The Feasibility of Magnetic Reconnection Powered Blazar Flares from Synchrotron Self-Compton Emission

(2018)

Authors:

Paul J Morris, William J Potter, Garret Cotter

A NICER Discovery of a Low-frequency Quasi-periodic Oscillation in the Soft-intermediate State of MAXI J1535-571

ASTROPHYSICAL JOURNAL LETTERS 865:2 (2018) ARTN L15

Authors:

AL Stevens, P Uttley, D Altamirano, Z Arzoumanian, P Bult, EM Cackett, AC Fabian, KC Gendreau, KQ Ha, J Homan, AR Ingram, E Kara, J Kellogg, RM Ludlam, JM Miller, J Neilsen, DR Pasham, RA Remillard, JF Steiner, J van den Eijnden

Characterisation and testing of CHEC-M—A camera prototype for the small-sized telescopes of the Cherenkov telescope array

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 904 (2018) 44-63

Authors:

J Zorn, R White, JJ Watson, TP Armstrong, A Balzer, M Barcelo, D Berge, R Bose, AM Brown, M Bryan, PM Chadwick, P Clark, H Costantini, G Cotter, L Dangeon, M Daniel, A De Franco, P Deiml, G Fasola, S Funk, M Gebyehu, J Gironnet, JA Graham, T Greenshaw, JA Hinton, M Kraus, JS Lapington, P Laporte, SA Leach, O Le Blanc, A Malouf, P Molyneux, P Moore, H Prokoph, A Okumura, D Ross, G Rowell, L Sapozhnikov, H Schoorlemmer, H Sol, M Stephan, H Tajima, L Tibaldo, G Varner, A Zink

Abstract:

© 2018 Elsevier B.V. The Compact High Energy Camera (CHEC) is a camera design for the Small-Sized Telescopes (SSTs; 4 m diameter mirror) of the Cherenkov Telescope Array (CTA). The SSTs are focused on very-high-energy γ-ray detection via atmospheric Cherenkov light detection over a very large area. This implies many individual units and hence cost-effective implementation, as well as shower detection at large impact distance, and hence large field of view (FoV), and efficient image capture in the presence of large time gradients in the shower image detected by the camera. CHEC relies on dual-mirror optics to reduce the plate-scale and make use of 6 × 6 mm2pixels, leading to a low-cost (∼150 k€), compact (0.5 m × 0.5 m), and light (∼45 kg) camera with 2048 pixels providing a camera FoV of ∼9 degrees. The CHEC electronics are based on custom TARGET (TeV array readout with GSa/s sampling and event trigger) application-specific integrated circuits (ASICs) and field programmable gate arrays (FPGAs) sampling incoming signals at a gigasample per second, with flexible camera-level triggering within a single backplane FPGA. CHEC is designed to observe in the γ-ray energy range of 1–300 TeV, and at impact distances up to ∼500 m. To accommodate this and provide full flexibility for later data analysis, full waveforms with 96 samples for all 2048 pixels can be read out at rates up to ∼900 Hz. The first prototype, CHEC-M, based on multi-anode photomultipliers (MAPMs) as photosensors, was commissioned and characterised in the laboratory and during two measurement campaigns on a telescope structure at the Paris Observatory in Meudon. In this paper, the results and conclusions from the laboratory and on-site testing of CHEC-M are presented. They have provided essential input on the system design and on operational and data analysis procedures for a camera of this type. A second full-camera prototype based on Silicon photomultipliers (SiPMs), addressing the drawbacks of CHEC-M identified during the first prototype phase, has already been built and is currently being commissioned and tested in the laboratory.

Discovery of X-Rays from the Old and Faint Pulsar J1154–6250

The Astrophysical Journal American Astronomical Society 865:2 (2018) 116

Authors:

Andrei P Igoshev, Sergey S Tsygankov, Michela Rigoselli, Sandro Mereghetti, Sergei B Popov, Justin G Elfritz, Alexander A Mushtukov

Testing the magnetar scenario for superluminous supernovae with circular polarimetry

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 479:4 (2018) 4984-4990

Authors:

Aleksandar Cikota, Giorgos Leloudas, Mattia Bulla, Cosimo Inserra, Ting-Wan Chen, Jason Spyromilio, Ferdinando Patat, Zach Cano, Stefan Cikota, Michael W Coughlin, Erkki Kankare, Thomas B Lowe, Justyn R Maund, Armin Rest, Stephen J Smartt, Ken W Smith, Richard J Wainscoat, David R Young