Publications


No surviving non-compact stellar companion to Cassiopeia A

ASTRONOMY & ASTROPHYSICS 623 (2019) ARTN A34

WE Kerzendorf, T Do, SE de Mink, Y Gotberg, D Milisavljevic, E Zapartas, M Renzo, S Justham, P Podsiadlowski, RA Fesen


First-order mean motion resonances in two-planet systems: general analysis and observed systems

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 482 (2019) 530-549

C Terquem, JCB Papaloizou


Ultrahigh energy cosmic rays from shocks in the lobes of powerful radio galaxies

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 482 (2019) 4303-4321

JH Matthews, AR Bell, KM Blundell, AT Araudo


Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

Astroparticle Physics 111 (2019) 35-53

A Acharyya, I Agudo, EO Angüner, R Alfaro, J Alfaro, C Alispach, R Aloisio, R Alves Batista, JP Amans, L Amati, E Amato, G Ambrosi, LA Antonelli, C Aramo, T Armstrong, F Arqueros, L Arrabito, K Asano, H Ashkar, C Balazs, M Balbo, B Balmaverde, P Barai, A Barbano, M Barkov, U Barres de Almeida, JA Barrio, D Bastieri, J Becerra González, J Becker Tjus, L Bellizzi, W Benbow, E Bernardini, MI Bernardos, K Bernlöhr, A Berti, M Berton, B Bertucci, V Beshley, B Biasuzzi, C Bigongiari, R Bird, E Bissaldi, J Biteau, O Blanch, J Blazek, C Boisson, G Bonanno, A Bonardi, C Bonavolontá, G Bonnoli, P Bordas, M Böttcher, J Bregeon, A Brill, AM Brown, K Brügge, P Brun, P Bruno, A Bulgarelli, T Bulik, M Burton, A Burtovoi, G Busetto, R Cameron, R Canestrari, M Capalbi, A Caproni, R Capuzzo-Dolcetta, P Caraveo, S Caroff, R Carosi, S Casanova, E Cascone, F Cassol, F Catalani, O Catalano, D Cauz, M Cerruti, S Chaty, A Chen, M Chernyakova, G Chiaro, M Cieślar, SM Colak, V Conforti, E Congiu, JL Contreras, J Cortina, A Costa, H Costantini, G Cotter, P Cristofari, P Cumani

© 2019 The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current ground-based instruments by a factor of five to twenty, depending on the energy, greatly improving both their angular and energy resolutions over four decades in energy (from 20 GeV to 300 TeV). This achievement will be possible by using tens of imaging Cherenkov telescopes of three successive sizes. They will be arranged into two arrays, one per hemisphere, located on the La Palma island (Spain) and in Paranal (Chile). We present here the optimised and final telescope arrays for both CTA sites, as well as their foreseen performance, resulting from the analysis of three different large-scale Monte Carlo productions.


Search for non-relativistic magnetic monopoles with IceCube: IceCube Collaboration (vol 74, 2938, 2014)

EUROPEAN PHYSICAL JOURNAL C 79 (2019) ARTN 124

MG Aartsen, R Abbasi, M Ackermann, J Adams, JA Aguilar, M Ahlers, D Altmann, C Arguelles, TC Arlen, J Auffenberg, X Bai, M Baker, SW Barwick, V Baum, R Bay, JJ Beatty, JB Tjus, K-H Becker, ML Benabderrahmane, S BenZvi, P Berghaus, D Berley, E Bernardini, A Bernhard, DZ Besson, G Binder, D Bindig, M Bissok, E Blaufuss, J Blumenthal, DJ Boersma, C Bohm, D Bose, S Boeser, O Botner, L Brayeur, H-P Bretz, AM Brown, R Bruijn, J Casey, M Casier, D Chirkin, A Christov, B Christy, K Clark, L Classen, F Clevermann, S Coenders, S Cohen, DF Cowen, AHC Silva, M Danninger, J Daughhetee, JC Davis, M Day, JPAM de Andre, C De Clercq, S De Ridder, P Desiati, KD de Vries, M de With, T DeYoung, JC Diaz-Velez, M Dunkman, R Eagan, B Eberhardt, B Eichmann, J Eisch, S Euler, PA Evenson, O Fadiran, AR Fazely, A Fedynitch, J Feintzeig, T Feusels, K Filimonov, C Finley, T Fischer-Wasels, S Flis, A Franckowiak, K Frantzen, T Fuchs, TK Gaisser, J Gallagher, L Gerhardt, L Gladstone, T Gluesenkamp, A Goldschmidt, G Golup, JG Gonzalez, JA Goodman, D Gora, DT Grandmont, D Grant, P Gretskov, JC Groh, A Gross, C Ha, C Haack, AH Ismail, P Hallen, A Hallgren, F Halzen, K Hanson, D Hebecker, D Heereman, D Heinen, K Helbing, R Hellauer, S Hickford, GC Hill, KD Hoffman, R Hoffmann, A Homeier, K Hoshina, F Huang, W Huelsnitz, PO Hulth, K Hultqvist, S Hussain, A Ishihara, E Jacobi, J Jacobsen, K Jagielski, GS Japaridze, K Jero, O Jlelati, B Kaminsky, A Kappes, T Karg, A Karle, M Kauer, JL Kelley, J Kiryluk, J Klaes, SR Klein, J-H Koehne, G Kohnen, H Kolanoski, L Kopke, C Kopper, S Kopper, DJ Koskinen, M Kowalski, M Krasberg, A Kriesten, K Krings, G Kroll, J Kunnen, N Kurahashi, T Kuwabara, M Labare, H Landsman, MJ Larson, M Lesiak-Bzdak, M Leuermann, J Leute, J Luenemann, O Macias, J Madsen, G Maggi, R Maruyama, K Mase, HS Matis, F McNally, K Meagher, A Meli, M Merck, T Meures, S Miarecki, E Middell, N Milke, J Miller, L Mohrmann, T Montaruli, R Morse, R Nahnhauer, U Naumann, H Niederhausen, SC Nowicki, DR Nygren, A Obertacke, S Odrowski, A Olivas, A Omairat, A O'Murchadha, T Palczewski, L Paul, JA Pepper, CP de los Heros, C Pfendner, D Pieloth, E Pinat, J Posselt, PB Price, GT Przybylski, M Quinnan, L Raedel, M Rameez, K Rawlins, P Redl, R Reimann, E Resconi, W Rhode, M Ribordy, M Richman, B Riedel, S Robertson, JP Rodrigues, C Rott, T Ruhe, B Ruzybayev, D Ryckbosch, SM Saba, H-G Sander, M Santander, S Sarkar, K Schatto, F Scheriau, T Schmidt, M Schmitz, S Schoenen, S Schoeneberg, A Schoenwald, A Schukraft, L Schulte, O Schulz, D Seckel, Y Sestayo, S Seunarine, R Shanidze, C Sheremata, MWE Smith, D Soldin, GM Spiczak, C Spiering, M Stamatikos, T Stanev, NA Stanisha, A Stasik, T Stezelberger, RG Stokstad, A Stoessl, EA Strahler, R Stroem, NL Strotjohann, GW Sullivan, H Taavola, I Taboada, A Tamburro, A Tepe, S Ter-Antonyan, G Tesic, S Tilav, PA Toale, MN Tobin, S Toscano, M Tselengidou, E Unger, M Usner, S Vallecorsa, N van Eijndhoven, J van Santen, M Vehring, M Voge, M Vraeghe, C Walck, M Wallraff, C Weaver, M Wellons, C Wendt, S Westerhoff, BJ Whelan, N Whitehorn, K Wiebe, CH Wiebusch, DR Williams, H Wissing, M Wolf, TR Wood, K Woschnagg, DL Xu, XW Xu, JP Yanez, G Yodh, S Yoshida, P Zarzhitsky, J Ziemann, S Zierke, M Zoll, I Collaboration


