Search Publications

Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys
DOI: 10.1093/mnras/stu949 Bibcode: 2014MNRAS.442.1507G

Gruen, D.; Bender, R.; Seitz, S. +8 more

We present the weak lensing analysis of the Wide-Field Imager Sunyaev-Zel'dovich Cluster of Galaxy (WISCy) sample, a set of 12 clusters of galaxies selected for their Sunyaev-Zel'dovich (SZ) effect. After developing new and improved methods for background selection and determination of geometric lensing scaling factors from absolute multiband phot…

2014 Monthly Notices of the Royal Astronomical Society
Planck 106
An X-ray survey of the 2 Jy sample - I. Is there an accretion mode dichotomy in radio-loud AGN?
DOI: 10.1093/mnras/stu263 Bibcode: 2014MNRAS.440..269M

Hardcastle, M. J.; Croston, J. H.; Morganti, R. +4 more

We carry out a systematic study of the X-ray emission from the active nuclei of the 0.02 < z < 0.7 2 Jy sample, using Chandra and XMM-Newton observations. We combine our results with those from mid-infrared, optical emission-line and radio observations, and add them to those of the 3CRR sources. We show that the low-excitation objects in our…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 105
The dust budget crisis in high-redshift submillimetre galaxies
DOI: 10.1093/mnras/stu605 Bibcode: 2014MNRAS.441.1040R

Aragón-Salamanca, A.; Dunne, L.; Dye, S. +5 more

We apply a chemical evolution model to investigate the sources and evolution of dust in a sample of 26 high-redshift (z > 1) submillimetre galaxies (SMGs) from the literature, with complete photometry from ultraviolet to the submillimetre. We show that dust produced only by low-intermediate-mass stars falls a factor 240 short of the observed du…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 105
Verifying the mass-metallicity relation in damped Lyman α selected galaxies at 0.1 < z < 3.2
DOI: 10.1093/mnras/stu1726 Bibcode: 2014MNRAS.445..225C

Fynbo, J. P. U.; Christensen, L.; Møller, P. +1 more

A scaling relation has recently been suggested to combine the galaxy mass-metallicity (MZ) relation with metallicities of damped Lyman α systems (DLAs) in quasar spectra. Based on this relation the stellar masses of the absorbing galaxies can be predicted. We test this prediction by measuring the stellar masses of 12 galaxies in confirmed DLA abso…

2014 Monthly Notices of the Royal Astronomical Society
eHST 104
PACS photometry of the Herschel Reference Survey - far-infrared/submillimetre colours as tracers of dust properties in nearby galaxies
DOI: 10.1093/mnras/stu175 Bibcode: 2014MNRAS.440..942C

Ciesla, L.; Buat, V.; Boquien, M. +26 more

We present Herschel/PACS 100 and 160 µm integrated photometry for the 323 galaxies in the Herschel Reference Survey (HRS), a K-band, volume-limited sample of galaxies in the local Universe. Once combined with the Herschel/SPIRE observations already available, these data make the HRS the largest representative sample of nearby galaxies with h…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 102
The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years
DOI: 10.1093/mnras/stt1897 Bibcode: 2014MNRAS.437..437A

Weiner, Benjamin J.; Moustakas, John; Dey, Arjun +14 more

We compare the star formation (SF) activity in cluster galaxies to the field from z = 0.3 to 1.5 using Herschel Spectral and Photometric Imaging REceiver 250 µm imaging and utilizing 274 clusters from the IRAC Shallow Cluster Survey (ISCS). These clusters were selected as rest-frame near-infrared overdensities over the 9 square degree Boötes…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 102
A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles
DOI: 10.1093/mnras/stt2349 Bibcode: 2014MNRAS.438.2341P

Fabian, A. C.; Sanders, J. S.; Panagoulia, E. K.

We present the first results of our study of a sample of 101 X-ray galaxy groups and clusters, which is volume-limited in each of three X-ray luminosity bins. The aim of this work is to study the properties of the innermost ICM in the cores of our groups and clusters, and to determine the effect of non-gravitational processes, such as active galac…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 101
The mass-metallicity-star formation rate relation at z ≳ 2 with 3D Hubble Space Telescope
DOI: 10.1093/mnras/stu443 Bibcode: 2014MNRAS.440.2300C

Bowler, R. A. A.; Cullen, F.; McLure, R. J. +2 more

We present new accurate measurements of the mass, metallicity and star-formation rate of a statistically significant sample of 93 galaxies at z ≳ 2 using near-infrared spectroscopy taken as part of the 3D-Hubble Space Telescope survey. We derive a mass-metallicity relation (MZR) for our sample with metallicities based on the oxygen and Hβ nebular …

2014 Monthly Notices of the Royal Astronomical Society
eHST 101
zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ∼ 0.7
DOI: 10.1093/mnras/stt2241 Bibcode: 2014MNRAS.438..717K

Kneib, J. -P.; Aussel, H.; Le Floc'h, E. +41 more

We explore the role of environment in the evolution of galaxies over 0.1 < z < 0.7 using the final zCOSMOS-bright data set. Using the red fraction of galaxies as a proxy for the quenched population, we find that the fraction of red galaxies increases with the environmental overdensity δ and with the stellar mass M*, consistent wit…

2014 Monthly Notices of the Royal Astronomical Society
eHST 100
On the determination of the spin and disc truncation of accreting black holes using X-ray reflection
DOI: 10.1093/mnras/stu045 Bibcode: 2014MNRAS.439.2307F

Fabian, A. C.; Miller, J. M.; Reynolds, C. S. +4 more

We discuss the application of simple relativistically blurred X-ray reflection models to the determination of the spin and the inner radius of the disc in accreting black holes. Observationally, the nature of the corona is uncertain a priori, but a robust determination of the inner disc radius can be made when the disc emissivity index is tightly …

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 99