Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data: IceCube Collaboration
 Aartsen, M Ackermann, M Adams, J Aguilar, J Ahlers, M Ahrens, M Alispach, C Andeen, K Anderson, T Ansseau, I Anton, G Argüelles, C Auffenberg, J Axani, S Backes, P Bagherpour, H Bai, X Barbano, A Barwick, S Baum, V Bay, R Beatty, J Becker, K Tjus, J BenZvi, S Berley, D Bernardini, E Besson, D Binder, G Bindig, D Blaufuss, E Blot, S Bohm, C Börner, M Böser, S Botner, O Bourbeau, E Bourbeau, J Bradascio, F Braun, J Bretz, H Bron, S Brostean-Kaiser, J Burgman, A Busse, R Carver, T Chen, C Cheung, E Chirkin, D Clark, K Classen, L Collin, G Conrad, J Coppin, P Correa, P Cowen, D Cross, R Dave, P de André, J De Clercq, C DeLaunay, J Dembinski, H Deoskar, K De Ridder, S Desiati, P de Vries, K de Wasseige, G de With, M DeYoung, T Diaz, A Díaz-Vélez, J Dujmovic, H Dunkman, M Dvorak, E Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Evans, J Evenson, P Fahey, S Fazely, A Felde, J Filimonov, K Finley, C Franckowiak, A Friedman, E Fritz, A Gaisser, T Gallagher, J Ganster, E Garrappa, S Gerhardt, L Ghorbani, K Glauch, T Glüsenkamp, T Goldschmidt, A Gonzalez, J Grant, D Griffith, Z European Physical Journal C volume 80 issue 1 (01 Jan 2020)
Searches for neutrinos from cosmic-ray interactions in the Sun using seven years of IceCube data
 Neer, G Nisa, M Nygren Pollmann, A Oehler, M Olivas, A O'Murchadha, A O'Sullivan, E Palczewski, T Pandya, H Pankova, D Park, N Peiffer, P Heros, C Philippen, S Pieloth, D Pieper, S Pinat, E Plum, M Porcelli, A Price, P Przybylski, G Raab, C Raissi, A Relethford, B Journal of Cosmology and Astroparticle Physics

Modelling functions of sequential data with neural networks and the signature transform

Oxford Mathematician Patrick Kidger talks about his recent work on applying the tools of controlled differential equations to machine learning.

Sequential Data

The changing air pressure at a particular location may be thought of as a sequence in $\mathbb{R}$; the motion of a pen on paper may be thought of as a sequence in $\mathbb{R}^2$; the changes within financial markets may be thought of as a sequence in $\mathbb{R}^d$, with $d$ potentially very large.