Zooming in on supermassive black holes: how resolving their gas cloud host renders their accretion episodic

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2018)

RS Beckmann, J Devriendt, A Slyz

Born in rapidly evolving mini-halos during the first billion years of the Universe, super- massive black holes (SMBH) feed from gas flows spanning many orders of magnitude, from the cosmic web in which they are embedded to their event horizon. As such, accretion onto SMBHs constitutes a formidable challenge to tackle numerically, and currently requires the use of sub-grid models to handle the flow on small, unresolved scales. In this paper, we study the impact of resolution on the accretion pattern of SMBHs initially inserted at the heart of dense galactic gas clouds, using a custom super-Lagrangian refinement scheme to resolve the black hole (BH) gravitational zone of influence. We find that once the self-gravitating gas cloud host is sufficiently well re- solved, accretion onto the BH is driven by the cloud internal structure, independently of the BH seed mass, provided dynamical friction is present during the early stages of cloud collapse. For a pristine gas mix of hydrogen and helium, a slim disc develops around the BH on sub-parsec scales, turning the otherwise chaotic BH accretion duty cycle into an episodic one, with potentially important consequences for BH feedback. In the presence of such a nuclear disc, BH mass growth predominantly occurs when infalling dense clumps trigger disc instabilities, fuelling intense albeit short-lived gas accretion episodes.


The feasibility of magnetic reconnection powered blazar flares from synchrotron self-Compton emission

