Search Publications

Scaling relations for galaxy clusters in the Millennium-XXL simulation
DOI: 10.1111/j.1365-2966.2012.21830.x Bibcode: 2012MNRAS.426.2046A

White, S. D. M.; Baugh, C. M.; Frenk, C. S. +3 more

We present a very large high-resolution cosmological N-body simulation, the Millennium-XXL or MXXL, which uses 303 billion particles to represent the formation of dark matter structures throughout a 4.1 Gpc box in a Λ cold dark matter cosmology. We create sky maps and identify large samples of galaxy clusters using surrogates for four different ob…

2012 Monthly Notices of the Royal Astronomical Society
Planck 473
A simplified view of blazars: clearing the fog around long-standing selection effects
DOI: 10.1111/j.1365-2966.2011.20044.x Bibcode: 2012MNRAS.420.2899G

D'Elia, V.; Polenta, G.; Giommi, P. +3 more

We propose a scenario where blazars are classified into flat-spectrum radio quasars (FSRQs), BL Lacertae (BL Lac) objects, low-synchrotron, or high-synchrotron peaked objects according to a varying mix of the Doppler-boosted radiation from the jet, the emission from the accretion disc, the broad-line region, and the light from the host galaxy. In …

2012 Monthly Notices of the Royal Astronomical Society
Planck 259
The Canadian Cluster Comparison Project: weak lensing masses and SZ scaling relations
DOI: 10.1111/j.1365-2966.2012.22072.x Bibcode: 2012MNRAS.427.1298H

Hoekstra, Henk; Babul, Arif; Mahdavi, Andisheh +1 more

The Canadian Cluster Comparison Project is a comprehensive multi-wavelength survey targeting 50 massive X-ray selected clusters of galaxies to examine baryonic tracers of cluster mass and to probe the cluster-to-cluster variation in the thermal properties of the hot intra-cluster medium. In this paper we present the weak lensing masses, based on t…

2012 Monthly Notices of the Royal Astronomical Society
Planck 133
Improved models for cosmic infrared background anisotropies: new constraints on the infrared galaxy population
DOI: 10.1111/j.1365-2966.2012.20510.x Bibcode: 2012MNRAS.421.2832S

Knox, Lloyd; Oh, S. Peng; Shang, Cien +1 more

The power spectrum of cosmic infrared background (CIB) anisotropies is sensitive to the connection between star formation and dark matter haloes over the entire cosmic star formation history. Here we develop a model that associates star-forming galaxies with dark matter haloes and their subhaloes. The model is based on a parametrized relation betw…

2012 Monthly Notices of the Royal Astronomical Society
Planck 87
Sunyaev-Zel'dovich clusters in Millennium gas simulations
DOI: 10.1111/j.1365-2966.2012.20623.x Bibcode: 2012MNRAS.422.1999K

Thomas, Peter A.; Kay, Scott T.; Liddle, Andrew R. +5 more

Large surveys using the Sunyaev-Zel'dovich (SZ) effect to find clusters of galaxies are now starting to yield large numbers of systems out to high redshift, many of which are new discoveries. In order to provide theoretical interpretation for the release of the full SZ cluster samples over the next few years, we have exploited the large-volume Mil…

2012 Monthly Notices of the Royal Astronomical Society
Planck 81
Optical flux and spectral variability of blazars
DOI: 10.1111/j.1365-2966.2012.21583.x Bibcode: 2012MNRAS.425.3002G

Gupta, Alok C.; Wiita, Paul J.; Bachev, R. +9 more

We report the results of optical monitoring for a sample of 11 blazars including 10 BL Lacertae objects (BL Lacs) and one flat spectrum radio quasar (FSRQ). We have measured the multiband optical flux and colour variations in these blazars on intraday and short-term time-scales of months and have limited data for two more blazars. These photometri…

2012 Monthly Notices of the Royal Astronomical Society
Planck 73
A Sunyaev-Zel'dovich take on cluster radio haloes - I. Global scaling and bi-modality using Planck data
DOI: 10.1111/j.1745-3933.2012.01217.x Bibcode: 2012MNRAS.421L.112B

Basu, Kaustuv

Giant radio haloes in galaxy clusters are the primary evidence for the existence of relativistic particles (cosmic rays) and magnetic fields over Mpc scales. Observational tests for the different theoretical models explaining their powering mechanism have so far been obtained through X-ray selection of clusters, e.g. by comparing cluster X-ray lum…

2012 Monthly Notices of the Royal Astronomical Society
Planck 73
The dust energy balance in the edge-on spiral galaxy NGC 4565
DOI: 10.1111/j.1365-2966.2012.22045.x Bibcode: 2012MNRAS.427.2797D

Gordon, Karl D.; De Looze, Ilse; Baes, Maarten +20 more

We combine new dust continuum observations of the edge-on spiral galaxy NGC 4565 in all Herschel/Spectral and Photometric Imaging Receiver (250, 350 and 500 µm) wavebands, obtained as part of the Herschel Reference Survey, and a large set of ancillary data (Spitzer, Sloan Digital Sky Survey, Galaxy Evolution Explorer) to analyse its dust ene…

2012 Monthly Notices of the Royal Astronomical Society
Herschel Planck 67
Galaxy cluster outskirts: a universal entropy profile for relaxed clusters?
DOI: 10.1111/j.1745-3933.2012.01342.x Bibcode: 2012MNRAS.427L..45W

Fabian, A. C.; Sanders, J. S.; Walker, S. A. +1 more

We fit a functional form for a universal intracluster medium entropy profile to the scaled entropy profiles of a catalogue of X-ray galaxy cluster outskirts results, which are all relaxed cool core clusters at redshift below 0.25. We also investigate the functional form suggested by Lapi et al. and Cavaliere et al. for the behaviour of the entropy…

2012 Monthly Notices of the Royal Astronomical Society
Planck Suzaku 51
Clustering of submillimetre galaxies in a self-regulated baryon collapse model
DOI: 10.1111/j.1365-2966.2012.20705.x Bibcode: 2012MNRAS.422.1324X

Danese, L.; Negrello, M.; Lapi, A. +3 more

We investigate anisotropies in the cosmic infrared background (CIB) using a combination of the physical evolutionary model for proto-spheroid galaxies of Granato et al. and an independent halo occupation distribution analysis. After having re-calibrated the cumulative flux function dS/dz at ?m using the available determinations of the shot-noise a…

2012 Monthly Notices of the Royal Astronomical Society
Planck 49