolved measurements of the Sunyaev-Zel'dovich effect in Abell 1656 (the Coma cluster of galaxies), so directly gauging…