A response to Rubin & Heitlauf: "Is the expansion of the universe accelerating? All signs still point to yes"
 Colin, J Mohayaee, R Rameez, M SARKAR, S (09 Dec 2019)
Constraints on Neutrino Emission from Nearby Galaxies Using the 2MASS
Redshift Survey and IceCube
 O'Murchadha, A O'Sullivan, E Palczewski, T Pollmann, A Nowicki, S Pandya, H Olivas, A Oehler, M Nygren Philippen, S Pankova, D Heros, C Pieloth, D Pizzuto, A Bourbeau, E Peiffer, P Pinat, E Park, N Gonzalez, J Hallgren, A Gündüz, M Griswold, S Griffith, Z Halliday, R Günder, M Journal of Cosmology and Astroparticle Physics
Is there really a `Hubble tension'?
 Rameez, M SARKAR, S Classical and Quantum Gravity
Combined sensitivity to the neutrino mass ordering with JUNO, the
IceCube Upgrade, and PINGU
 Collaboration, I Aartsen, M Ackermann, M Adams, J Aguilar, J Ahlers, M Ahrens, M Alispach, C Andeen, K Anderson, T Ansseau, I Anton, G Argüelles, C Arlen, T Auffenberg, J Axani, S Backes, P Bagherpour, H Bai, X V, A Barbano, A Bartos, I Barwick, S Bastian, B Baum, V Baur, S Bay, R Beatty, J Becker, K Tjus, J BenZvi, S Berley, D Bernardini, E Besson, D Binder, G Bindig, D Blaufuss, E Blot, S Bohm, C Bohmer, M Böser, S Botner, O Böttcher, J Bourbeau, E Bourbeau, J Bradascio, F Braun, J Bron, S Brostean-Kaiser, J Burgman, A Buscher, J Busse, R Carver, T Chen, C Cheung, E Chirkin, D Choi, S Clark, K Classen, L Coleman, A Collin, G Conrad, J Coppin, P Correa, P Cowen, D Cross, R Dave, P Clercq, C DeLaunay, J Dembinski, H Deoskar, K Ridder, S Desiati, P Vries, K Wasseige, G With, M DeYoung, T Diaz, A Díaz-Vélez, J Dujmovic, H Dunkman, M DuVernois, M Dvorak, E Eberhardt, B Ehrhardt, T Eller, P Engel, R Evans, J Evenson, P Fahey, S Farrag, K Fazely, A Felde, J Filimonov, K Finley, C Fox, D Franckowiak, A Friedman, E Fritz, A Gaisser, T Gallagher, J Ganster, E Garrappa, S Gartner, A Gerhardt, L Gernhaeuser, R Ghorbani, K Glauch, T Glüsenkamp, T Goldschmidt, A Gonzalez, J Grant, D Griffith, Z Griswold, S Günder, M Gündüz, M Haack, C Hallgren, A Halliday, R Halve, L Halzen, F Hanson, K Haugen, J Haungs, A Hebecker, D Heereman, D Heix, P Helbing, K Hellauer, R Henningsen, F Hickford, S Hignight, J Hill, G Hoffman, K Hoffmann, B Hoffmann, R Hoinka, T Hokanson-Fasig, B Holzapfel, K Hoshina, K Huang, F Huber, M Huber, T Huege, T Hultqvist, K Hünnefeld, M Hussain, R In, S Iovine, N Ishihara, A Japaridze, G Jeong, M Jero, K Jones, B Jonske, F Joppe, R Kalekin, O Kang, D Kang, W Kappes, A Kappesser, D Karg, T Karl, M Karle, A Katori, T Katz, U Kauer, M Keivani, A Kelley, J Kheirandish, A Kim, J Kintscher, T Kiryluk, J Kittler, T Klein, S Koirala, R Kolanoski, H Köpke, L Kopper, C Kopper, S Koskinen, D Kowalski, M Krauss, C Krings, K Krückl, G Kulacz, N Kurahashi, N Kyriacou, A Lanfranchi, J Larson, M Lauber, F Lazar, J Leonard, K Leszczyńska, A Leuermann, M Liu, Q Lohfink, E LoSecco, J Mariscal, C Lu, L Lucarelli, F Lünemann, J Luszczak, W Lyu, Y Ma, W Madsen, J Maggi, G Mahn, K Makino, Y Mallik, P Mallot, K Mancina, S Mandalia, S Mariş, I Marka, S Marka, Z Maruyama, R Mase, K Maunu, R McNally, F Meagher, K Medici, M Medina, A Meier, M Meighen-Berger, S Merino, G Meures, T Micallef, J Mockler, D Momenté, G Montaruli, T Moore, R Morse, R Moulai, M Muth, P Nagai, R Naumann, U Neer, G Niederhausen, H Nisa, M Nowicki, S Nygren, D Pollmann, A Oehler, M Olivas, A O'Murchadha, A O'Sullivan, E Palczewski, T Pandya, H Pankova, D Papp, L Park, N Peiffer, P Heros, C Petersen, T Philippen, S Pieloth, D Pinat, E Pinfold, J Pizzuto, A Plum, M Porcelli, A Price, P Przybylski, G Raab, C Raissi, A Rameez, M Rauch, L Rawlins, K Rea, I Reimann, R Relethford, B Renschler, M Renzi, G Resconi, E Rhode, W Richman, M Riegel, M Robertson, S Rongen, M Rott, C Ruhe, T Ryckbosch, D Rysewyk, D Safa, I Herrera, S Sandrock, A Sandroos, J Sandstrom, P Santander, M Sarkar, S Satalecka, K Schaufel, M Schieler, H Schlunder, P Schmidt, T Schneider, A Schneider, J Schröder, F Schumacher, L Sclafani, S Seckel, D Seunarine, S Shaevitz, M Shefali, S Silva, M Snihur, R Soedingrekso, J Soldin, D Söldner-Rembold, S Song, M Spiczak, G Spiering, C Stachurska, J Stamatikos, M Stanev, T Stein, R Stettner, J Steuer, A Stezelberger, T Stokstad, R Stößl, A Strotjohann, N Stürwald, T Stuttard, T Sullivan, G Taboada, I Taketa, A Tanaka, H Tenholt, F Ter-Antonyan, S Terliuk, A Tilav, S Tollefson, K Tomankova, L Tönnis, C Toscano, S Tosi, D Trettin, A Tselengidou, M Tung, C Turcati, A Turcotte, R Turley, C Ty, B Unger, E Elorrieta, M Usner, M Vandenbroucke, J Driessche, W Eijk, D Eijndhoven, N Santen, J Veberic, D Verpoest, S Vraeghe, M Walck, C Wallace, A Wallraff, M Wandkowsky, N Watson, T Weaver, C Weindl, A Weiss, M Weldert, J Wendt, C Werthebach, J Whelan, B Whitehorn, N Wiebe, K Wiebusch, C Wille, L Williams, D Wills, L Wolf, M Wood, J Wood, T Woschnagg, K Wrede, G Wren, S Xu, D Xu, X Xu, Y Yanez, J Yodh, G Yoshida, S Yuan, T Zöcklein, M Members, J Bezerra, T Birkenfeld, T Blum, D Bongrand, M Cabrera, A Cheng, Y Depnering, W Dötterl, O Enqvist, T Enzmann, H Genster, C Grassi, M Göttel, A Hackspacher, P Hagner, C Han, Y Heinz, T Kampmann, P Kuusiniemi, P Lachenmaier, T Loo, K Lorenz, S Lubsandorzhiev, B Ludhova, L Malyshkin, Y Meyhöfer, D Miramonti, L Müller, A Oberauer, L Pilarczyk, O Rebber, H Sawatzki, J Schever, M Schweizer, K Settimo, M Sirignano, C Smirnov, M Stahl, A Steiger, H Steinmann, J Sterr, T Stock, M Studenikin, A Tietzsch, A Trzaska, W Viaud, B Volpe, C Wang, W Wonsak, B Wurm, M Wysotzki, C Xuefeng, D Yermia, F Physical Review D: Particles, Fields, Gravitation and Cosmology http://arxiv.org/abs/1911.06745v1
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