Evidence for Late-stage Eruptive Mass-loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient

(2019)

Authors:

Anna YQ Ho, Daniel A Goldstein, Steve Schulze, David K Khatami, Daniel A Perley, Mattias Ergon, Avishay Gal-Yam, Alessandra Corsi, Igor Andreoni, Cristina Barbarino, Eric C Bellm, Nadia Blagorodnova, Joe S Bright, Eric Burns, S Bradley Cenko, Virginia Cunningham, Kishalay De, Richard Dekany, Alison Dugas, Rob P Fender, Claes Fransson, Christoffer Fremling, Adam Goldstein, Matthew J Graham, David Hale, Assaf Horesh, Tiara Hung, Mansi M Kasliwal, N Paul M Kuin, Shri R Kulkarni, Thomas Kupfer, Ragnhild Lunnan, Frank J Masci, Chow-Choong Ngeow, Peter E Nugent, Eran O Ofek, Maria T Patterson, Glen Petitpas, Ben Rusholme, Hanna Sai, Itai Sfaradi, David L Shupe, Jesper Sollerman, Maayane T Soumagnac, Yutaro Tachibana, Francesco Taddia, Richard Walters, Xiaofeng Wang, Yuhan Yao, Xinhan Zhang

The tidal disruption event AT2017eqx: spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow

(2019)

Authors:

M Nicholl, PK Blanchard, E Berger, S Gomez, R Margutti, KD Alexander, J Guillochon, J Leja, R Chornock, B Snios, K Auchettl, AG Bruce, P Challis, DJ D'Orazio, MR Drout, T Eftekhari, RJ Foley, O Graur, CD Kilpatrick, A Lawrence, AL Piro, C Rojas-Bravo, NP Ross, P Short, SJ Smartt, KW Smith, B Stalder

On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion

(2019)

Authors:

Lluís Galbany, Chris Ashall, Peter Hoeflich, Santiago González-Gaitán, Stefan Taubenberger, Maximilian Stritzinger, Eric Y Hsiao, Paolo Mazzali, Eddie Baron, Stéphane Blondin, Subhash Bose, Mattia Bulla, Jamison F Burke, Christopher R Burns, Régis Cartier, Ping Chen, Massimo Della Valle, Tiara R Diamond, Claudia P Gutiérrez, Jussi Harmanen, Daichi Hiramatsu, TW-S Holoien, Griffin Hosseinzadeh, D Andrew Howell, Yiwen Huang, Cosimo Inserra, Thomas de Jaeger, Saurabh W Jha, Tuomas Kangas, Markus Kromer, Joseph D Lyman, Kate Maguire, George Howie Marion, Dan Milisavljevic, Simon J Prentice, Alessandro Razza, Thomas M Reynolds, David J Sand, Benjamin J Shappee, Rohit Shekhar, Stephen J Smartt, Keivan G Stassun, Mark Sullivan, Stefano Valenti, Steven Villanueva, Xiaofeng Wang, J Craig Wheeler, Qian Zhai, Jujia Zhang

Search for invisible Higgs boson decays in vector boson fusion at root s=13 TeV with the ATLAS detector

Physics Letters B Elsevier 793 (2019) 499-519

Authors:

KJ Anderson, A Andreazza, V Andrei, CR Anelli, S Angelidakis, I Angelozzi, A Angerami, AV Anisenkov, A Annovi, C Antel, MT Anthony, M Antonelli, DJA Antrim, F Anulli, M Aoki, LA Bella, G Arabidze, JP Araque, V Araujo Ferraz, R Araujo Pereira, ATH Arce, RE Ardell, FA Arduh, J-F Arguin, S Argyropoulos

Abstract:

We report a search for Higgs bosons that are produced via vector boson fusion and subsequently decay into invisible particles. The experimental signature is an energetic jet pair with invariant mass of O(1)TeV and O(100)GeV missing transverse momentum. The analysis uses 36.1 fb −1 of pp collision data at s=13TeV recorded by the ATLAS detector at the LHC. In the signal region the 2252 observed events are consistent with the background estimation. Assuming a 125GeV scalar particle with Standard Model cross sections, the upper limit on the branching fraction of the Higgs boson decay into invisible particles is 0.37 at 95% confidence level where 0.28 was expected. This limit is interpreted in Higgs portal models to set bounds on the WIMP–nucleon scattering cross section. We also consider invisible decays of additional scalar bosons with masses up to 3TeV for which the upper limits on the cross section times branching fraction are in the range of 0.3–1.7pb.

A detailed radio study of the energetic, nearby, and puzzling GRB 171010A

Monthly Notices of the Royal Astronomical Society Oxford University Press 486:2 (2019) 2721-2729

Authors:

Joe Bright, A Horesh, Aj van der Horst, R Fender, Ge Anderson, Sara Motta, Sb Cenko, Da Green, Y Perrott, D Titterington

Abstract:

We present the results of an intensive multi-epoch radio frequency campaign on the energetic and nearby GRB 171010A with the Karl G. Janksy Very Large Array and Arcminute Microkelvin Imager Large Array. We began observing GRB 171010A a day after its initial detection, and were able to monitor the temporal and spectral evolution of the source over the following weeks. The spectra and their evolution are compared to the canonical theories for broad-band GRB afterglows, with which we find a general agreement. There are, however, a number of features that are challenging to explain with a simple forward shock model, and we discuss possible reasons for these discrepancies. This includes the consideration of the existence of a reverse shock component, potential microphysical parameter evolution, and the effect of scintillation.