The rest-frame UV luminosity function at z≃4 : a significant contribution of AGN to the bright-end of the galaxy population

Monthly Notices of the Royal Astronomical Society Oxford University Press 494:2 (2020) 1771-1783

Authors:

Nathan Adams, Rebecca Bowler, Matthew Jarvis, Boris Haussler, Ross McLure, Andrew Bunker, James Dunlop, Aprajita Verma

Abstract:

We measure the rest-frame UV luminosity function (LF) at z ∼ 4 self-consistently over a wide range in absolute magnitude (−27 . MUV . −20). The LF is measured with 46,904 sources selected using a photometric redshift approach over ∼ 6 deg2 of the combined COSMOS and XMM-LSS fields. We simultaneously fit for both AGN and galaxy LFs using a combination of Schechter or Double Power Law (DPL) functions alongside a single power law for the faint-end slope of the AGN LF. We find a lack of evolution in the shape of the bright-end of the LBG component when compared to other studies at z ' 5 and evolutionary recipes for the UV LF. Regardless of whether the LBG LF is fit with a Schechter function or DPL, AGN are found to dominate at MUV < −23.5. We measure a steep faint-end slope of the AGN LF with αAGN = −2.09+0.35 −0.38 (−1.66+0.29 −0.58) when fit alongside a Schechter function (DPL) for the galaxies. Our results suggest that if AGN are morphologically selected it results in a bias to lower number densities. Only by considering the full galaxy population over the transition region from AGN to LBG domination can an accurate measurement of the total LF be attained.

Recent measurements on MiniMALTA, a radiationhard CMOS sensor with small collection electrodesfor ATLAS

Sissa Medialab Srl (2020) 020

Authors:

Patrick Moriishi Freeman, P Allport, A Andreazza, I Asensi Tortajada, M Barbero, S Bhat, D Bortoletto, I Berdalovic, C Bespin, C Buttar, I Caicedo, R Cardella, F Dachs, V Dao, Y Degerli, H Denizli, M Dyndal, L Flores Sanz de Acedo, L Gonella, A Habib, T Hemperek, T Hirono, T Kugathasan, V Liberali, I Mandic, D Maneuski, K Metodiev, M Mikuž, M Mironova, K Moustakas, M Munker, KY Oyulmaz, P Pangaud, H Pernegger, F Piro, R Plackett, P Riedler, H Sandaker, EJ Schioppa, P Schwemling, A Sharma, I Shipsey, L Simon Argemim, C Solans Sanchez, W Snoeys, T Suligoj, L Vigorelli, T Wang, D Weatherill, H Wennlöf, N Wermes, D Wood, S Worm

Searches for electroweak production of supersymmetric particles with compressed mass spectra in √s=13 TeV pp collisions with the ATLAS detector

Physical Review D: Particles, Fields, Gravitation and Cosmology American Physical Society 101:5 (2020) 052005

Authors:

Luca Ambroz, Giacomo Artoni, Moritz Backes, William Balunas, Alan Barr, Lydia Beresford, Daniela Bortoletto, Amanda Cooper-Sarkar, Foti, Joanna Frost, Gabriel Emmanuel Gallardo, Elizabeth Gallas, Claire Gwenlan, Hays, Brian Huffman, Kla Karava, Luigi Marchese, Claudia Merlassino, Koichi Nagai, Richard Nickerson, O'Neill, SR Paredes Saenz, Petrov, Elisabeth Schopf, Sharma, Shipsey, Beojan Stanislaus, Migle Stankaityte, Cecilia Tosciri, Tseng, Georg Viehhauser, Anthony Weidberg, Wölker, Gabija Zemaityte, Zgubič

Abstract:

This paper presents results of searches for the electroweak production of supersymmetric particles in models with compressed mass spectra. The searches use 139 fb⁻¹ of √s = 13 TeV proton-proton collision data collected by the ATLAS experiment at the Large Hadron Collider. Events with missing transverse momentum and two same-flavor, oppositely charged, low-transverse-momentum leptons are selected, and are further categorized by the presence of hadronic activity from initial-state radiation or a topology compatible with vector-boson fusion processes. The data are found to be consistent with predictions from the Standard Model. The results are interpreted using simplified models of R-parity-conserving supersymmetry in which the lightest supersymmetric partner is a neutralino with a mass similar to the lightest chargino, the second-to-lightest neutralino, or the slepton. Lower limits on the masses of charginos in different simplified models range from 193 to 240 GeV for moderate mass splittings, and extend down to mass splittings of 1.5 to 2.4 GeV at the LEP chargino bounds (92.4 GeV). Similar lower limits on degenerate light-flavor sleptons extend up to masses of 251 GeV and down to mass splittings of 550 MeV. Constraints on vector-boson fusion production of electroweak SUSY states are also presented.

A Rapid Change in X-Ray Variability and a Jet Ejection in the Black Hole Transient MAXI J1820+070

The Astrophysical Journal Letters American Astronomical Society 891:2 (2020) l29

Authors:

Jeroen Homan, Joe Bright, Sara E Motta, Diego Altamirano, Zaven Arzoumanian, Arkadip Basak, Tomaso M Belloni, Edward M Cackett, Rob Fender, Keith C Gendreau, Erin Kara, Dheeraj R Pasham, Ronald A Remillard, James F Steiner, Abigail L Stevens, Phil Uttley

Measurement of the Z ( → ℓ + ℓ − ) γ production cross-section in pp collisions at s = 13 TeV with the ATLAS detector

Journal of High Energy Physics Springer 2020:3 (2020) 54

Authors:

G Aad, B Abbott, DC Abbott, A Abed Abud, K Abeling, DK Abhayasinghe, SH Abidi, OS AbouZeid, NL Abraham, H Abramowicz, H Abreu, Y Abulaiti, BS Acharya, B Achkar, S Adachi, L Adam, C Adam Bourdarios, L Adamczyk, L Adamek, J Adelman, M Adersberger, A Adiguzel, S Adorni, T Adye

Abstract:

The production of a prompt photon in association with a Z boson is studied in proton-proton collisions at a centre-of-mass energy s = 13 TeV. The analysis uses a data sample with an integrated luminosity of 139 fb−1 collected by the ATLAS detector at the LHC from 2015 to 2018. The production cross-section for the process pp → ℓ+ℓ−γ + X (ℓ = e, μ) is measured within a fiducial phase-space region defined by kinematic requirements on the photon and the leptons, and by isolation requirements on the photon. An experimental precision of 2.9% is achieved for the fiducial cross-section. Differential cross-sections are measured as a function of each of six kinematic variables characterising the ℓ+ℓ−γ system. The data are compared with theoretical predictions based on next-to-leading-order and next-to-next-to-leading-order perturbative QCD calculations. The impact of next-to-leading-order electroweak corrections is also considered.