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 486 (2019) 1548-1562

PJ Morris, WJ Potter, G Cotter


Intrinsic rotation driven by turbulent acceleration

PLASMA PHYSICS AND CONTROLLED FUSION 61 (2019) ARTN 025003

M Barnes, FI Parra


Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

ASTROPHYSICAL JOURNAL 870 (2019) ARTN 134

A Albert, M Andre, M Anghinolfi, M Ardid, J-J Aubert, J Aublin, T Avgitas, B Baret, J Barrios-Marti, S Basa, B Belhorma, V Bertin, S Biagi, R Bormuth, J Boumaaza, S Bourret, MC Bouwhuis, H Branzas, R Bruijn, J Brunner, J Busto, A Capone, L Caramete, J Carr, S Celli, M Chabab, RC El Moursli, T Chiarusi, M Circella, JAB Coelho, A Coleiro, M Colomer, R Coniglione, H Costantini, P Coyle, A Creusot, AF Diaz, A Deschamps, C Distefano, I Di Palma, A Domi, R Dona, C Donzaud, D Dornic, D Drouhin, T Eberl, I El Bojaddaini, N El Khayati, D Elsaesser, A Enzenhoefer, A Ettahiri, F Fassi, I Felis, P Fermani, G Ferrara, L Fusco, P Gay, H Glotin, T Gregoire, RG Ruiz, K Graf, S Hallmann, H van Haren, AJ Heijboer, Y Hello, JJ Hernandez-Rey, J Hoessl, J Hofestaedt, G Illuminati, M de Jong, M Jongen, M Kadler, O Kalekin, U Katz, NR Khan-Chowdhury, A Kouchner, M Kreter, I Kreykenbohm, V Kulikovskiy, C Lachaud, R Lahmann, D Lefevre, E Leonora, G Levi, M Lotze, S Loucatos, G Maggi, M Marcelin, A Margiotta, A Marinelli, JA Martinez-Mora, R Mele, K Melis, P Migliozzi, A Moussa, S Navas, E Nezri, A Nunez, M Organokov, GE Pavalas, C Pellegrino, P Piattelli, V Popa, T Pradier, L Quinn, C Racca, N Randazzo, G Riccobene, A Sanchez-Losa, M Saldana, I Salvadori, DFE Samtleben, M Sanguineti, P Sapienza, F Schussler, M Spurio, T Stolarczyk, M Taiuti, Y Tayalati, A Trovato, B Vallage, V Van Elewyck, F Versari, D Vivolo, J Wilms, D Zaborov, JD Zornoza, J Zuniga, MG Aartsen, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, D Altmann, K Andeen, T Anderson, I Ansseau, G Anton, C Arguelles, J Auffenberg, S Axani, P Backes, H Bagherpour, X Bai, A Barbano, JP Barron, SW Barwick, V Baum, R Bay, JJ Beatty, JB Tjus, K-H Becker, S BenZvi, D Berley, E Bernardini, DZ Besson, G Binder, D Bindig, E Blaufuss, S Blot, C Bohm, M Boerner, F Bos, S Boeser, O Botner, E Bourbeau, J Bourbeau, F Bradascio, J Braun, M Brenzke, H-P Bretz, S Bron, J Brostean-Kaiser, A Burgman, RS Busse, T Carver, E Cheung, D Chirkin, K Clark, L Classen, GH Collin, JM Conrad, P Coppin, P Correa, DF Cowen, R Cross, P Dave, M Day, JPAM de Andre, C De Clercq, JJ DeLaunay, H Dembinski, K Deoskar, S De Ridder, P Desiati, KD de Vries, G de Wasseige, M de With, T DeYoung, JC Diaz-Velez, V di Lorenzo, H Dujmovic, JP Dumm, M Dunkman, E Dvorak, B Eberhardt, T Ehrhardt, B Eichmann, P Eller, PA Evenson, S Fahey, AR Fazely, J Felde, K Filimonov, C Finley, A Franckowiak, E Friedman, A Fritz, TK Gaisser, J Gallagher, E Ganster, S Garrappa, L Gerhardt, K Ghorbani, W Giang, T Glauch, T Gluesenkamp, A Goldschmidt, JG Gonzalez, D Grant, Z Griffith, C Haack, A Hallgren, L Halve, F Halzen, K Hanson, D Hebecker, D Heereman, K Helbing, R Hellauer, S Hickford, J Hignight, GC Hill, KD Hoffman, R Hoffmann, T Hoinka, B Hokanson-Fasig, K Hoshina, F Huang, M Huber, K Hultqvist, M Huennefeld, R Hussain, S In, N Iovine, A Ishihara, E Jacobi, GS Japaridze, M Jeong, K Jero, BJP Jones, P Kalaczynski, W Kang, A Kappes, D Kappesser, T Karg, A Karle, M Kauer, A Keivani, JL Kelley, A Kheirandish, J Kim, T Kintscher, J Kiryluk, T Kittler, SR Klein, R Koirala, H Kolanoski, L Koepke, C Kopper, S Kopper, JP Koschinsky, DJ Koskinen, M Kowalski, K Krings, M Kroll, G Krueckl, S Kunwar, N Kurahashi, A Kyriacou, M Labare, JL Lanfranchi, MJ Larson, F Lauber, K Leonard, M Leuermann, QR Liu, E Lohfink, CJL Mariscal, L Lu, J Lunemann, W Luszczak, J Madsen, KBM Mahn, Y Makino, S Mancina, IC Maris, R Maruyama, K Mase, R Maunu, K Meagher, M Medici, M Meier, T Menne, G Merino, T Meures, S Miarecki, J Micallef, G Momente, T Montaruli, RW Moore, M Moulai, R Nagai, R Nahnhauer, P Nakarmi, U Naumann, G Neer, H Niederhausen, SC Nowicki, DR Nygren, AO Pollmann, A Olivas, A O'Murchadha, E O'Sullivan, T Palczewski, H Pandya, DV Pankova, P Peiffer, JA Pepper, CP de los Heros, D Pieloth, E Pinat, A Pizzuto, M Plum, PB Price, GT Przybylski, C Raab, M Rameez, L Rauch, K Rawlins, IC Rea, R Reimann, B Relethford, G Renzi, E Resconi, W Rhode, M Richman, S Robertson, M Rongen, C Rott, T Ruhe, D Ryckbosch, D Rysewyk, I Safa, SES Herrera, A Sandrock, J Sandroos, M Santander, S Sarkar, K Satalecka, M Schaufel, P Schlunder, T Schmidt, A Schneider, J Schneider, S Schoeneberg, L Schumacher, S Sclafani, D Seckel, S Seunarine, J Soedingrekso, D Soldin, M Song, GM Spiczak, C Spiering, J Stachurska, M Stamatikos, T Stanev, A Stasik, R Stein, J Stettner, A Steuer, T Stezelberger, RG Stokstad, A Stossl, NL Strotjohann, T Stuttard, GW Sullivan, M Sutherland, I Taboada, F Tenholt, S Ter-Antonyan, A Terliuk, S Tilav, PA Toale, MN Tobin, C Tonnis, S Toscano, D Tosi, M Tselengidou, CF Tung, A Turcati, R Turcotte, CF Turley, B Ty, E Unger, MAU Elorrieta, M Usner, J Vandenbroucke, W Van Driessche, D van Eijk, N van Eijndhoven, S Vanheule, J van Santen, M Vraeghe, C Walck, A Wallace, M Wallraff, FD Wandler, N Wandkowsky, TB Watson, A Waza, C Weaver, MJ Weiss, C Wendt, J Werthebach, S Westerhoff, BJ Whelan, N Whitehorn, K Wiebe, CH Wiebusch, L Wille, DR Williams, L Wills, M Wolf, J Wood, TR Wood, E Woolsey, K Woschnagg, G Wrede, DL Xu, XW Xu, Y Xu, JP Yanez, G Yodh, S Yoshida, T Yuan, BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, C Adams, VB Adya, C Affeldt, M Agathos, K Agatsuma, N Aggarwal, OD Aguiar, L Aiello, A Ain, P Ajith, G Allen, A Allocca, MA Aloy, PA Altin, A Amato, A Ananyeva, SB Anderson, WG Anderson, SV Angelova, S Antier, S Appert, K Arai, MC Araya, JS Areeda, M Arene, N Arnaud, KG Arun, S Ascenzi, G Ashton, SM Aston, P Astone, F Aubin, P Aufmuth, K AultONeal, C Austin, V Avendano, A Avila-Alvarez, S Babak, P Bacon, F Badaracco, MKM Bader, S Bae, PT Baker, F Baldaccini, G