Dust properties, magnetic fields and grain alignment investigated via mid-IR polarimetry
Zenodo (2020)
Neutrino interaction classification with a convolutional neural network in the DUNE far detector
Physical Review D American Physical Society (APS) 102:9 (2020) 092003
Authors:
B Abi, R Acciarri, MA Acero, G Adamov, D Adams, M Adinolfi, Z Ahmad, J Ahmed, T Alion, S Alonso Monsalve, C Alt, J Anderson, C Andreopoulos, MP Andrews, F Andrianala, S Andringa, A Ankowski, M Antonova, S Antusch, A Aranda-Fernandez, A Ariga, LO Arnold, MA Arroyave, J Asaadi, A Aurisano, V Aushev, D Autiero, F Azfar, H Back, JJ Back, C Backhouse, P Baesso, L Bagby, R Bajou, S Balasubramanian, P Baldi, B Bambah, F Barao, G Barenboim, GJ Barker, W Barkhouse, C Barnes, G Barr, J Barranco Monarca, N Barros, JL Barrow, A Bashyal, V Basque, F Bay, JL Bazo Alba, JF Beacom, E Bechetoille, B Behera, L Bellantoni, G Bellettini, V Bellini, O Beltramello, D Belver, N Benekos, F Bento Neves, J Berger, S Berkman, P Bernardini, RM Berner, H Berns, S Bertolucci, M Betancourt, Y Bezawada, M Bhattacharjee, B Bhuyan, S Biagi, J Bian, M Biassoni, K Biery, B Bilki, M Bishai, A Bitadze, A Blake, B Blanco Siffert, FDM Blaszczyk, GC Blazey, E Blucher, J Boissevain, S Bolognesi, T Bolton, M Bonesini, M Bongrand, F Bonini, A Booth, C Booth, S Bordoni, A Borkum, T Boschi, N Bostan, P Bour, SB Boyd, D Boyden, J Bracinik, D Braga, D Brailsford, A Brandt, J Bremer, C Brew, E Brianne, SJ Brice, C Brizzolari, C Bromberg, G Brooijmans, J Brooke, A Bross, G Brunetti, N Buchanan, H Budd, D Caiulo, P Calafiura, J Calcutt, M Calin, S Calvez, E Calvo, L Camilleri, A Caminata, M Campanelli, D Caratelli, G Carini, B Carlus, P Carniti, I Caro Terrazas, H Carranza, A Castillo, C Castromonte, C Cattadori, F Cavalier, F Cavanna, S Centro, G Cerati, A Cervelli, A Cervera Villanueva, M Chalifour, C Chang, E Chardonnet, A Chatterjee, S Chattopadhyay, J Chaves, H Chen, M Chen, Y Chen, D Cherdack, C Chi, S Childress, A Chiriacescu, K Cho, S Choubey, A Christensen, D Christian, G Christodoulou, E Church, P Clarke, TE Coan, AG Cocco, JAB Coelho, E Conley, JM Conrad, M Convery, L Corwin, P Cotte, L Cremaldi, L Cremonesi, JI Crespo-Anadón, E Cristaldo, R Cross, C Cuesta, Y Cui, D Cussans, M Dabrowski, H da Motta, L Da Silva Peres, C David, Q David, GS Davies, S Davini, J Dawson, K De, RM De Almeida, P Debbins, I De Bonis, MP Decowski, A de Gouvêa, PC De Holanda, IL De Icaza Astiz, A Deisting, P De Jong, A Delbart, D Delepine, M Delgado, A Dell’Acqua, P De Lurgio, JRT de Mello Neto, DM DeMuth, S Dennis, C Densham, G Deptuch, A De Roeck, V De Romeri, JJ De Vries, R Dharmapalan, M Dias, F Diaz, JS Díaz, S Di Domizio, L Di Giulio, P Ding, L Di Noto, C Distefano, R Diurba, M Diwan, Z Djurcic, N Dokania, MJ Dolinski, L Domine, D Douglas, F Drielsma, D Duchesneau, K Duffy, P Dunne, T Durkin, H Duyang, O Dvornikov, DA Dwyer, AS Dyshkant, M Eads, D Edmunds, J Eisch, S Emery, A Ereditato, CO Escobar, L Escudero Sanchez, JJ Evans, E Ewart, AC Ezeribe, K Fahey, A Falcone, C Farnese, Y Farzan, J Felix, E Fernandez-Martinez, P Fernandez Menendez, F Ferraro, L Fields, A Filkins, F Filthaut, RS Fitzpatrick, W Flanagan, B Fleming, R Flight, J Fowler, W Fox, J Franc, K Francis, D Franco, J Freeman, J Freestone, J Fried, A Friedland, S Fuess, I Furic, AP Furmanski, A Gago, H Gallagher, A Gallego-Ros, N Gallice, V Galymov, E