Search Publications

Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z ≃ 0.1
DOI: 10.1111/j.1365-2966.2011.18842.x Bibcode: 2011MNRAS.415.2215B

Treu, Tommaso; Czoske, Oliver; Koopmans, Léon V. E. +2 more

We combine in a self-consistent way the constraints from both gravitational lensing and stellar kinematics to perform a detailed investigation of the internal mass distribution, amount of dark matter, and dynamical structure of the 16 early-type lens galaxies from the SLACS Survey, at z = 0.08 - 0.33, for which both HST/ACS and NICMOS high-resolut…

2011 Monthly Notices of the Royal Astronomical Society
eHST 224
Discovery of the nearby long, soft GRB 100316D with an associated supernova
DOI: 10.1111/j.1365-2966.2010.17879.x Bibcode: 2011MNRAS.411.2792S

Sakamoto, T.; Covino, S.; D'Avanzo, P. +43 more

We report the Swift discovery of the nearby long, soft gamma-ray burst GRB 100316D, and the subsequent unveiling of its low-redshift host galaxy and associated supernova. We derive the redshift of the event to be z= 0.0591 ± 0.0001 and provide accurate astrometry for the gamma-ray burst (GRB) supernova (SN). We study the extremely unusual prompt e…

2011 Monthly Notices of the Royal Astronomical Society
eHST 200
A robust sample of galaxies at redshifts 6.0<z<8.7: stellar populations, star formation rates and stellar masses
DOI: 10.1111/j.1365-2966.2011.19626.x Bibcode: 2011MNRAS.418.2074M

Bowler, R. A. A.; McLure, R. J.; Dunlop, J. S. +7 more

We present the results of a photometric redshift analysis designed to identify z≥ 6 galaxies from the near-infrared Hubble Space Telescope imaging in three deep fields [Hubble Ultra Deep Field (HUDF), HUDF09-2 and Early Release Science] covering a total area of 45 square arcmin. By adopting a rigorous set of criteria for rejecting low-redshift int…

2011 Monthly Notices of the Royal Astronomical Society
eHST 200
The causal connection between disc and power-law variability in hard state black hole X-ray binaries
DOI: 10.1111/j.1745-3933.2011.01056.x Bibcode: 2011MNRAS.414L..60U

Wilms, J.; Uttley, P.; Pottschmidt, K. +4 more

We use the XMM-Newton EPIC-pn instrument in timing mode to extend spectral time-lag studies of hard state black hole X-ray binaries into the soft X-ray band. We show that variations of the disc blackbody emission substantially lead variations in the power-law emission, by tenths of a second on variability time-scales of seconds or longer. The larg…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 193
Dynamical masses of early-type galaxies: a comparison to lensing results and implications for the stellar initial mass function and the distribution of dark matter
DOI: 10.1111/j.1365-2966.2011.18725.x Bibcode: 2011MNRAS.415..545T

Saglia, R. P.; Thomas, D.; Thomas, J. +6 more

This work aims to study the distribution of the luminous and dark matter in Coma early-type galaxies. Dynamical masses obtained under the assumption that mass follows light do not match with the masses of strong gravitational lens systems of similar velocity dispersions. Instead, dynamical fits with dark matter haloes are in good agreement with le…

2011 Monthly Notices of the Royal Astronomical Society
eHST 175
Families of dynamically hot stellar systems over 10 orders of magnitude in mass
DOI: 10.1111/j.1365-2966.2011.18669.x Bibcode: 2011MNRAS.414.3699M

Hilker, M.; Misgeld, I.

Dynamically hot stellar systems, whether star clusters or early-type galaxies, follow well-defined scaling relations over many orders of magnitudes in mass. These Fundamental Plane relations have been subject of several studies, which have been mostly confined to certain types of galaxies and/or star clusters so far. Here, we present a complete pi…

2011 Monthly Notices of the Royal Astronomical Society
eHST 171
The dependence of star formation activity on environment and stellar mass at z∼ 1 from the HiZELS-Hα survey
DOI: 10.1111/j.1365-2966.2010.17707.x Bibcode: 2011MNRAS.411..675S

Smail, Ian; Sobral, David; Geach, James E. +4 more

This paper presents an environment and stellar mass study of a large sample of star-forming Hα emitters at z= 0.84 from the High-z Emission Line Survey (HiZELS), over 1.3 deg2 split over two fields (COSMOS and UKIDSS UDS). By taking advantage of a truly panoramic coverage of a wide range of environments, from the field to a rich cluster…

2011 Monthly Notices of the Royal Astronomical Society
eHST 170
Dissecting the size evolution of elliptical galaxies since z∼ 1: puffing-up versus minor-merging scenarios
DOI: 10.1111/j.1365-2966.2011.19017.x Bibcode: 2011MNRAS.415.3903T

Trujillo, Ignacio; Ferreras, Ignacio; de La Rosa, Ignacio G.

At a fixed stellar mass, the size of low-redshift early-type galaxies is found to be a factor of 2 larger than that of their counterparts at z∼ 1, a result with important implications for galaxy formation models. In this paper, we have explored the buildup of the local mass-size relation of elliptical galaxies using two visually classified samples…

2011 Monthly Notices of the Royal Astronomical Society
eHST 169
On the evolution of the velocity-mass-size relations of disc-dominated galaxies over the past 10 billion years
DOI: 10.1111/j.1365-2966.2010.17555.x Bibcode: 2011MNRAS.410.1660D

Koekemoer, Anton M.; Weiner, Benjamin J.; van den Bosch, Frank C. +10 more

We study the evolution of the scaling relations between the maximum circular velocity, stellar mass and optical half-light radius of star-forming disc-dominated galaxies in the context of Λ cold dark matter-based galaxy formation models. Using data from the literature combined with new data from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) …

2011 Monthly Notices of the Royal Astronomical Society
eHST 165
Anisotropy of Alfvénic turbulence in the solar wind and numerical simulations
DOI: 10.1111/j.1365-2966.2011.18933.x Bibcode: 2011MNRAS.415.3219C

Horbury, T. S.; Chen, C. H. K.; Mallet, A. +2 more

We investigate the anisotropy of Alfvénic turbulence in the inertial range of slow solar wind and in both driven and decaying reduced magnetohydrodynamic simulations. A direct comparison is made by measuring the anisotropic second-order structure functions in both data sets. In the solar wind, the perpendicular spectral index of the magnetic field…

2011 Monthly Notices of the Royal Astronomical Society
Cluster 148