output
20032015
most citedAn eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent

691 citations

Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2015

CLASH-VLT: Substructure in the galaxy cluster MACS J1206.2-0847 from kinematics of galaxy populations

M. Girardi, A. Mercurio, I. Balestra +35

In the effort to understand the link between the structure of galaxy clusters and their galaxy populations, we focus on MACSJ1206.2-0847 at z~0.44 and probe its substructure in the…

astro-ph.CO20131 cited

Active Galactic Nuclei - the Physics of Individual Sources and the Cosmic History of Formation and Evolution

Henric Krawczynski, Ezequiel Treister

In this paper we give a brief review of the astrophysics of active galactic nuclei (AGN). After a general introduction motivating the study of AGNs, we discuss our present understa…

astro-ph.CO201298 cited

Second Season QUIET Observations: Measurements of the CMB Polarization Power Spectrum at 95 GHz

QUIET Collaboration, D. Araujo, C. Bischoff +48

The Q/U Imaging ExperimenT (QUIET) has observed the cosmic microwave background (CMB) at 43 and 95GHz. The 43-GHz results have been published in QUIET Collaboration et al. (2011),…

astro-ph.CO2011

Radio-Quiet AGN and the Transient Radio Sky

C. G. Mundell, N. Nagar, P. Ferruit

8.4-GHZ radio imaging study of an optically selected sample of early type Seyfert galaxies; comparison of images taken at two epochs reveals possible variation in the nuclear radio…

astro-ph.CO20119 cited

Constraints from CMB in the intermediate Brans-Dicke inflation

Antonella Cid, Sergio del Campo

We study an intermediate inflationary stage in a Jordan-Brans-Dicke theory. In this scenario we analyze the quantum fluctuations corresponding to adiabatic and isocurvature modes.…

astro-ph.CO201081 cited

How effective is harassment on infalling late-type dwarfs?

R. Smith, J. I. Davies, A. H. Nelson

A new harassment model is presented that models the complex, and dynamical tidal field of a Virgo like galaxy cluster. The model is applied to small, late-type dwarf disc galaxies…