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SN2017jgh: a high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 507:3 (2021) 3125-3138

Authors:

P Armstrong, BE Tucker, A Rest, R Ridden-Harper, Y Zenati, AL Piro, S Hinton, C Lidman, S Margheim, G Narayan, E Shaya, P Garnavich, D Kasen, V Villar, A Zenteno, I Arcavi, M Drout, RJ Foley, J Wheeler, J Anais, A Campillay, D Coulter, G Dimitriadis, D Jones, CD Kilpatrick, N Muñoz-Elgueta, C Rojas-Bravo, J Vargas-González, J Bulger, K Chambers, M Huber, T Lowe, E Magnier, BJ Shappee, S Smartt, KW Smith, T Barclay, G Barentsen, J Dotson, M Gully-Santiago, C Hedges, S Howell, A Cody, K Auchettl, A Bódi, Zs Bognár, J Brimacombe, P Brown, B Cseh, L Galbany, D Hiramatsu, TW-S Holoien, DA Howell, SW Jha, R Könyves-Tóth, L Kriskovics, C McCully, P Milne, J Muñoz, Y Pan, A Pál, H Sai, K Sárneczky, N Smith, Á Sódor, R Szabó, R Szakáts, S Valenti, J Vinkó, X Wang, K Zhang, G Zsidi
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A fast semidiscrete optimal transport algorithm for a unique reconstruction of the early Universe

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 506:1 (2021) 1165-1185

Authors:

Bruno Levy, Roya Mohayaee, Sebastian von Hausegger
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SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)

(2021)

Authors:

Qinan Wang, Armin Rest, Yossef Zenati, Ryan Ridden-Harper, Georgios Dimitriadis, Gautham Narayan, V Ashley Villar, Mark R Magee, Ryan J Foley, Edward J Shaya, Peter Garnavich, Lifan Wang, Lei Hu, Attila Bodi, Patrick Armstrong, Katie Auchettl, Thomas Barclay, Geert Barentsen, Zsófia Bognár, Joseph Brimacombe, Joanna Bulger, Jamison Burke, Peter Challis, Kenneth Chambers, David A Coulter, Géza Csörnyei, Borbála Cseh, Maxime Deckers, Jessie L Dotson, Lluís Galbany, Santiago González-Gaitán, Mariusz Gromadzki, Michael Gully-Santiago, Ottó Hanyecz, Christina Hedges, Daichi Hiramatsu, Griffin Hosseinzadeh, D Andrew Howell, Steve B Howell, Mark E Huber, Saurabh W Jha, David O Jones, Réka Könyves-Tóth, Csilla Kalup, Charlie Kilpatrick, Levente Kriskovics, Wenxiong Li, Thomas B Lowe, Steven Margheim, Curtis McCully, Ayan Mitra, Jose A Muñoz, Matt Nicholl, Jakob Nordin, András Pál, Yen-Chen Pan, Anthony L Piro, Sofia Rest, João Rino-Silvestre, César Rojas-Bravo, Krisztián Sárneczky, Matthew R Siebert, Stephen J Smartt, Ken Smith, Ádám Sódor, Maximilian D Stritzinger, Róbert Szabó, Róbert Szakáts, Brad E Tucker, József Vinkó, Xiaofeng Wang, J Craig Wheeler, David R Young, Alfredo Zenteno, Kaicheng Zhang, Gabriella Zsidi
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The LSST-DESC 3x2pt Tomography Optimization Challenge

(2021)

Authors:

Joe Zuntz, François Lanusse, Alex I Malz, Angus H Wright, Anže Slosar, Bela Abolfathi, David Alonso, Abby Bault, Clécio R Bom, Massimo Brescia, Adam Broussard, Jean-Eric Campagne, Stefano Cavuoti, Eduardo S Cypriano, Bernardo MO Fraga, Eric Gawiser, Elizabeth J Gonzalez, Dylan Green, Peter Hatfield, Kartheik Iyer, David Kirkby, Andrina Nicola, Erfan Nourbakhsh, Andy Park, Gabriel Teixeira, Katrin Heitmann, Eve Kovacs, Yao-Yuan Mao
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The SNO+ experiment

Journal of Instrumentation IOP Publishing 16:8 (2021) P08059

Authors:

V Albanese, R Alves, Mr Anderson, S Andringa, L Anselmo, E Arushanova, S Asahi, M Askins, Dj Auty, Ar Back, S Back, F Bar o, Z Barnard, A Barr, N Barros, D Bartlett, R Bayes, C Beaudoin, Ew Beier, G Berardi, A Bialek, Sd Biller, E Blucher, R Bonventre, M Boulay, D Braid, E Caden, Ej Callaghan, J Caravaca, J Carvalho, L Cavalli, D Chauhan, M Chen, O Chkvorets, Kj Clark, B Cleveland, C Connors, D Cookman, It Coulter, Ma Cox, D Cressy, X Dai, C Darrach, B Davis-Purcell, C Deluce, Mm Depatie, F Descamps, Armin Reichold

Abstract:

The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta (0νββ) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural tellurium, corresponding to 1.3 tonnes of 130Te. This paper provides a general overview of the SNO+ experiment, including detector design, construction of process plants, commissioning efforts, electronics upgrades, data acquisition systems, and calibration techniques. The SNO+ collaboration is reusing the acrylic vessel, PMT array, and electronics of the SNO detector, having made a number of experimental upgrades and essential adaptations for use with the liquid scintillator. With low backgrounds and a low energy threshold, the SNO+ collaboration will also pursue a rich physics program beyond the search for 0νββ decay, including studies of geo- and reactor antineutrinos, supernova and solar neutrinos, and exotic physics such as the search for invisible nucleon decay. The SNO+ approach to the search for 0νββ decay is scalable: a future phase with high 130Te-loading is envisioned to probe an effective Majorana mass in the inverted mass ordering region.
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