Radio observations of the 2022 outburst of the transitional Z-Atoll source XTE J1701−462

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 533:2 (2024) 1800-1807

Authors:

KVS Gasealahwe, IM Monageng, RP Fender, PA Woudt, AK Hughes, SE Motta, J van den Eijnden, P Saikia, E Tremou

The Dark Energy Survey 5-yr photometrically classified type Ia supernovae without host-galaxy redshifts

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 533:2 (2024) 2073-2088

Authors:

A Möller, P Wiseman, M Smith, C Lidman, TM Davis, R Kessler, M Sako, M Sullivan, L Galbany, J Lee, RC Nichol, BO Sánchez, M Vincenzi, BE Tucker, TMC Abbott, M Aguena, S Allam, O Alves, F Andrade-Oliveira, D Bacon, E Bertin, D Brooks, A Carnero Rosell, FJ Castander, S Desai, HT Diehl, S Everett, I Ferrero, D Friedel, J Frieman, J García-Bellido, E Gaztanaga, G Giannini, RA Gruendl, G Gutierrez, SR Hinton, DL Hollowood, K Honscheid, DJ James, K Kuehn, O Lahav, S Lee, JL Marshall, J Mena-Fernández, F Menanteau, R Miquel, J Myles, RLC Ogando, A Palmese, A Pieres, AA Plazas Malagón, A Roodman, E Sanchez, D Sanchez Cid, I Sevilla-Noarbe, E Suchyta, MEC Swanson, G Tarle, DL Tucker, AR Walker, N Weaverdyck, LN da Costa, MES Pereira

Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A

(2024)

Authors:

JH Gillanders, SJ Smartt

Galaxy Zoo: Morphologies Based on UKIDSS NIR Imaging for 71,052 Galaxies

Research Notes of the American Astronomical Society American Astronomical Society 8:8 (2024) 198

Authors:

Karen L Masters, Melanie Galloway, Lucy Fortson, Chris J Lintott, Mike Read, Claudia Scarlata, Brooke Simmons, Mike Walmsley, Kyle Willett

Abstract:

We present morphological classifications based on Galaxy Zoo analysis of 71,052 galaxies with imaging from the United Kingdom Infrared Telescope Infrared Deep Sky Survey (UKIDSS). Galaxies were selected out of the Galaxy Zoo 2 (GZ2) sample, so also have gri imaging from the Sloan Digital Sky Survey. An identical classification tree, and vote weighting/aggregation was applied to both UKIDSS and GZ2 classifications enabling direct comparisons. With this Research Note we provide a public release of the GZ:UKIDSS morphologies and discuss some initial comparisons with GZ2.

Search for leptoquark pair production decaying into t e - t ¯ e + or t μ - t ¯ μ + in multi-lepton final states in pp collisions at s = 13 TeV with the ATLAS detector

The European Physical Journal C SpringerOpen 84:8 (2024) 818

Authors:

G Aad, B Abbott, DC Abbott, K Abeling, SH Abidi, A Aboulhorma, H Abramowicz, H Abreu, Y Abulaiti, AC Abusleme Hoffman, BS Acharya, B Achkar, C Adam Bourdarios, L Adamczyk, L Adamek, SV Addepalli, J Adelman, A Adiguzel, S Adorni, T Adye, AA Affolder, Y Afik, MN Agaras, J Agarwala

Abstract:

A search for leptoquark pair production decaying into te-t¯e+ or tμ-t¯μ+ in final states with multiple leptons is presented. The search is based on a dataset of pp collisions at s=13TeV recorded with the ATLAS detector during Run 2 of the Large Hadron Collider, corresponding to an integrated luminosity of 139 fb-1. Four signal regions, with the requirement of at least three light leptons (electron or muon) and at least two jets out of which at least one jet is identified as coming from a b-hadron, are considered based on the number of leptons of a given flavour. The main background processes are estimated using dedicated control regions in a simultaneous fit with the signal regions to data. No excess above the Standard Model background prediction is observed and 95% confidence level limits on the production cross section times branching ratio are derived as a function of the leptoquark mass. Under the assumption of exclusive decays into te- (tμ-), the corresponding lower limit on the scalar mixed-generation leptoquark mass mLQmixd is at 1.58 (1.59) TeV and on the vector leptoquark mass mU~1 at 1.67 (1.67) TeV in the minimal coupling scenario and at 1.95 (1.95) TeV in the Yang–Mills scenario.