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Measurement of the $^8$B Solar Neutrino Flux Using the Full SNO+ Water Phase

(2024)

Authors:

SNO Collaboration, :, A Allega, MR Anderson, S Andringa, M Askins, DJ Auty, A Bacon, J Baker, F Barão, N Barros, R Bayes, EW Beier, A Bialek, SD Biller, E Blucher, E Caden, EJ Callaghan, M Chen, S Cheng, B Cleveland, D Cookman, J Corning, MA Cox, R Dehghani, J Deloye, MM Depatie, F Di Lodovico, C Dima, J Dittmer, KH Dixon, MS Esmaeilian, E Falk, N Fatemighomi, R Ford, A Gaur, OI González-Reina, D Gooding, C Grant, J Grove, S Hall, AL Hallin, D Hallman, WJ Heintzelman, RL Helmer, C Hewitt, V Howard, B Hreljac, J Hu, P Huang, R Hunt-Stokes, SMA Hussain, AS Inácio, CJ Jillings, S Kaluzienski, T Kaptanoglu, H Khan, J Kladnik, JR Klein, LL Kormos, B Krar, C Kraus, CB Krauss, T Kroupová, C Lake, L Lebanowski, C Lefebvre, V Lozza, M Luo, A Maio, S Manecki, J Maneira, RD Martin, N McCauley, AB McDonald, G Milton, A Molina Colina, D Morris, M Mubasher, S Naugle, LJ Nolan, HM O'Keeffe, GD Orebi Gann, J Page, K Paleshi, W Parker, J Paton, SJM Peeters, L Pickard, B Quenallata, P Ravi, A Reichold, S Riccetto, J Rose, R Rosero, I Semenec, J Simms, P Skensved, M Smiley, J Smith, R Svoboda, B Tam, J Tseng, E Vázquez-Jáuregui, JGC Veinot, CJ Virtue, M Ward, JJ Weigand, JR Wilson, JD Wilson, A Wright, S Yang, M Yeh, Z Ye, S Yu, Y Zhang, K Zuber, A Zummo
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The ATLAS trigger system for LHC Run 3 and trigger performance in 2022

Journal of Instrumentation IOP Publishing 19:06 (2024) P06029

Authors:

G Aad, E Aakvaag, B Abbott, K Abeling, NJ Abicht, SH Abidi, A Aboulhorma, H Abramowicz, H Abreu, Y Abulaiti, BS Acharya, C Adam Bourdarios, L Adamczyk, SV Addepalli, MJ Addison, J Adelman, A Adiguzel, T Adye, AA Affolder, Y Afik, MN Agaras, J Agarwala, A Aggarwal, C Agheorghiesei

Abstract:

The ATLAS trigger system is a crucial component of the ATLAS experiment at the LHC. It is responsible for selecting events in line with the ATLAS physics programme. This paper presents an overview of the changes to the trigger and data acquisition system during the second long shutdown of the LHC, and shows the performance of the trigger system and its components in the proton-proton collisions during the 2022 commissioning period as well as its expected performance in proton-proton and heavy-ion collisions for the remainder of the third LHC data-taking period (2022–2025).
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Initial measurement of reactor antineutrino oscillation at SNO+

(2024)

Authors:

SNO Collaboration, :, A Allega, MR Anderson, S Andringa, M Askins, DM Asner, DJ Auty, A Bacon, J Baker, F Barão, N Barros, R Bayes, EW Beier, TS Bezerra, A Bialek, SD Biller, E Blucher, E Caden, EJ Callaghan, M Chen, S Cheng, B Cleveland, D Cookman, J Corning, MA Cox, R Dehghani, J Deloye, MM Depatie, F Di Lodovico, C Dima, J Dittmer, KH Dixon, MS Esmaeilian, E Falk, N Fatemighomi, R Ford, A Gaur, OI González-Reina, D Gooding, C Grant, J Grove, S Hall, AL Hallin, D Hallman, WJ Heintzelman, RL Helmer, C Hewitt, V Howard, B Hreljac, J Hu, P Huang, R Hunt-Stokes, SMA Hussain, AS Inácio, CJ Jillings, S Kaluzienski, T Kaptanoglu, H Khan, J Kladnik, JR Klein, LL Kormos, B Krar, C Kraus, CB Krauss, T Kroupová, C Lake, L Lebanowski, C Lefebvre, V Lozza, M Luo, A Maio, S Manecki, J Maneira, RD Martin, N McCauley, AB McDonald, C Mills, G Milton, A Molina Colina, D Morris, I Morton-Blake, M Mubasher, S Naugle, LJ Nolan, HM O'Keeffe, GD Orebi Gann, J Page, K Paleshi, W Parker, J Paton, SJM Peeters, L Pickard, B Quenallata, P Ravi, A Reichold, S Riccetto, J Rose, R Rosero, I Semenec, J Simms, P Skensved, M Smiley, J Smith, R Svoboda, B Tam, J Tseng, E Vázquez-Jáuregui, JGC Veinot, CJ Virtue, M Ward, JJ Weigand, JR Wilson, JD Wilson, A Wright, S Yang, M Yeh, Z Ye, S Yu, Y Zhang, K Zuber, A Zummo
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Event-by-event direction reconstruction of solar neutrinos in a high light-yield liquid scintillator

