Very low-frequency oscillations from the 11 Hz pulsar in Terzan 5: frame dragging back on the table.

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 502:4 (2021) 5472-5479

Authors:

L du Buisson, S Motta, R Fender

An early peak in the radio light curve of short-duration Gamma-Ray Burst 200826A

(2021)

Authors:

Lauren Rhodes, Rob Fender, David RA Williams, Kunal Mooley

MIGHTEE: are giant radio galaxies more common than we thought?

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 501:3 (2021) 3833-3845

Authors:

J Delhaize, I Heywood, M Prescott, Mj Jarvis, I Delvecchio, Ih Whittam, Sv White, Mj Hardcastle, Cl Hale, J Afonso, Y Ao, M Brienza, M Brueggen, Jd Collier, E Daddi, M Glowacki, N Maddox, Lk Morabito, I Prandoni, Z Randriamanakoto, S Sekhar, Fangxia An, Nj Adams, S Blyth, Raa Bowler, L Leeuw, L Marchetti, Sm Randriamampandry, K Thorat, N Seymour, O Smirnov, Ar Taylor, C Tasse, M Vaccari

Planet Hunters TESS II: Findings from the first two years of TESS

Monthly Notices of the Royal Astronomical Society 501:4 (2021) 4669-4690

Authors:

Nl Eisner, O Barragán, C Lintott, S Aigrain, B Nicholson, Ts Boyajian, S Howell, C Johnston, B Lakeland, G Miller, A McMaster, H Parviainen, Ej Safron, Me Schwamb, L Trouille, S Vaughan, N Zicher, C Allen, S Allen, M Bouslog, C Johnson, Mn Simon, Z Wolfenbarger, Eml Baeten, Dm Bundy, T Hoffman

Abstract:

© 2021 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We present the results from the first two years of the Planet Hunters TESS (PHT) citizen science project, which identifies planet candidates in the TESS (Transiting Exoplanet Survey Satellite) data by engaging members of the general public. Over 22 000 citizen scientists from around the world visually inspected the first 26 sectors of TESS data in order to help identify transit-like signals. We use a clustering algorithm to combine these classifications into a ranked list of events for each sector, the top 500 of which are then visually vetted by the science team. We assess the detection efficiency of this methodology by comparing our results to the list of TESS Objects of Interest (TOIs) and show that we recover 85 per cent of the TOIs with radii greater than 4 R and 51 per cent of those with radii between 3 and 4 R. Additionally, we present our 90 most promising planet candidates that had not previously been identified by other teams, 73 of which exhibit only a single-transit event in the TESS light curve, and outline our efforts to follow these candidates up using ground-based observatories. Finally, we present noteworthy stellar systems that were identified through the Planet Hunters TESS project.

SNEWS 2.0: a next-generation supernova early warning system for multi-messenger astronomy

New Journal of Physics IOP Publishing 23:3 (2021) 031201

Authors:

S Al Kharusi, SY BenZvi, JS Bobowski, W Bonivento, V Brdar, T Brunner, E Caden, M Clark, A Coleiro, M Colomer-Molla, JI Crespo-Anadón, A Depoian, D Dornic, V Fischer, D Franco, W Fulgione, A Gallo Rosso, M Geske, S Griswold, M Gromov, D Haggard, A Habig, O Halim, A Higuera, R Hill, S Horiuchi, K Ishidoshiro, C Kato, E Katsavounidis, D Khaitan, JP Kneller, A Kopec, V Kulikovskiy, M Lai, M Lamoureux, RF Lang, HL Li, M Lincetto, C Lunardini, J Migenda, D Milisavljevic, ME McCarthy, EO Connor, EO Sullivan, G Pagliaroli, D Patel, R Peres, BW Pointon, J Qin, N Raj, A Renshaw, A Roeth, J Rumleskie, K Scholberg, A Sheshukov, T Sonley, M Strait, V Takhistov, I Tamborra, J Tseng, CD Tunnell, J Vasel, CF Vigorito, B Viren, CJ Virtue, JS Wang, LJ Wen, L Winslow, FLH Wolfs, XJ Xu, Y Xu