Volume IV. The DUNE far detector single-phase technology

Journal of Instrumentation IOP Publishing 15:08 (2020) t08010-t08010

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, M 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, G Barker, W Barkhouse, C Barnes, G Barr, J Barranco Monarca, N Barros, JL Barrow, A Bashyal, V Basque, F Bay, J 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, F Blaszczyk, G 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, S 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, J Coelho, E Conley, J 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, Q David, GS Davies, S Davini, J Dawson, K De, RM De Almeida, P Debbins, I De Bonis, M Decowski, A De Gouvea, PC De Holanda, IL De Icaza Astiz, A Deisting, P De Jong, A Delbart, D Delepine, M Delgado, A Dell'Acqua, P De Lurgio, JR De Mello Neto, DM DeMuth, S Dennis, C Densham, G Deptuch, A De Roeck, V De Romeri, J De Vries, R Dharmapalan, M Dias, F Diaz, J Diaz, S Di Domizio, L Di Giulio, P Ding, L Di Noto, C Distefano, R Diurba, M Diwan, Z Djurcic, N Dokania, M Dolinski, L Domine, D Douglas, F Drielsma, D Duchesneau, K Duffy, P Dunne, T Durkin, H Duyang, O Dvornikov, D Dwyer, A Dyshkant, M Eads, D Edmunds, J Eisch, S Emery, A Ereditato, C 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, 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, A Giri, D Gnani, O Gogota, M Gold, S Gollapinni, K Gollwitzer, RA Gomes, L Gomez Bermeo, LS Gomez Fajardo, F Gonnella, J 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, C Griffith, M Groh, J Grudzinski, K Grzelak, W Gu, V Guarino, R Guenette, A Guglielmi, B Guo, K 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, K Hennessy, S Henry, M Hernandez Morquecho, K Herner, L Hertel, AS Hesam, J Hewes, A Higuera Pichardo, 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, AM Iliescu, R Illingworth, A Ioannisian, R Itay, A Izmaylov, E James, B Jargowsky, F Jediny, C Jesús-Valls, X Ji, L Jiang, S Jiménez, A Jipa, A Joglekar, C Johnson, R Johnson, B Jones, S Jones, C 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, S 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, V Kostelecky, K Kothekar, F Krennrich, I Kreslo, Y Kudenko, V 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, M Leigui de Oliveira, M Leitner, M Leyton, L Li, S Li, S Li, T Li, Y Li, H Liao, C 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, J LoSecco, WC Louis, K Luk, X Luo, N Lurkin, T Lux, VP Luzio, D MacFarland, A Machado, P Machado, C Macias, J Macier, A Maddalena, P Madigan, S Magill, K Mahn, A Maio, JA Maloney, G Mandrioli, JC 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, M 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, C Mishra, S Mishra, A Mislivec, D Mladenov, I Mocioiu, K Moffat, N Moggi, R Mohanta, TA Mohayai, N Mokhov, JA 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, 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, S Patton, T Patzak, A Paudel, B Paulos, L Paulucci, Z Pavlovic, G Pawloski, D Payne, V Pec, SJ Peeters, Y Penichot, E Pennacchio, A Penzo, OL Peres, J Perry, D Pershey, G Pessina, G Petrillo, C Petta, R Petti, F Piastra, L Pickering, F Pietropaolo, J Pillow, R Plunkett, R Poling, X Pons, N Poonthottathil, S Pordes, M Potekhin, R Potenza, BV Potukuchi, J Pozimski, M Pozzato, S Prakash, T Prakash, S Prince, G Prior, D Pugnere, K Qi, X Qian, J Raaf, R Raboanary, V Radeka, J Rademacker, B Radics, A Rafique, E Raguzin, M Rai, M Rajaoalisoa, I Rakhno, H Rakotondramanana, L Rakotondravohitra, Y Ramachers, R Rameika, M Ramirez Delgado, B Ramson, A Rappoldi, G Raselli, P Ratoff, S Ravat, H Razafinime, J Real, B Rebel, D Redondo, M Reggiani-Guzzo, T Rehak, J Reichenbacher, SD Reitzner, A Renshaw, S Rescia, F Resnati, A Reynolds, G Riccobene, LC Rice, K Rielage, Y Rigaut, D Rivera, L Rochester, M Roda, P Rodrigues, M Rodriguez Alonso, J Rodriguez Rondon, A 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, M 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, M 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, F 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, NJ Spooner, K Spurgeon, R Staley, M Stancari, L Stanco, H 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, C Sutera, R Svoboda, B Szczerbinska, A Szelc, R Talaga, H Tanaka, B Tapia Oregui, A Tapper, S Tariq, E Tatar, R Tayloe, A Teklu, M Tenti, K Terao, CA Ternes, F Terranova, G Testera, A Thea, JL Thompson, C Thorn, S Timm, A Tonazzo, M Torti, M Tortola, F Tortorici, D Totani, M Toups, C Touramanis, J Trevor, WH Trzaska, YT Tsai, Z Tsamalaidze, K Tsang, N Tsverava, S Tufanli, C Tull, E Tyley, M Tzanov, MA Uchida, J Urheim, T Usher, M Vagins, P Vahle, G Valdiviesso, E Valencia, Z Vallari, JW 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, J Zalesak, L Zambelli, B Zamorano, A Zani, L Zazueta, G Zeller, J Zennamo, K Zeug, C Zhang, M Zhao, E Zhivun, G Zhu, ED Zimmerman, M Zito, S Zucchelli, J Zuklin, V Zutshi, R Zwaska