Ballardin, SW Ballmer, S Banagiri, JC Barayoga, SE Barclay, BC Barish, D Barker, K Barkett, S Barnum, F Barone, B Barr, L Barsotti, M Barsuglia, D Barta, J Bartlett, I Bartos, R Bassiri, A Basti, M Bawaj, JC Bayley, M Bazzan, B Becsy, M Bejger, I Belahcene, AS Bell, D Beniwal, BK Berger, G Bergmann, S Bernuzzi, JJ Bero, CPL Berry, D Bersanetti, A Bertolini, J Betzwieser, R Bhandare, J Bidler, IA Bilenko, SA Bilgili, G Billingsley, J Birch, R Birney, O Birnholtz, S Biscans, S Biscoveanu, A Bisht, M Bitossi, MA Bizouard, JK Blackburn, CD Blair, DG Blair, RM Blair, S Bloemen, N Bode, M Boer, Y Boetzel, G Bogaert, F Bondu, E Bonilla, R Bonnand, P Booker, BA Boom, CD Booth, R Bork, V Boschi, S Bose, K Bossie, V Bossilkov, J Bosveld, Y Bouffanais, A Bozzi, C Bradaschia, PR Brady, A Bramley, M Branchesi, JE Brau, T Briant, JH Briggs, F Brighenti, A Brillet, M Brinkmann, V Brisson, P Brockill, AF Brooks, DD Brown, S Brunett, A Buikema, T Bulik, HJ Bulten, A Buonanno, D Buskulic, C Buy, RL Byer, M Cabero, L Cadonati, G Cagnoli, C Cahillane, JC Bustillo, TA Callister, E Calloni, JB Camp, WA Campbell, KC Cannon, H Cao, J Cao, E Capocasa, F Carbognani, S Caride, MF Carney, G Carullo, JC Diaz, C Casentini, S Caudill, M Cavaglia, F Cavalier, R Cavalieri, G Cella, P Cerda-Duran, G Cerretani, E Cesarini, O Chaibi, K Chakravarti, SJ Chamberlin, M Chan, S Chao, P Charlton, EA Chase, E Chassande-Mottin, D Chatterjee, M Chaturvedi, BD Cheeseboro, HY Chen, X Chen, Y Chen, H-P Cheng, CK Cheong, HY Chia, A Chincarini, A Chiummo, G Cho, HS Cho, M Cho, N Christensen, Q Chu, S Chua, KW Chung, S Chung, G Ciani, AA Ciobanu, R Ciolfi, F Cipriano, A Cirone, F Clara, JA Clark, P Clearwater, F Cleva, C Cocchieri, E Coccia, P-F Cohadon, D Cohen, R Colgan, M Colleoni, CG Collette, C Collins, LR Cominsky, M Constancio Jr, L Conti, SJ Cooper, P Corban, TR Corbitt, I Cordero-Carrion, KR Corley, N Cornish, A Corsi, S Cortese, CA Costa, R Cotesta, MW Coughlin, SB Coughlin, J-P Coulon, ST Countryman, P Couvares, PB Covas, EE Cowan, DM Coward, MJ Cowart, DC Coyne, R Coyne, JDE Creighton, TD Creighton, J Cripe, M Croquette, SG Crowder, TJ Cullen, A Cumming, L Cunningham, E Cuoco, T Dal Canton, G Dalya, SL Danilishin, S D'Antonio, K Danzmann, A Dasgupta, CFDS Costa, LEH Datrier, V Dattilo, I Dave, M Davier, D Davis, EJ Daw, D DeBra, M Deenadayalan, J Degallaix, M De Laurentis, S Deleglise, W Del Pozzo, LM DeMarchi, N Demos, T Dent, M Denys, R De Pietri, J Derby, R De Rosa, C De Rossi, R DeSalvo, O de Varona, S Dhurandhar, MC Diaz, T Dietrich, L Di Fiore, M Di Giovanni, T Di Girolamo, A Di Lieto, B Ding, S Di Pace, F Di Renzo, A Dmitriev, Z Doctor, F Donovan, KL Dooley, S Doravari, I Dorrington, TP Downes, M Drago, JC Driggers, Z Du, J-G Ducoin, P Dupej, SE Dwyer, PJ Easter, TB Edo, MC Edwards, A Effler, P Ehrens, J Eichholz, SS Eikenberry, M Eisenmann, RA Eisenstein, RC Essick, H Estelles, D Estevez, ZB Etienne, T Etzel, M Evans, TM Evans, V Fafone, H Fair, S Fairhurst, X Fan, S Farinon, B Farr, WM Farr, EJ Fauchon-Jones, M Favata, M Fays, M Fazio, C Fee, J Feicht, MM Fejer, F Feng, A Fernandez-Galiana, I Ferrante, EC Ferreira, TA Ferreira, F Ferrini, F Fidecaro, I Fiori, D Fiorucci, M Fishbach, RP Fisher, JM Fishner, M Fitz-Axen, R Flaminio, M Fletcher, E Flynn, H Fong, JA Font, PWF Forsyth, J-D Fournier, S Frasca, F Frasconi, Z Frei, A Freise, R Frey, V Frey, P Fritschel, VV Frolov, P Fulda, M Fyffe, HA Gabbard, BU Gadre, SM Gaebel, JR Gair, L Gammaitoni, MR Ganija, SG Gaonkar, A Garcia, C Garcia-Quiros, F Garufi, B Gateley, S Gaudio, G Gaur, V Gayathri, G Gemme, E Genin, A Gennai, D George, J George, L Gergely, V Germain, S Ghonge, A Ghosh, A Ghosh, S Ghosh, B Giacomazzo, JA Giaime, KD Giardina, A Giazotto, K Gill, G Giordano, L Glover, P Godwin, E Goetz, R Goetz, B Goncharov, G Gonzalez, JMG Castro, A Gopakumar, ML Gorodetsky, SE Gossan, M Gosselin, R Gouaty, A Grado, C Graef, M Granata, A Grant, S Gras, P Grassia, C Gray, R Gray, G Greco, AC Green, R Green, EM Gretarsson, P Groot, H Grote, S Grunewald, P Gruning, GM Guidi, HK Gulati, Y Guo, A Gupta, MK Gupta, EK Gustafson, R Gustafson, L Haegel, O Halim, BR Hall, ED Hall, EZ Hamilton, G Hammond, M Haney, MM Hanke, J Hanks, C Hanna, OA Hannuksela, J Hanson, T Hardwick, K Haris, J Harms, GM Harry, IW Harry, C-J Haster, K Haughian, FJ Hayes, J Healy, A Heidmann, MC Heintze, H Heitmann, P Hello, G Hemming, M Hendry, IS Heng, J Hennig, AW Heptonstall, FJ Hernandez, M Heurs, S Hild, T Hinderer, D Hoak, S Hochheim, D Hofman, AM Holgado, NA Holland, K Holt, DE Holz, P Hopkins, C Horst, J Hough, EJ Howell, CG Hoy, A Hreibi, EA Huerta, D Huet, B Hughey, M Hulko, S Husa, SH Huttner, T Huynh-Dinh, B Idzkowski, A Iess, C Ingram, R Inta, G Intini, B Irwin, HN Isa, J-M Isac, M Isi, BR Iyer, K Izumi, T Jacqmin, SJ Jadhav, K Jani, NN Janthalur, P Jaranowski, AC Jenkins, J Jiang, DS Johnson, AW Jones, DI Jones, R Jones, RJG Jonker, L Ju, J Junker, CV Kalaghatgi, V Kalogera, B Kamai, S Kandhasamy, G Kang, JB Kanner, SJ Kapadia, S Karki, KS Karvinen, R Kashyap, M Kasprzack, S Katsanevas, E Katsavounidis, W Katzman, S Kaufer, K Kawabe, NV Keerthana, F Kefelian, D Keitel, R Kennedy, JS Key, FY Khalili, H Khan, I Khan, S Khan, Z Khan, EA Khazanov, M Khursheed, N Kijbunchoo, C Kim, JC Kim, K Kim, W Kim, WS Kim, Y-M Kim, C Kimball, EJ King, PJ King, M Kinley-Hanlon, R Kirchhoff, JS Kissel, L Kleybolte, JH Klika, S Klimenko, TD Knowles, P Koch, SM Koehlenbeck, G Koekoek, S Koley, V Kondrashov, A Kontos, N Koper, M Korobko, WZ Korth, I Kowalska, DB Kozak, V Kringel, N Krishnendu, A Krolak, G Kuehn, A Kumar, P Kumar, R Kumar, S Kumar, L Kuo, A Kutynia, S Kwang, BD Lackey, KH Lai, TL Lam, M Landry, BB Lane, RN Lang, J Lange, B Lantz, RK Lanza, A Lartaux-Vollard, PD Lasky, M Laxen, A Lazzarini, C Lazzaro, P Leaci, S Leavey, YK Lecoeuche, CH Lee, HK Lee, HM Lee, HW Lee, J Lee, K Lee, J Lehmann, A Lenon, N Leroy, N Letendre, Y Levin, J Li, KJL Li, TGF Li, X Li, F Lin, F