The Square Kilometre Array (SKA): publications

FRB 20121102A: images of the bursts and the varying radio counterpart

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 525:3 (2023) 3626-3632

Authors:

L Rhodes, M Caleb, BW Stappers, A Andersson, MC Bezuidenhout, LN Driessen, I Heywood

Multiwavelength Observations of the Blazar PKS 0735+178 in Spatial and Temporal Coincidence with an Astrophysical Neutrino Candidate IceCube-211208A

The Astrophysical Journal American Astronomical Society 954:1 (2023) 70

Authors:

A Acharyya, CB Adams, A Archer, P Bangale, JT Bartkoske, P Batista, W Benbow, A Brill, JH Buckley, JL Christiansen, AJ Chromey, M Errando, A Falcone, Q Feng, GM Foote, L Fortson, A Furniss, G Gallagher, W Hanlon, D Hanna, O Hervet, CE Hinrichs, J Hoang, J Holder, TB Humensky, W Jin, P Kaaret, M Kertzman, M Kherlakian, D Kieda, TK Kleiner, N Korzoun, S Kumar, MJ Lang, M Lundy, G Maier, CE McGrath, MJ Millard, J Millis, CL Mooney, P Moriarty, R Mukherjee, S O’Brien, RA Ong, M Pohl, E Pueschel, J Quinn, K Ragan, PT Reynolds, D Ribeiro, E Roache, I Sadeh, AC Sadun, L Saha, M Santander, GH Sembroski, R Shang, M Splettstoesser, A Kaushik Talluri, JV Tucci, VV Vassiliev, A Weinstein, DA Williams, SL Wong, J Woo, The VERITAS Collaboration, F Aharonian, J Aschersleben, M Backes, V Barbosa Martins, R Batzofin, Y Becherini, D Berge, K Bernlöhr, B Bi, M Böttcher, C Boisson, J Bolmont, M de Bony de Lavergne, J Borowska, M Bouyahiaoui, F Bradascio, M Breuhaus, R Brose, F Brun, B Bruno, T Bulik, C Burger-Scheidlin, S Caroff, S Casanova, R Cecil, J Celic, M Cerruti, T Chand, S Chandra, A Chen, J Chibueze, O Chibueze, G Cotter, S Dai, J Damascene Mbarubucyeye, A Djannati-Ataï, A Dmytriiev, V Doroshenko, S Einecke, J-P Ernenwein, G Fichet de Clairfontaine, M Filipovic, G Fontaine, M Füßling, S Funk, S Gabici, S Ghafourizadeh, G Giavitto, D Glawion, JF Glicenstein, P Goswami, G Grolleron, L Haerer, JA Hinton, TL Holch, M Holler, D Horns, M Jamrozy, F Jankowsky, V Joshi, I Jung-Richardt, E Kasai, K Katarzyński, R Khatoon, B Khélifi, S Klepser, W Kluźniak, K Kosack, D Kostunin, RG Lang, S Le Stum, A Lemière, J-P Lenain, F Leuschner, T Lohse, A Luashvili, I Lypova, J Mackey, D Malyshev, V Marandon, P Marchegiani, A Marcowith, G Martí-Devesa, R Marx, A Mitchell, R Moderski, L Mohrmann, A Montanari, E Moulin, T Murach, K Nakashima, J Niemiec, A Priyana Noel, P O’Brien, L Olivera-Nieto, E de Ona Wilhelmi, M Ostrowski, S Panny, M Panter, G Peron, DA Prokhorov, G Pühlhofer, M Punch, A Quirrenbach, P Reichherzer, A Reimer, O Reimer, H Ren, M Renaud, F Rieger, B Rudak, E Ruiz-Velasco, V Sahakian, A Santangelo, M Sasaki, J Schäfer, F Schüssler, HM Schutte, U Schwanke, JNS Shapopi, A Specovius, S Spencer, Ł Stawarz, R Steenkamp, S Steinmassl, I Sushch, H Suzuki, T Takahashi, T Tanaka, R Terrier, C van Eldik, M Vecchi, J Veh, C Venter, J Vink, R White, A Wierzcholska, Yu Wun Wong, M Zacharias, D Zargaryan, AA Zdziarski, A Zech, S Zouari, N Żywucka, The HESS Collaboration, K Mori

Star formation in the centre of NGC 1808 as observed by ALMA

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 525:3 (2023) 3645-3661

Authors:

Guangwen Chen, George J Bendo, Gary A Fuller, Christian Henkel, Xu Kong

Pulsar polarization: a partial-coherence model

Monthly Notices of the Royal Astronomical Society 91̽�� University Press 525:1 (2023) 840-853

Authors:

Lucy S Oswald, Aris Karastergiou, Simon Johnston

Abstract:

The population of radio pulsars is observed to demonstrate certain polarization properties not explained by the conventional picture of pulsar polarization, namely frequency evolution of polarization, deviations of the linear polarization angle from a curve of geometric origins, and the presence of features in the circular polarization. We present the partial-coherence model as a way to explain the co-occurrence of these features and to provide an origin for circular polarization in radio pulsar profiles. We describe the mathematics of the model and demonstrate how it can explain these observed features, both on a population level and for the idiosyncrasies of individual pulsars. The partial coherence model can account for complex polarization behaviour, enabling improved access to information about pulsar geometries. We discuss the scientific implications of this for our understanding of pulsar radio emission and propagation.

A Radio Flare in the Long-Lived Afterglow of the Distant Short GRB 210726A: Energy Injection or a Reverse Shock from Shell Collisions?

(2023)

Authors:

Genevieve Schroeder, Lauren Rhodes, Tanmoy Laskar, Anya Nugent, Alicia Rouco Escorial, Jillian C Rastinejad, Wen-fai Fong, Alexander J van der Horst, Péter Veres, Kate D Alexander, Alex Andersson, Edo Berger, Peter K Blanchard, Sarah Chastain, Lise Christensen, Rob Fender, David A Green, Paul Groot, Ian Heywood, Assaf Horesh, Luca Izzo, Charles D Kilpatrick, Elmar Körding, Amy Lien, Daniele B Malesani, Vanessa McBride, Kunal Mooley, Antonia Rowlinson, Huei Sears, Ben Stappers, Nial Tanvir, Susanna D Vergani, Ralph AMJ Wijers, David Williams-Baldwin, Patrick Woudt

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