Measurements of electroweak Wjj production and constraints on anomalous gauge couplings with the ATLAS detector

European Journal of Physics Springer Berlin Heidelberg 77:7 (2017) 474

Authors:

M Aaboud, G Aad, B Abbott, Giacomo Artoni, Moritz Backes, Alan J Barr, Kathrin Becker, Lydia A Beresford, Daniela Bortoletto, Jonathan TP Burr, Amanda M Cooper-Sarkar, William J Fawcett, James A Frost, Elizabeth J Gallas, Francesco Giuli, Claire Gwenlan, Christopher Hays, B Todd Huffman, Cigdem Issever, Koichi Nagai, Richard B Nickerson, Nurfikri Norjoharuddeen, Mariyan Petrov, Mark A Pickering, Jeffrey C-L Tseng, Georg HA Viehhauser, Luigi Vigani, Anthony R Weidberg, Et Et al.

Abstract:

Measurements of the electroweak production of a W boson in association with two jets at high dijet invariant mass are performed using √s = 7 and 8 TeV proton–proton collision data produced by the Large Hadron Collider, corresponding respectively to 4.7 and 20.2 fb−1 of integrated luminosity collected by the ATLAS detector. The measurements are sensitive to the production of a W boson via a triple-gauge-boson vertex and include both the fiducial and differential cross sections of the electroweak process.

LSQ14efd: observations of the cooling of a shock break-out event in a type Ic Supernova

(2017)

Authors:

C Barbarino, MT Botticella, M Dall'Ora, M Della Valle, S Benetti, JD Lyman, SJ Smartt, I Arcavi, C Baltay, D Bersier, M Dennefeld, N Ellman, M Fraser, A Gal-Yam, G Hosseinzadeh, DA Howell, C Inserra, E Kankare, G Leloudas, K Maguire, C McCully, A Mitra, R McKinnon, F Olivares E., G Pignata, D Rabinowitz, S Rostami, KW Smith, M Sullivan, S Valenti, O Yaron, D Young

On the use of variability time-scales as an early classifier of radio transients and variables

Monthly Notices of the Royal Astronomical Society Oxford University Press 471:4 (2017) 3788-3805

Authors:

Malgorzata Pietka, Timothy Staley, ML Pretorius, Robert Fender

Abstract:

We have shown previously that a broad correlation between the peak radio luminosity and the variability time-scales, approximately L ∝ τ5, exists for variable synchrotron emitting sources and that different classes of astrophysical sources occupy different regions of luminosity and time-scale space. Based on those results, we investigate whether the most basic information available for a newly discovered radio variable or transient – their rise and/or decline rate – can be used to set initial constraints on the class of events from which they originate. We have analysed a sample of ≈800 synchrotron flares, selected from light curves of ≈90 sources observed at 5–8 GHz, representing a wide range of astrophysical phenomena, from flare stars to supermassive black holes. Selection of outbursts from the noisy radio light curves has been done automatically in order to ensure reproducibility of results. The distribution of rise/decline rates for the selected flares is modelled as a Gaussian probability distribution for each class of object, and further convolved with estimated areal density of that class in order to correct for the strong bias in our sample. We show in this way that comparing the measured variability time-scale of a radio transient/variable of unknown origin can provide an early, albeit approximate, classification of the object, and could form part of a suite of measurements used to provide early categorization of such events. Finally, we also discuss the effect scintillating sources will have on our ability to classify events based on their variability time-scales.

On the use of variability time-scales as an early classifier of radio transients and variables

(2017)

Authors:

M Pietka, TD Staley, ML Pretorius, RP Fender

Complexity in the light curves and spectra of slow-evolving superluminous supernovae

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 468:4 (2017) 4642-4662

Authors:

C Inserra, M Nicholl, T-W Chen, A Jerkstrand, SJ Smartt, T Krühler, JP Anderson, C Baltay, M Della Valle, M Fraser, A Gal-Yam, L Galbany, E Kankare, K Maguire, D Rabinowitz, K Smith, S Valenti, DR Young