Linde, SD Linker, TB Littenberg, J Liu, X Liu, RKL Lo, NA Lockerbie, LT London, A Longo, M Lorenzini, V Loriette, M Lormand, G Losurdo, JD Lough, CO Lousto, G Lovelace, ME Lower, H Lueck, D Lumaca, AP Lundgren, R Lynch, Y Ma, R Macas, S Macfoy, M MacInnis, DM Macleod, A Macquet, F Magana-Sandoval, LM Zertuche, RM Magee, E Majorana, I Maksimovic, A Malik, N Man, V Mandic, V Mangano, GL Mansell, M Manske, M Mantovani, F Marchesoni, F Marion, S Marka, Z Marka, C Markakis, AS Markosyan, A Markowitz, E Maros, A Marquina, S Marsat, F Martelli, IW Martin, RM Martin, DV Martynov, K Mason, E Massera, A Masserot, TJ Massinger, M Masso-Reid, S Mastrogiovanni, A Matas, F Matichard, L Matone, N Mavalvala, N Mazumder, JJ McCann, R McCarthy, DE McClelland, S McCormick, L McCuller, SC McGuire, J McIver, DJ McManus, T McRae, ST McWilliams, D Meacher, GD Meadors, M Mehmet, AK Mehta, J Meidam, A Melatos, G Mendell, RA Mercer, L Mereni, EL Merilh, M Merzougui, S Meshkov, C Messenger, C Messick, R Metzdorff, PM Meyers, H Miao, C Michel, H Middleton, EE Mikhailov, L Milano, AL Miller, A Miller, M Millhouse, JC Mills, MC Milovich-Goff, O Minazzoli, Y Minenkov, A Mishkin, C Mishra, T Mistry, S Mitra, VP Mitrofanov, G Mitselmakher, R Mittleman, G Mo, D Moffa, K Mogushi, SRP Mohapatra, M Montani, CJ Moore, D Moraru, G Moreno, S Morisaki, B Mours, CM Mow-Lowry, A Mukherjee, D Mukherjee, S Mukherjee, N Mukund, A Mullavey, J Munch, EA Muniz, M Muratore, PG Murray, I Nardecchia, L Naticchioni, RK Nayak, J Neilson, G Nelemans, TJN Nelson, M Nery, A Neunzert, KY Ng, S Ng, P Nguyen, D Nichols, S Nissanke, F Nocera, C North, LK Nuttall, M Obergaulinger, J Oberling, BD O'Brien, GD O'Dea, GH Ogin, JJ Oh, SH Oh, F Ohme, H Ohta, MA Okada, M Oliver, P Oppermann, RJ Oram, B O'Reilly, RG Ormiston, LF Ortega, R O'Shaughnessy, S Ossokine, DJ Ottaway, H Overmier, BJ Owen, AE Pace, G Pagano, MA Page, A Pai, SA Pai, JR Palamos, O Palashov, C Palomba, A Pal-Singh, H-W Pan, B Pang, PTH Pang, C Pankow, F Pannarale, BC Pant, F Paoletti, A Paoli, A Parida, W Parker, D Pascucci, A Pasqualetti, R Passaquieti, D Passuello, M Patil, B Patricelli, BL Pearlstone, C Pedersen, M Pedraza, R Pedurand, A Pele, S Penn, CJ Perez, A Perreca, HP Pfeiffer, M Phelps, KS Phukon, OJ Piccinni, M Pichot, F Piergiovanni, G Pillant, L Pinard, M Pirello, M Pitkin, R Poggiani, DYT Pong, S Ponrathnam, P Popolizio, EK Porter, J Powell, AK Prajapati, J Prasad, K Prasai, R Prasanna, G Pratten, T Prestegard, S Privitera, GA Prodi, LG Prokhorov, O Puncken, M Punturo, P Puppo, M Puerrer, H Qi, V Quetschke, PJ Quinonez, EA Quintero, R Quitzow-James, FJ Raab, H Radkins, N Radulescu, P Raffai, S Raja, C Rajan, B Rajbhandari, M Rakhmanov, KE Ramirez, A Ramos-Buades, J Rana, K Rao, P Rapagnani, V Raymond, M Razzano, J Read, T Regimbau, L Rei, S Reid, DH Reitze, W Ren, F Ricci, CJ Richardson, JW Richardson, PM Ricker, K Riles, M Rizzo, NA Robertson, R Robie, F Robinet, A Rocchi, L Rolland, JG Rollins, VJ Roma, M Romanelli, R Romano, CL Romel, JH Romie, K Rose, D Rosinska, SG Rosofsky, MP Ross, S Rowan, A Ruediger, P Ruggi, G Rutins, K Ryan, S Sachdev, T Sadecki, M Sakellariadou, L Salconi, M Saleem, A Samajdar, L Sammut, EJ Sanchez, LE Sanchez, N Sanchis-Gual, V Sandberg, JR Sanders, KA Santiago, N Sarin, B Sassolas, PR Saulson, O Sauter, RL Savage, P Schale, M Scheel, J Scheuer, F Schiettekatte, P Schmidt, R Schnabel, RMS Schofield, A Schoenbeck, E Schreiber, BW Schulte, BF Schutz, SG Schwalbe, J Scott, SM Scott, E Seidel, D Sellers, AS Sengupta, N Sennett, D Sentenac, V Sequino, A Sergeev, Y Setyawati, DA Shaddock, T Shaffer, MS Shahriar, MB Shaner, L Shao, P Sharma, P Shawhan, H Shen, R Shink, DH Shoemaker, DM Shoemaker, S ShyamSundar, K Siellez, M Sieniawska, D Sigg, AD Silva, LP Singer, N Singh, A Singhal, AM Sintes, S Sitmukhambetov, V Skliris, BJJ Slagmolen, TJ Slaven-Blair, JR Smith, RJE Smith, S Somala, EJ Son, B Sorazu, F Sorrentino, T Souradeep, E Sowell, AP Spencer, AK Srivastava, V Srivastava, K Staats, C Stachie, M Standke, DA Steer, M Steinke, J Steinlechner, S Steinlechner, D Steinmeyer, SP Stevenson, D Stocks, R Stone, DJ Stops, KA Strain, G Stratta, SE Strigin, A Strunk, R Sturani, AL Stuver, V Sudhir, TZ Summerscales, L Sun, S Sunil, J Suresh, PJ Sutton, BL Swinkels, MJ Szczepanczyk, M Tacca, SC Tait, C Talbot, D Talukder, DB Tanner, M Tapai, A Taracchini, JD Tasson, R Taylor, F Thies, M Thomas, P Thomas, SR Thondapu, KA Thorne, E Thrane, S Tiwari, S Tiwari, V Tiwari, K Toland, M Tonelli, Z Tornasi, A Torres-Forne, CI Torrie, D Toyra, F Travasso, G Traylor, MC Tringali, L Trozzo, R Trudeau, KW Tsang, M Tse, R Tso, L Tsukada, D Tsuna, D Tuyenbayev, K Ueno, D Ugolini, CS Unnikrishnan, AL Urban, SA Usman, H Vahlbruch, G Vajente, G Valdes, N van Bakel, M van Beuzekom, JFJ van den Brand, C Van Den Broeck, DC Vander-Hyde, L van der Schaaf, HJV van, AA van Veggel, M Vardaro, V Varma, S Vass, M Vasuth, A Vecchio, G Vedovato, J Veitch, PJ Veitch, K Venkateswara, G Venugopalan, D Verkindt, F Vetrano, A Vicere, AD Viets, DJ Vine, J-Y Vinet, S Vitale, T Vo, H Vocca, C Vorvick, SP Vyatchanin, AR Wade, LE Wade, M Wade, R Walet, M Walker, L Wallace, S Walsh, G Wang, H Wang, JZ Wang, WH Wang, YF Wang, RL Ward, ZA Warden, J Warner, M Was, J Watchi, B Weaver, L-W Wei, M Weinert, AJ Weinstein, R Weiss, F Wellmann, L Wen, EK Wessel, P Wessels, JW Westhouse, K Wette, JT Whelan, BF Whiting, C Whittle, DM Wilken, D Williams, AR Williamson, JL Willis, B Willke, MH Wimmer, W Winkler, CC Wipf, H Wittel, G Woan, J Woehler, JK Wofford, J Worden, JL Wright, DS Wu, DM Wysocki, L Xiao, H Yamamoto, CC Yancey, L Yang, MJ Yap, M Yazback, DW Yeeles, H Yu, H Yu, SHR Yuen, M Yvert, AK Zadrozny, A Zadrozny, M Zanolin, T Zelenova, J-P Zendri, M Zevin, J Zhang, L Zhang, T Zhang, C Zhao, M Zhou, Z Zhou, XJ Zhu, ME Zucker, J Zweizig, ANTARES Collaboration, ANTARES Collaboration, I Collaboration, I Collaboration, LIGOS Collaboration, LIGOS Collaboration, V Collaboration


