Galaxy Zoo: Clump Scout: Surveying the Local Universe for Giant Star-forming Clumps

The Astrophysical Journal American Astronomical Society 931:1 (2022) 16

Authors:

Dominic Adams, Vihang Mehta, Hugh Dickinson, Claudia Scarlata, Lucy Fortson, Sandor Kruk, Brooke Simmons, Chris Lintott

The SAMI Galaxy Survey: The Internal Orbital Structure and Mass Distribution of Passive Galaxies from Triaxial Orbit-superposition Schwarzschild Models

The Astrophysical Journal American Astronomical Society 930:2 (2022) 153

Authors:

Giulia Santucci, Sarah Brough, Jesse van de Sande, Richard M McDermid, Glenn van de Ven, Ling Zhu, Francesco D’Eugenio, Joss Bland-Hawthorn, Stefania Barsanti, Julia J Bryant, Scott M Croom, Roger L Davies, Andrew W Green, Jon S Lawrence, Nuria PF Lorente, Matt S Owers, Adriano Poci, Samuel N Richards, Sabine Thater, Sukyoung Yi

Deep extragalactic visible legacy survey (DEVILS): the emergence of bulges and decline of disc growth since z = 1

Monthly Notices of the Royal Astronomical Society Oxford University Press 515:1 (2022) 1175-1198

Authors:

Abdolhosein Hashemizadeh, Simon P Driver, Luke JM Davies, Aaron SG Robotham, Sabine Bellstedt, Caroline Foster, Benne W Holwerda, Matt Jarvis, Steven Phillipps, Malgorzata Siudek, Jessica E Thorne, Rogier A Windhorst, Christian Wolf

Abstract:

We present a complete structural analysis of the ellipticals (E), diffuse bulges (dB), compact bulges (cB), and discs (D) within a redshift range 0 < z < 1, and stellar mass log10(M∗/M⊙) ≥ 9.5 volume-limited sample drawn from the combined DEVILS and HST-COSMOS region. We use the profit code to profile over ∼35 000 galaxies for which visual classification into single or double component was pre-defined in Paper-I. Over this redshift range, we see a growth in the total stellar mass density (SMD) of a factor of 1.5. At all epochs we find that the dominant structure, contributing to the total SMD, is the disc, and holds a fairly constant share of ∼ 60 per cent of the total SMD from z = 0.8 to z = 0.2, dropping to ∼ 30 per cent at z = 0.0 (representing ∼ 33 per cent decline in the total disc SMD). Other classes (E, dB, and cB) show steady growth in their numbers and integrated stellar mass densities. By number, the most dramatic change across the full mass range is in the growth of diffuse bulges. In terms of total SMD, the biggest gain is an increase in massive elliptical systems, rising from 20 per cent at z = 0.8 to equal that of discs at z = 0.0 (30 per cent) representing an absolute mass growth of a factor of 2.5. Overall, we see a clear picture of the emergence and growth of all three classes of spheroids over the past 8 Gyr, and infer that in the later half of the Universe's timeline spheroid-forming processes and pathways (secular evolution, mass-accretion, and mergers) appear to dominate mass transformation over quiescent disc growth.

Search for flavour-changing neutral-current interactions of a top quark and a gluon in pp collisions at $$\sqrt{s}=13$$ TeV with the ATLAS detector

The European Physical Journal C SpringerOpen 82:4 (2022) 334

Authors:

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

Abstract:

A search is presented for the production of a single top quark via left-handed flavour-changing neutral-current (FCNC) interactions of a top quark, a gluon and an up or charm quark. Two production processes are considered: u+ g→ t and c+ g→ t. The analysis is based on proton–proton collision data taken at a centre-of-mass energy of 13 TeV with the ATLAS detector at the LHC. The data set corresponds to an integrated luminosity of 139 fb- 1. Events with exactly one electron or muon, exactly one b-tagged jet and missing transverse momentum are selected, resembling the decay products of a singly produced top quark. Neural networks based on kinematic variables differentiate between events from the two signal processes and events from background processes. The measured data are consistent with the background-only hypothesis, and limits are set on the production cross-sections of the signal processes: σ(u+g→t)×B(t→Wb)×B(W→ℓν)<3.0pb and σ(c+g→t)×B(t→Wb)×B(W→ℓν)<4.7pb at the 95% confidence level, with B(W→ ℓν) = 0.325 being the sum of branching ratios of all three leptonic decay modes of the W boson. Based on the framework of an effective field theory, the cross-section limits are translated into limits on the strengths of the tug and tcg couplings occurring in the theory: |CuGut|/Λ2<0.057TeV- 2 and |CuGct|/Λ2<0.14TeV- 2. These bounds correspond to limits on the branching ratios of FCNC-induced top-quark decays: B(t→ u+ g) < 0.61 × 10 - 4 and B(t→ c+ g) < 3.7 × 10 - 4

The science case and challenges of space-borne sub-millimeter interferometry

(2022)

Authors:

Leonid I Gurvits, Zsolt Paragi, Ricardo I Amils, Ilse van Bemmel, Paul Boven, Viviana Casasola, John Conway, Jordy Davelaar, M Carmen Díez-González, Heino Falcke, Rob Fender, Sándor Frey, Christian M Fromm, Juan D Gallego-Puyol, Cristina García-Miró, Michael A Garrett, Marcello Giroletti, Ciriaco Goddi, José L Gómez, Jeffrey van der Gucht, José Carlos Guirado, Zoltán Haiman, Frank Helmich, Ben Hudson, Elizabeth Humphreys, Violette Impellizzeri, Michael Janssen, Michael D Johnson, Yuri Y Kovalev, Michael Kramer, Michael Lindqvist, Hendrik Linz, Elisabetta Liuzzo, Andrei P Lobanov, Isaac López-Fernández, Inmaculada Malo-Gómez, Kunal Masania, Yosuke Mizuno, Alexander V Plavin, Raj T Rajan, Luciano Rezzolla, Freek Roelofs, Eduardo Ros, Kazi LJ Rygl, Tuomas Savolainen, Karl Schuster, Tiziana Venturi, Marjolein Verkouter, Pablo de Vicente, Pieter NAM Visser, Martina C Wiedner, Maciek Wielgus, Kaj Wiik, J Anton Zensus