Gamberini, T Gamble, R Gandhi, R Gandrajula, S Gao, F García-Carballeira, D Garcia-Gamez, MÁ García-Peris, S Gardiner, D Gastler, G Ge, B Gelli, A Gendotti, S Gent, Z Ghorbani-Moghaddam, D Gibin, I Gil-Botella, C Girerd, AK Giri, D Gnani, O Gogota, M Gold, S Gollapinni, K Gollwitzer, RA Gomes, LV Gomez Bermeo, LS Gomez Fajardo, F Gonnella, JA Gonzalez-Cuevas, MC Goodman, O Goodwin, S Goswami, C Gotti, E Goudzovski, C Grace, M Graham, E Gramellini, R Gran, E Granados, A Grant, C Grant, D Gratieri, P Green, S Green, L Greenler, M Greenwood, J Greer, WC Griffith, M Groh, J Grudzinski, K Grzelak, W Gu, V Guarino, R Guenette, A Guglielmi, B Guo, KK Guthikonda, R Gutierrez, P Guzowski, MM Guzzo, S Gwon, A Habig, A Hackenburg, H Hadavand, R Haenni, A Hahn, J Haigh, J Haiston, T Hamernik, P Hamilton, J Han, K Harder, DA Harris, J Hartnell, T Hasegawa, R Hatcher, E Hazen, A Heavey, KM Heeger, J Heise, K Hennessy, S Henry, MA Hernandez Morquecho, K Herner, L Hertel, AS Hesam, J Hewes, A Higuera, T Hill, SJ Hillier, A Himmel, J Hoff, C Hohl, A Holin, E Hoppe, GA Horton-Smith, M Hostert, A Hourlier, B Howard, R Howell, J Huang, J Huang, J Hugon, G Iles, N Ilic, AM Iliescu, R Illingworth, A Ioannisian, R Itay, A Izmaylov, E James, B Jargowsky, F Jediny, C Jesùs-Valls, X Ji, L Jiang, S Jiménez, A Jipa, A Joglekar, C Johnson, R Johnson, B Jones, S Jones, CK Jung, T Junk, Y Jwa, M Kabirnezhad, A Kaboth, I Kadenko, F Kamiya, G Karagiorgi, A Karcher, M Karolak, Y Karyotakis, S Kasai, SP Kasetti, L Kashur, N Kazaryan, E Kearns, P Keener, KJ Kelly, E Kemp, W Ketchum, SH Kettell, M Khabibullin, A Khotjantsev, A Khvedelidze, D Kim, B King, B Kirby, M Kirby, J Klein, K Koehler, LW Koerner, S Kohn, PP Koller, M Kordosky, T Kosc, U Kose, VA Kostelecký, K Kothekar, F Krennrich, I Kreslo, Y Kudenko, VA Kudryavtsev, S Kulagin, J Kumar, R Kumar, C Kuruppu, V Kus, T Kutter, A Lambert, K Lande, CE Lane, K Lang, T Langford, P Lasorak, D Last, C Lastoria, A Laundrie, A Lawrence, I Lazanu, R LaZur, T Le, J Learned, P LeBrun, G Lehmann Miotto, R Lehnert, MA Leigui de Oliveira, M Leitner, M Leyton, L Li, S Li, SW Li, T Li, Y Li, H Liao, CS Lin, S Lin, A Lister, BR Littlejohn, J Liu, S Lockwitz, T Loew, M Lokajicek, I Lomidze, K Long, K Loo, D Lorca, T Lord, JM LoSecco, WC Louis, KB Luk, X Luo, N Lurkin, T Lux, VP Luzio, D MacFarland, AA Machado, P Machado, CT Macias, JR Macier, A Maddalena, P Madigan, S Magill, K Mahn, A Maio, JA Maloney, G Mandrioli, J Maneira, L Manenti, S Manly, A Mann, K Manolopoulos, M Manrique Plata, A Marchionni, W Marciano, D Marfatia, C Mariani, J Maricic, F Marinho, AD Marino, M Marshak, C Marshall, J Marshall, J Marteau, J Martin-Albo, N Martinez, DA Martinez Caicedo, S Martynenko, K Mason, A Mastbaum, M Masud, S Matsuno, J Matthews, C Mauger, N Mauri, K Mavrokoridis, R Mazza, A Mazzacane, E Mazzucato, E McCluskey, N McConkey, KS McFarland, C McGrew, A McNab, A Mefodiev, P Mehta, P Melas, M Mellinato, O Mena, S Menary, H Mendez, A Menegolli, G Meng, MD Messier, W Metcalf, M Mewes, H Meyer, T Miao, G Michna, T Miedema, J Migenda, R Milincic, W Miller, J Mills, C Milne, O Mineev, OG Miranda, S Miryala, CS Mishra, SR Mishra, A Mislivec, D Mladenov, I Mocioiu, K Moffat, N Moggi, R Mohanta, TA Mohayai, N Mokhov, J Molina, L Molina Bueno, A Montanari, C Montanari, D Montanari, LM Montano Zetina, J Moon, M Mooney, A Moor, D Moreno, B Morgan, C