$\texttt{stella}$: a mixed implicit-explicit, delta-f gyrokinetic code for general magnetic field configurations

Journal of Computational Physics Elsevier (2019)

M Barnes, F Parra-Diaz, M Landreman

Here we present details of a mixed implicit-explicit numerical scheme for the solution of the gyrokinetic-Poisson system of equations in the local limit. This scheme has been implemented in a new code called $\texttt{stella}$, which is capable of evolving electrostatic fluctuations with full kinetic electron effects and an arbitrary number of ion species in general magnetic geometry. We demonstrate the advantages of this mixed approach over a fully explicit treatment and provide linear and nonlinear benchmark comparisons for both axisymmetric and non-axisymmetric magnetic equilibria.


Supersonic plasma turbulence in the laboratory.

Nature communications 10 (2019) 1758-

TG White, MT Oliver, P Mabey, M Kühn-Kauffeldt, AFA Bott, LNK Döhl, AR Bell, R Bingham, R Clarke, J Foster, G Giacinti, P Graham, R Heathcote, M Koenig, Y Kuramitsu, DQ Lamb, J Meinecke, T Michel, F Miniati, M Notley, B Reville, D Ryu, S Sarkar, Y Sakawa, MP Selwood, J Squire, RHH Scott, P Tzeferacos, N Woolsey, AA Schekochihin, G Gregori

The properties of supersonic, compressible plasma turbulence determine the behavior of many terrestrial and astrophysical systems. In the interstellar medium and molecular clouds, compressible turbulence plays a vital role in star formation and the evolution of our galaxy. Observations of the density and velocity power spectra in the Orion B and Perseus molecular clouds show large deviations from those predicted for incompressible turbulence. Hydrodynamic simulations attribute this to the high Mach number in the interstellar medium (ISM), although the exact details of this dependence are not well understood. Here we investigate experimentally the statistical behavior of boundary-free supersonic turbulence created by the collision of two laser-driven high-velocity turbulent plasma jets. The Mach number dependence of the slopes of the density and velocity power spectra agree with astrophysical observations, and supports the notion that the turbulence transitions from being Kolmogorov-like at low Mach number to being more Burgers-like at higher Mach numbers.


First demonstration of ARC-accelerated proton beams at the National Ignition Facility

Physics of Plasmas 26 (2019)

D Mariscal, T Ma, SC Wilks, AJ Kemp, GJ Williams, P Michel, H Chen, PK Patel, BA Remington, M Bowers, L Pelz, MR Hermann, W Hsing, D Martinez, R Sigurdsson, M Prantil, A Conder, J Lawson, M Hamamoto, P Di Nicola, C Widmayer, D Homoelle, R Lowe-Webb, S Herriot, W Williams, D Alessi, D Kalantar, R Zacharias, C Haefner, N Thompson, T Zobrist, D Lord, N Hash, A Pak, N Lemos, M Tabak, C McGuffey, J Kim, FN Beg, MS Wei, P Norreys, A Morace, N Iwata, Y Sentoku, D Neely, GG Scott, K Flippo

© 2019 Author(s). New short-pulse kilojoule, Petawatt-class lasers, which have recently come online and are coupled to large-scale, many-beam long-pulse facilities, undoubtedly serve as very exciting tools to capture transformational science opportunities in high energy density physics. These short-pulse lasers also happen to reside in a unique laser regime: very high-energy (kilojoule), relatively long (multi-picosecond) pulse-lengths, and large (10s of micron) focal spots, where their use in driving energetic particle beams is largely unexplored. Proton acceleration via Target Normal Sheath Acceleration (TNSA) using the Advanced Radiographic Capability (ARC) short-pulse laser at the National Ignition Facility in the Lawrence Livermore National Laboratory is demonstrated for the first time, and protons of up to 18 MeV are measured using laser irradiation of >1 ps pulse-lengths and quasi-relativistic (∼10 18 W/cm 2 ) intensities. This is indicative of a super-ponderomotive electron acceleration mechanism that sustains acceleration over long (multi-picosecond) time-scales and allows for proton energies to be achieved far beyond what the well-established scalings of proton acceleration via TNSA would predict at these modest intensities. Furthermore, the characteristics of the ARC laser (large ∼100 μm diameter focal spot, flat spatial profile, multi-picosecond, relatively low prepulse) provide acceleration conditions that allow for the investigation of 1D-like particle acceleration. A high flux ∼ 50 J of laser-accelerated protons is experimentally demonstrated. A new capability in multi-picosecond particle-in-cell simulation is applied to model the data, corroborating the high proton energies and elucidating the physics of multi-picosecond particle acceleration.


