Oxford SWIFT integral field spectrograph and multiwavelength observations of the Eagle galaxy at z= 0.77
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 417:4 (2011) 2882-2890
The X-Shooter Lens Survey – I. Dark matter domination and a Salpeter-type initial mass function in a massive early-type galaxy
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 417:4 (2011) 3000-3009
Search for new physics with a monojet and missing transverse energy in pp collisions at √s=7TeV
Physical Review Letters 107:20 (2011)
Abstract:
A study of events with missing transverse energy and an energetic jet is performed using pp collision data at a center-of-mass energy of 7 TeV. The data were collected by the CMS detector at the LHC, and correspond to an integrated luminosity of 36pb-1. An excess of these events over standard model contributions is a signature of new physics such as large extra dimensions and unparticles. The number of observed events is in good agreement with the prediction of the standard model, and significant extension of the current limits on parameters of new physics benchmark models is achieved. © 2011 CERN.Galaxy Zoo: building the low-mass end of the red sequence with local post-starburst galaxies
ArXiv 1111.1785 (2011)
Abstract:
We present a study of local post-starburst galaxies (PSGs) using the photometric and spectroscopic observations from the Sloan Digital Sky Survey (SDSS) and the results from the Galaxy Zoo project. We find that the majority of our local PSG population have neither early- nor late- type morphologies but occupy a well-defined space within the colour-stellar mass diagram, most notably, the low-mass end of the "green valley" below the transition mass thought to be the mass division between low-mass star-forming galaxies and high-mass passively-evolving bulge-dominated galaxies. Our analysis suggests that it is likely that a local PSG will quickly transform into "red", low-mass early-type galaxies as the stellar morphologies of the "green" PSGs largely resemble that of the early-type galaxies within the same mass range. We propose that the current population of PSGs represents a population of galaxies which is rapidly transitioning between the star-forming and the passively-evolving phases. Subsequently, these PSGs will contribute towards the build-up of the low-mass end of the "red sequence" once the current population of young stars fade and stars are no longer being formed. These results are consistent with the idea of "downsizing" where the build-up of smaller galaxies occurs at later epochs.Observation of the baryonic flavor-changing neutral current decay Λb0→Λμ+μ-
Physical Review Letters 107:20 (2011)