Morris, C Mossey, E Motuk, CA Moura, J Mousseau, W Mu, L Mualem, J Mueller, M Muether, S Mufson, F Muheim, A Muir, M Mulhearn, H Muramatsu, S Murphy, J Musser, J Nachtman, S Nagu, M Nalbandyan, R Nandakumar, D Naples, S Narita, D Navas-Nicolás, N Nayak, M Nebot-Guinot, L Necib, K Negishi, JK Nelson, J Nesbit, M Nessi, D Newbold, M Newcomer, D Newhart, R Nichol, E Niner, K Nishimura, A Norman, A Norrick, R Northrop, P Novella, JA Nowak, M Oberling, A Olivares Del Campo, A Olivier, Y Onel, Y Onishchuk, J Ott, L Pagani, S Pakvasa, O Palamara, S Palestini, JM Paley, M Pallavicini, C Palomares, E Pantic, V Paolone, V Papadimitriou, R Papaleo, A Papanestis, S Paramesvaran, S Parke, Z Parsa, M Parvu, S Pascoli, L Pasqualini, J Pasternak, J Pater, C Patrick, L Patrizii, RB Patterson, SJ Patton, T Patzak, A Paudel, B Paulos, L Paulucci, Z Pavlovic, G Pawloski, D Payne, V Pec, SJM Peeters, Y Penichot, E Pennacchio, A Penzo, OLG Peres, J Perry, D Pershey, G Pessina, G Petrillo, C Petta, R Petti, F Piastra, L Pickering, F Pietropaolo, J Pillow, J Pinzino, R Plunkett, R Poling, X Pons, N Poonthottathil, S Pordes, M Potekhin, R Potenza, BVKS Potukuchi, J Pozimski, M Pozzato, S Prakash, T Prakash, S Prince, G Prior, D Pugnere, K Qi, X Qian, JL Raaf, R Raboanary, V Radeka, J Rademacker, B Radics, A Radovic, A Rafique, E Raguzin, M Rai, M Rajaoalisoa, I Rakhno, HT Rakotondramanana, L Rakotondravohitra, YA Ramachers, R Rameika, MA Ramirez Delgado, B Ramson, A Rappoldi, G Raselli, P Ratoff, S Ravat, H Razafinime, JS Real, B Rebel, D Redondo, M Reggiani-Guzzo, T Rehak, J Reichenbacher, SD Reitzner, A Renshaw, S Rescia, F Resnati, A Reynolds, G Riccobene, LCJ Rice, K Rielage, Y Rigaut, D Rivera, L Rochester, M Roda, P Rodrigues, MJ Rodriguez Alonso, J Rodriguez Rondon, AJ Roeth, H Rogers, S Rosauro-Alcaraz, M Rossella, J Rout, S Roy, A Rubbia, C Rubbia, B Russell, J Russell, D Ruterbories, R Saakyan, S Sacerdoti, T Safford, N Sahu, P Sala, N Samios, MC Sanchez, DA Sanders, D Sankey, S Santana, M Santos-Maldonado, N Saoulidou, P Sapienza, C Sarasty, I Sarcevic, G Savage, V Savinov, A Scaramelli, A Scarff, A Scarpelli, T Schaffer, H Schellman, P Schlabach, D Schmitz, K Scholberg, A Schukraft, E Segreto, J Sensenig, I Seong, A Sergi, F Sergiampietri, D Sgalaberna, MH Shaevitz, S Shafaq, M Shamma, HR Sharma, R Sharma, T Shaw, C Shepherd-Themistocleous, S Shin, D Shooltz, R Shrock, L Simard, N Simos, J Sinclair, G Sinev, J Singh, J Singh, V Singh, R Sipos, FW Sippach, G Sirri, A Sitraka, K Siyeon, D Smargianaki, A Smith, A Smith, E Smith, P Smith, J Smolik, M Smy, P Snopok, M Soares Nunes, H Sobel, M Soderberg, CJ Solano Salinas, S Söldner-Rembold, N Solomey, V Solovov, WE Sondheim, M Sorel, J Soto-Oton, A Sousa, K Soustruznik, F Spagliardi, M Spanu, J Spitz, NJC Spooner, K Spurgeon, R Staley, M Stancari, L Stanco, HM Steiner, J Stewart, B Stillwell, J Stock, F Stocker, T Stokes, M Strait, T Strauss, S Striganov, A Stuart, D Summers, A Surdo, V Susic, L Suter, CM Sutera, R Svoboda, B Szczerbinska, AM Szelc, R Talaga, HA Tanaka, B Tapia Oregui, A Tapper, S Tariq, E Tatar, R Tayloe, AM Teklu, M Tenti, K Terao, CA Ternes, F Terranova, G Testera, A Thea, JL Thompson, C Thorn, SC Timm, A Tonazzo, M Torti, M Tortola, F Tortorici, D Totani, M Toups, C Touramanis, J Trevor, WH Trzaska, YT Tsai, Z Tsamalaidze, KV Tsang, N Tsverava, S Tufanli, C Tull, E Tyley, M