Galaxies flowing in the oriented saddle frame of the cosmic web

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 483 (2019) 3227-3254

K Kraljic, C Pichon, Y Dubois, S Codis, C Cadiou, J Devriendt, M Musso, C Welker, S Arnouts, HS Hwang, C Laigle, S Peirani, A Slyz, M Treyer, D Vibert


The formation and evolution of low-surface-brightness galaxies

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 485 (2019) 796-818

G Martin, S Kaviraj, C Laigle, JEG Devriendt, RA Jackson, S Peirani, Y Dubois, C Pichon, A Slyz


Search for annihilating dark matter in the Sun with 3 years of IceCube data (vol 77, pg 146, 2017)

EUROPEAN PHYSICAL JOURNAL C 79 (2019) ARTN 214

MG Aartsen, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, D Altmann, K Andeen, T Anderson, I Ansseau, G Anton, M Archinger, C Arguelles, J Auffenberg, S Axani, X Bai, SW Barwick, V Baum, R Bay, JJ Beatty, JB Tjus, K-H Becker, S BenZvi, D Berley, E Bernardini, A Bernhard, DZ Besson, G Binder, D Bindig, M Bissok, E Blaufuss, S Blot, C Bohm, M Boerner, F Bos, D Bose, S Boeser, O Botner, J Braun, L Brayeur, H-P Bretz, S Bron, A Burgman, T Carver, M Casier, E Cheung, D Chirkin, A Christov, K Clark, L Classen, S Coenders, GH Collin, JM Conrad, DF Cowen, R Cross, M Day, JPAM de Andre, C De Clercq, E del Pino Rosendo, H Dembinski, S De Ridder, P Desiati, KD de Vries, G de Wasseige, M de With, T DeYoung, JC Diaz-Velez, V di Lorenzo, H Dujmovic, JP Dumm, M Dunkman, B Eberhardt, T Ehrhardt, B Eichmann, P Eller, S Euler, PA Evenson, S Fahey, AR Fazely, J Feintzeig, J Felde, K Filimonov, C Finley, S Flis, C-C Foesig, A Franckowiak, E Friedman, T Fuchs, TK Gaisser, J Gallagher, L Gerhardt, K Ghorbani, W Giang, L Gladstone, T Glauch, T Gluesenkamp, A Goldschmidt, JG Gonzalez, D Grant, Z Griffith, C Haack, A Hallgren, F Halzen, E Hansen, T Hansmann, K Hanson, D Hebecker, D Heereman, K Helbing, R Hellauer, S Hickford, J Hignight, GC Hill, KD Hoffman, R Hoffmann, K Hoshina, F Huang, M Huber, K Hultqvist, S In, A Ishihara, E Jacobi, GS Japaridze, M Jeong, K Jero, BJP Jones, W Kang, A Kappes, T Karg, A Karle, U Katz, M Kauer, A Keivani, JL Kelley, A Kheirandish, J Kim, M Kim, T Kintscher, J Kiryluk, T Kittler, SR Klein, G Kohnen, R Koirala, H Kolanoski, R Konietz, L Koepke, C Kopper, S Kopper, DJ Koskinen, M Kowalski, K Krings, M Kroll, G Krueckl, C Krueger, J Kunnen, S Kunwar, N Kurahashi, T Kuwabara, M Labare, JL Lanfranchi, MJ Larson, F Lauber, D Lennarz, M Lesiak-Bzdak, M Leuermann, L Lu, J Lunemann, J Madsen, G Maggi, KBM Mahn, S Mancina, M Mandelartz, R Maruyama, K Mase, R Maunu, F McNally, K Meagher, M Medici, M Meier, A Meli, T Menne, G Merino, T Meures, S Miarecki, T Montaruli, M Moulai, R Nahnhauer, U Naumann, G Neer, H Niederhausen, SC Nowicki, DR Nygren, AO Pollmann, A Olivas, A O'Murchadha, T Palczewski, H Pandya, DV Pankova, P Peiffer, O Penek, JA Pepper, CP de los Heros, D Pieloth, E Pinat, PB Price, GT Przybylski, M Quinnan, C Raab, L Raedel, M Rameez, K Rawlins, R Reimann, B Relethford, M Relich, E Resconi, W Rhode, M Richman, B Riedel, S Robertson, M Rongen, C Rott, T Ruhe, D Ryckbosch, D Rysewyk, L Sabbatini, SES Herrera, A Sandrock, J Sandroos, S Sarkar, K Satalecka, P Schlunder, T Schmidt, S Schoenen, S Schoeneberg, L Schumacher, D Seckel, S Seunarine, D Soldin, M Song, GM Spiczak, C Spiering, T Stanev, A Stasik, J Stettner, A Steuer, T Stezelberger, RG Stokstad, A Stossl, R Strom, NL Strotjohann, GW Sullivan, M Sutherland, H Taavola, I Taboada, J Tatar, F Tenholt, S Ter-Antonyan, A Terliuk, G Tesic, S Tilav, PA Toale, MN Tobin, S Toscano, D Tosi, M Tselengidou, A Turcati, E Unger, M Usner, J Vandenbroucke, N van Eijndhoven, S Vanheule, M van Rossem, J van Santen, M Vehring, M Voge, E Vogel, M Vraeghe, C Walck, A Wallace, M Wallraff, N Wandkowsky, C Weaver, MJ Weiss, C Wendt, S Westerhoff, BJ Whelan, S Wickmann, K Wiebe, CH Wiebusch, L Wille, DR Williams, L Wills, M Wolf, TR Wood, E Woolsey, K Woschnagg, DL Xu, XW Xu, Y Xu, JP Yanez, G Yodh, S Yoshida, M Zoll, I Collaboration


Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields

MNRAS (0)

H Katz, S Martin-Alvarez, J Devriendt, A Slyz, T Kimm

Despite their ubiquity, the origin of cosmic magnetic fields remains unknown. Various mechanisms have been proposed for their existence including primordial fields generated by inflation, or amplification and injection by compact astrophysical objects. Separating the potential impact of each magnetogenesis scenario on the magnitude and orientation of the magnetic field and their impact on gas dynamics may give insight into the physics that magnetised our Universe. In this work, we demonstrate that because the induction equation and solenoidal constraint are linear with $B$, the contribution from different sources of magnetic field can be separated in cosmological magnetohydrodynamics simulations and their evolution and influence on the gas dynamics can be tracked. Exploiting this property, we develop a magnetic field tracer algorithm for cosmological simulations that can track the origin and evolution of different components of the magnetic field. We present a suite of cosmological magnetohydrodynamical RAMSES simulations that employ this algorithm where the primordial field strength is varied to determine the contributions of the primordial and supernovae-injected magnetic fields to the total magnetic energy as a function of time and spatial location. We find that, for our specific model, the supernova-injected fields rarely penetrate far from haloes, despite often dominating the total magnetic energy in the simulations. The magnetic energy density from the supernova-injected field scales with density with a power-law slope steeper than 4/3 and often dominates the total magnetic energy inside of haloes. However, the star formation rates in our simulations are not affected by the presence of magnetic fields, for the ranges of primordial field strengths examined. These simulations represent a first demonstration of the magnetic field tracer algorithm (abridged).


