Search Publications

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples
DOI: 10.1093/mnras/stu523 Bibcode: 2014MNRAS.441...24A

Petitjean, Patrick; Aubourg, Éric; Ross, Nicholas P. +62 more

We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey, which is part of the Sloan Digital Sky Survey III. Our results come from the Data Release 11 (DR11) sample, containing nearly one million ga…

2014 Monthly Notices of the Royal Astronomical Society
Planck 1374
New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star-forming dwarf galaxies
DOI: 10.1093/mnras/stu2029 Bibcode: 2014MNRAS.445.4287T

Slemer, Alessandra; Girardi, Léo; Marigo, Paola +4 more

We extend the PARSEC library of stellar evolutionary tracks by computing new models of massive stars, from 14 to 350 M. The input physics is the same used in the PARSEC V1.1 version, but for the mass-loss rate from considering the most recent updates in the literature. We focus on low metallicity, Z = 0.001 and Z = 0.004, for which the…

2014 Monthly Notices of the Royal Astronomical Society
eHST 416
Planets and stellar activity: hide and seek in the CoRoT-7 system
DOI: 10.1093/mnras/stu1320 Bibcode: 2014MNRAS.443.2517H

Deleuil, M.; Moutou, C.; Queloz, D. +12 more

Since the discovery of the transiting super-Earth CoRoT-7b, several investigations have yielded different results for the number and masses of planets present in the system, mainly owing to the star's high level of activity. We re-observed CoRoT-7 in 2012 January with both HARPS and CoRoT, so that we now have the benefit of simultaneous radial-vel…

2014 Monthly Notices of the Royal Astronomical Society
CoRoT 410
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: testing gravity with redshift space distortions using the power spectrum multipoles
DOI: 10.1093/mnras/stu1051 Bibcode: 2014MNRAS.443.1065B

Ross, Nicholas P.; Font-Ribera, Andreu; Ho, Shirley +15 more

We analyse the anisotropic clustering of the Baryon Oscillation Spectroscopic Survey (BOSS) CMASS Data Release 11 (DR11) sample, which consists of 690 827 galaxies in the redshift range 0.43 < z < 0.7 and has a sky coverage of 8498 deg2. We perform our analysis in Fourier space using a power spectrum estimator suggested by Yamamot…

2014 Monthly Notices of the Royal Astronomical Society
Planck 316
An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs
DOI: 10.1093/mnras/stt2273 Bibcode: 2014MNRAS.438.1267S

Thomson, A. P.; Ivison, R. J.; Smail, Ian +22 more

We exploit Atacama Large Millimeter Array (ALMA) 870 µm observations of sub-millimetre sources in the Extended Chandra Deep Field South to investigate the far-infrared properties of high-redshift sub-millimetre galaxies (SMGs). Using the precisely located 870 µm ALMA positions of 99 SMGs, together with 24µm and radio imaging, we …

2014 Monthly Notices of the Royal Astronomical Society
Herschel 312
The role of the reflection fraction in constraining black hole spin.
DOI: 10.1093/mnrasl/slu125 Bibcode: 2014MNRAS.444L.100D

Fabian, A. C.; Dauser, T.; Wilms, J. +2 more

In many active galaxies, the X-ray reflection features from the innermost regions of the accretion disc are relativistically distorted. This distortion allows us to measure parameters of the black hole such as its spin. The ratio in flux between the direct and the reflected radiation, the so-called reflection fraction, is determined directly from …

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 303
On the age of the β Pictoris moving group
DOI: 10.1093/mnras/stu1894 Bibcode: 2014MNRAS.445.2169M

Mamajek, Eric E.; Bell, Cameron P. M.

Binks & Jeffries and Malo et al. have recently reported Li depletion boundary (LDB) ages for the β Pictoris moving group (BPMG) which are twice as old as the oft-cited kinematic age of ∼12 Myr. In this study, we present (1) a new evaluation of the internal kinematics of the BPMG using the revised Hipparcos astrometry and best available publish…

2014 Monthly Notices of the Royal Astronomical Society
Hipparcos 280
The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field
DOI: 10.1093/mnras/stu1622 Bibcode: 2014MNRAS.444.2960D

Dickinson, M.; Ferguson, H. C.; Giavalisco, M. +16 more

We measure new estimates for the galaxy stellar mass function and star formation rates for samples of galaxies at z ∼ 4, 5, 6 and 7 using data in the CANDELS GOODS South field. The deep near-infrared observations allow us to construct the stellar mass function at z ≥ 6 directly for the first time. We estimate stellar masses for our sample by fitti…

2014 Monthly Notices of the Royal Astronomical Society
eHST 273
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring growth rate and geometry with anisotropic clustering
DOI: 10.1093/mnras/stu197 Bibcode: 2014MNRAS.439.3504S

Aubourg, Éric; Ross, Nicholas P.; Streblyanska, Alina +27 more

We use the observed anisotropic clustering of galaxies in the Baryon Oscillation Spectroscopic Survey Data Release 11 CMASS sample to measure the linear growth rate of structure, the Hubble expansion rate and the comoving distance scale. Our sample covers 8498 deg2 and encloses an effective volume of 6 Gpc3 at an effective re…

2014 Monthly Notices of the Royal Astronomical Society
Planck 271
The incidence of obscuration in active galactic nuclei
DOI: 10.1093/mnras/stt2149 Bibcode: 2014MNRAS.437.3550M

Berta, S.; Magnelli, B.; Lutz, D. +22 more

We study the incidence of nuclear obscuration on a complete sample of 1310 active galactic nuclei (AGN) selected on the basis of their rest-frame 2-10 keV X-ray flux from the XMM-COSMOS survey, in the redshift range 0.3 < z < 3.5. We classify the AGN as obscured or unobscured on the basis of either the optical spectral properties and the ove…

2014 Monthly Notices of the Royal Astronomical Society
Herschel XMM-Newton 245