Tzanov, MA Uchida, J Urheim, T Usher, MR Vagins, P Vahle, GA Valdiviesso, E Valencia, Z Vallari, JWF Valle, S Vallecorsa, R Van Berg, RG Van de Water, D Vanegas Forero, F Varanini, D Vargas, G Varner, J Vasel, G Vasseur, K Vaziri, S Ventura, A Verdugo, S Vergani, MA Vermeulen, M Verzocchi, H Vieira de Souza, C Vignoli, C Vilela, B Viren, T Vrba, T Wachala, AV Waldron, M Wallbank, H Wang, J Wang, Y Wang, Y Wang, K Warburton, D Warner, M Wascko, D Waters, A Watson, P Weatherly, A Weber, M Weber, H Wei, A Weinstein, D Wenman, M Wetstein, MR While, A White, LH Whitehead, D Whittington, MJ Wilking, C Wilkinson, Z Williams, F Wilson, RJ Wilson, J Wolcott, T Wongjirad, K Wood, L Wood, E Worcester, M Worcester, C Wret, W Wu, W Wu, Y Xiao, G Yang, T Yang, N Yershov, K Yonehara, T Young, B Yu, J Yu, R Zaki, J Zalesak, L Zambelli, B Zamorano, A Zani, L Zazueta, GP Zeller, J Zennamo, K Zeug, C Zhang, M Zhao, E Zhivun, G Zhu, ED Zimmerman, M Zito, S Zucchelli, J Zuklin, V Zutshi, R ZwaskaProspects for characterizing the haziest sub-Neptune exoplanets with high-resolution spectroscopy
Astronomical Journal IOP Publishing 160:5 (2020) 160-198
Authors:
Callie E Hood, Jonathan J Fortney, Michael R Line, Emily C Martin, Caroline V Morley, Jayne L Birkby, Zafar Rustamkulov, Roxana E Lupu, Richard S FreedmanAbstract:
Observations to characterize planets larger than Earth but smaller than Neptune have led to largely inconclusive interpretations at low spectral resolution due to hazes or clouds that obscure molecular features in their spectra. However, here we show that high-resolution spectroscopy (R ~ 25,000–100,000) enables one to probe the regions in these atmospheres above the clouds where the cores of the strongest spectral lines are formed. We present models of transmission spectra for a suite of GJ 1214b–like planets with thick photochemical hazes covering 1–5 μm at a range of resolutions relevant to current and future ground-based spectrographs. Furthermore, we compare the utility of the cross-correlation function that is typically used with a more formal likelihood-based approach, finding that only the likelihood-based method is sensitive to the presence of haze opacity. We calculate the signal-to-noise ratio (S/N) of these spectra, including telluric contamination, Required to robustly detect a host of molecules such as CO, CO2, H2O, and CH4 and photochemical products like HCN as a function of wavelength range and spectral resolution. Spectra in the M band require the lowest S/Nres to detect multiple molecules simultaneously. CH4 is only observable for the coolest models (T eff = 412 K) and only in the L band. We quantitatively assess how these requirements compare to what is achievable with current and future instruments, demonstrating that characterization of small cool worlds with ground-based high-resolution spectroscopy is well within reach.First Principle Simulator of a Stochastically Varying Image Plane for Photon-counting High Contrast Applications
Publications of the Astronomical Society of the Pacific IOP Publishing 132:1016 (2020) 104503
Authors:
Rupert H Dodkins, Kristina K Davis, Briley Lewis, Sumedh Mahashabde, Benjamin A Mazin, Isabel A Lipartito, Neelay Fruitwala, Kieran O’Brien, Niranjan ThatteLong-baseline neutrino oscillation physics potential of the DUNE experiment
European Physical Journal C Springer Nature 80:10 (2020) 978