The use of geometric effects in diagnosing ion density in ICF-related dot spectroscopy experiments

HIGH ENERGY DENSITY PHYSICS 30 (2019) 45-51

G Perez-Callejo, DA Liedahl, MB Schneider, SJ Rose, JS Wark


Maser radiation from collisionless shocks: application to astrophysical jets

HIGH POWER LASER SCIENCE AND ENGINEERING 7 (2019) ARTN e17

DC Speirs, K Ronald, ADR Phelps, ME Koepke, RA Cairns, A Rigby, F Cruz, RMGM Trines, R Bamford, BJ Kellett, B Albertazzi, JE Cross, F Fraschetti, P Graham, PM Kozlowski, Y Kuramitsu, F Miniati, T Morita, M Oliver, B Reville, Y Sakawa, S Sarkar, C Spindloe, M Koenig, LO Silva, DQ Lamb, P Tzeferacos, S Lebedev, G Gregori, R Bingham


Probing Cosmic Dawn: Modelling the Assembly History, SEDs, and Dust Content of Selected $z\sim9$ Galaxies

MNRAS (0)

H Katz, N Laporte, RS Ellis, J Devriendt, A Slyz

The presence of spectroscopically confirmed Balmer breaks in galaxy spectral energy distributions (SEDs) at $z>9$ provides one of the best probes of the assembly history of the first generations of stars in our Universe. Recent observations of the gravitationally lensed source, MACS 1149_JD1 (JD1), indicate that significant amounts of star formation likely occurred at redshifts as high as $z\simeq15$. The inferred stellar mass, dust mass, and assembly history of JD1, or any other galaxy at these redshifts that exhibits a strong Balmer break, can provide a strong test of our best theoretical models from high-resolution cosmological simulations. In this work, we present the results from a cosmological radiation-hydrodynamics simulation of the region surrounding a massive Lyman-break galaxy. For two of our most massive systems, we show that dust preferentially resides in the vicinity of the young stars thereby increasing the strength of the measured Balmer break such that the simulated SEDs are consistent with the photometry of JD1 and two other $z>9$ systems (GN-z10-3 and GN-z9-1) that have proposed Balmer breaks at high redshift. We find strong variations in the shape and luminosity of the SEDs of galaxies with nearly identical stellar and halo masses, indicating the importance of morphology, assembly history, and dust distribution in making inferences on the properties of individual galaxies at high redshifts. Our results stress the importance that dust may play in modulating the observable properties of galaxies, even at the extreme redshifts of $z>9$.


Astrophysical neutrinos and cosmic rays observed by IceCube

ADVANCES IN SPACE RESEARCH 62 (2018) 2902-2930

MG Aartsen, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, D Altmann, K Andeen, T Anderson, I Ansseau, G Anton, M Archinger, C Arguelles, J Auffenberg, S Axani, X Bai, SW Barwick, V Baum, R Bay, JJ Beatty, JB Tjus, K-H Becker, S BenZvi, D Berley, E Bernardini, A Bernhard, DZ Besson, G Binder, D Bindig, M Bissok, E Blaufuss, S Blot, C Bohm, M Boerner, F Bos, D Bose, S Boeser, O Botner, J Braun, L Brayeur, H-P Bretz, S Bron, A Burgman, T Carver, M Casier, E Cheung, D Chirkin, A Christov, K Clark, L Classen, S Coenders, GH Collin, JM Conrad, DF Cowen, R Cross, M Day, JPAM de Andre, C De Clercq, EDP Rosendo, H Dembinski, S De Ridder, P Desiati, KD de Vries, G de Wasseige, M de With, T de Young, JC Diaz-Velez, V di Lorenzo, H Dujmovic, JP Dumm, M Dunkman, B Eberhardt, T Ehrhardt, B Eichmann, P Eller, S Euler, PA Evenson, S Fahey, AR Fazely, J Feintzeig, J Felde, K Filimonov, C Finley, S Flis, C-C Foesig, A Franckowiak, E Friedman, T Fuchs, TK Gaisser, J Gallagher, L Gerhardt, K Ghorbani, W Giang, L Gladstone, T Glauch, T Gluesenkamp, A Goldschmidt, JG Gonzalez, D Grant, Z Griffith, C Haack, A Hallgren, F Halzen, E Hansen, T Hansmann, K Hanson, D Hebecker, D Heereman, K Helbing, R Hellauer, S Hickford, J Hignight, GC Hill, KD Hoffman, R Hoffmann, K Holzapfel, K Hoshina, F Huang, M Huber, K Hultqvist, S In, A Ishihara, E Jacobi, GS Japaridze, M Jeong, K Jero, BJP Jones, M Jurkovic, W Kang, A Kappes, T Karg, A Karle, U Katz, M Kauer, A Keivani, JL Kelley, A Kheirandish, J Kim, M Kim, T Kintscher, J Kiryluk, T Kittler, SR Klein, G Kohnen, R Koirala, H Kolanoski, R Konietz, L Koepke, C Kopper, S Kopper, DJ Koskinen, M Kowalski, K Krings, M Kroll, G Krueckl, C Kruger, J Kunnen, S Kunwar, N Kurahashi, T Kuwabara, M Labare, JL Lanfranchi, MJ Larson, F Lauber, D Lennarz, M Lesiak-Bzdak, M Leuermann, L Lu, J Lunemann, J Madsen, G Maggi, KBM Mahn, S Mancina, M Mandelartz, R Maruyama, K Mase, R Maunu, F McNally, K Meagher, M Medici, M Meier, A Meli, T Menne, G Merino, T Meures, S Miarecki, T Montaruli, M Moulai, R Nahnhauer, U Naumann, G Neer, H Niederhausen, SC Nowicki, DR Nygren, AO Pollmann, A Olivas, A O'Murchadha, T Palczewski, H Pandya, DV Pankova, P Peiffer, O Penek, JA Pepper, CP de los Heros, D Pielothu, E Pinat, PB Price, GT Przybylski, M Quinnan, C Raab, L Raedel, M Rameez, K Rawlins, R Reimann, B Relethford, M Relich, E Resconi, W Rhode, M Richman, B Riedel, S Robertson, M Rongen, C Rott, T Ruhe, D Ryckbosch, D Rysewyk, L Sabbatini, SES Herrera, A Sandrock, J Sandroos, S Sarkar, K Satalecka, P Schlunder, T Schmidt, S Schoenen, S Schoeneberg, L Schumacher, D Seckel, S Seunarine, D Soldin, M Song, GM Spiczak, C Spiering, T Stanev, A Stasik, J Stettner, A Steuer, T Stezelberger, RG Stokstad, A Stossl, R Strom, NL Strotjohann, GW Sullivan, M Sutherland, H Taavola, I Taboada, J Tatar, F Tenholti, S Ter-Antonyan, A Terliuk, G Tesic, S Tilav, PA Toale, MN Tobin, S Toscano, D Tosi, M Tselengidou, A Turcati, E Unger, M Usner, J Vandenbroucke, N van Eijndhoven, S Vanheule, M van Rossem, J van Santen, J Veenkamp, M Vehring, M Voge, E Vogel, M Vraeghe, C Walck, A Wallace, M Wallraff, N Wandkowsky, C Weaver, MJ Weiss, C Wendt, S Westerhoff, BJ Whelan, S Wickmann, K Wiebe, CH Wiebusch, L Wille, DR Williams, L Wills, M Wolf, TR Wood, E Woolsey, K Woschnagg, DL Xu, XW Xu, Y Xu, JP Yanez, G Yodh, S Yoshida, M Zoll

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