Physical Review D American Physical Society (APS) 109:7 (2024) 072002

Authors:

A Allega, MR Anderson, S Andringa, J Antunes, M Askins, DJ Auty, A Bacon, J Baker, N Barros, F Barão, R Bayes, EW Beier, TS Bezerra, A Bialek, SD Biller, E Blucher, E Caden, EJ Callaghan, M Chen, S Cheng, B Cleveland, D Cookman, J Corning, MA Cox, R Dehghani, J Deloye, MM Depatie, F Di Lodovico, J Dittmer, KH Dixon, E Falk, N Fatemighomi, R Ford, A Gaur, OI González-Reina, D Gooding, C Grant, J Grove, S Hall, AL Hallin, WJ Heintzelman, RL Helmer, C Hewitt, B Hreljac, V Howard, J Hu, R Hunt-Stokes, SMA Hussain, AS Inácio, CJ Jillings, S Kaluzienski, T Kaptanoglu, P Khaghani, H Khan, JR Klein, LL Kormos, B Krar, C Kraus, CB Krauss, T Kroupová, C Lake, L Lebanowski, J Lee, C Lefebvre, YH Lin, V Lozza, M Luo, A Maio, S Manecki, J Maneira, RD Martin, N McCauley, AB McDonald, C Mills, G Milton, I Morton-Blake, M Mubasher, A Molina Colina, D Morris, S Naugle, LJ Nolan, HM O’Keeffe, GD Orebi Gann, J Page, K Paleshi, W Parker, J Paton, SJM Peeters, L Pickard, P Ravi, A Reichold, S Riccetto, M Rigan, J Rose, R Rosero, J Rumleskie, I Semenec, P Skensved, M Smiley, J Smith, R Svoboda, B Tam, J Tseng, S Valder, E Vázquez-Jáuregui, CJ Virtue, J Wang, M Ward, JR Wilson, JD Wilson, A Wright, JP Yanez, S Yang, M Yeh, Z Ye, S Yu, Y Zhang, K Zuber, A Zummo
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Red supergiant candidates for multimessenger monitoring of the next Galactic supernova

Monthly Notices of the Royal Astronomical Society Oxford University Press 529:4 (2024) 3630-3650

Authors:

Sarah Healy, Shunsaku Horiuchi, Marta Colomer Molla, Dan Milisavljevic, Jeffrey Tseng, Faith Bergin, Kathryn Weil, Masaomi Tanaka, Sebastián Otero

Abstract:

We compile a catalogue of 578 highly probable and 62 likely red supergiants (RSGs) of the Milky Way, which represents the largest list of Galactic RSG candidates designed for continuous follow-up efforts to date. We match distances measured by Gaia DR3, 2MASS photometry, and a 3D Galactic dust map to obtain luminous bright late-type stars. Determining the stars' bolometric luminosities and effective temperatures, we compare to Geneva stellar evolution tracks to determine likely RSG candidates, and quantify contamination using a catalogue of Galactic AGB in the same luminosity-temperature space. We add details for common or interesting characteristics of RSG, such as multistar system membership, variability, and classification as a runaway. As potential future core-collapse supernova progenitors, we study the ability of the catalogue to inform the Supernova Early Warning System (SNEWS) coincidence network made to automate pointing, and show that for 3D position estimates made possible by neutrinos, the number of progenitor candidates can be significantly reduced, improving our ability to observe the progenitor pre-explosion and the early phases of core-collapse supernovae.
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