Resolved observations at 31 GHz of spinning dust emissivity variations in rho Oph

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 495:3 (2020) 3482-3493

Authors:

Carla Arce-Tord, Matias Vidal, Simon Casassus, Miguel Carcamo, Clive Dickinson, Brandon S Hensley, Ricardo Genova-Santos, J Richard Bond, Michael E Jones, Anthony CS Readhead, Angela C Taylor, J Anton Zensus

Abstract:

© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. The ρ Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the cosmic background imager (CBI). Here, we present 4.5 arcmin observations with CBI 2 that confirm 31 GHz emission from ρ Oph W, the PDR exposed to B-Type star HD 147889, and highlight the absence of signal from S1, the brightest IR nebula in the complex. In order to quantify an association with dust-related emission mechanisms, we calculated correlations at different angular resolutions between the 31 GHz map and proxies for the column density of IR emitters, dust radiance, and optical depth templates. We found that the 31 GHz emission correlates best with the PAH column density tracers, while the correlation with the dust radiance improves when considering emission that is more extended (from the shorter baselines), suggesting that the angular resolution of the observations affects the correlation results. A proxy for the spinning dust emissivity reveals large variations within the complex, with a dynamic range of 25 at 3σ and a variation by a factor of at least 23, at 3σ, between the peak in ρ Oph W and the location of S1, which means that environmental factors are responsible for boosting spinning dust emissivities locally.

The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 249:1 (2020) ARTN 3

Authors:

Romina Ahumada, Carlos Allende Prieto, Andres Almeida, Friedrich Anders, Scott F Anderson, Brett H Andrews, Borja Anguiano, Riccardo Arcodia, Eric Armengaud, Marie Aubert, Santiago Avila, Vladimir Avila-Reese, Carles Badenes, Christophe Balland, Kat Barger, Jorge K Barrera-Ballesteros, Sarbani Basu, Julian Bautista, Rachael L Beaton, Timothy C Beers, B Izamar T Benavides, Chad F Bender, Mariangela Bernardi, Matthew Bershady, Florian Beutler, Christian Moni Bidin, Jonathan Bird, Dmitry Bizyaev, Guillermo A Blanc, Michael R Blanton, Mederic Boquien, Jura Borissova, Jo Bovy, Wn Brandt, Jonathan Brinkmann, Joel R Brownstein, Kevin Bundy, Martin Bureau, Adam Burgasser, Etienne Burtin, Mariana Cano-Diaz, Raffaella Capasso, Michele Cappellari, Ricardo Carrera, Solene Chabanier, William Chaplin, Michael Chapman, Brian Cherinka, Cristina Chiappini, Peter Doohyun Choi

Abstract:

© 2020. The Author(s). Published by the American Astronomical Society.. This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17).

Cold molecular gas and PAH emission in the nuclear and circumnuclear regions of Seyfert galaxies

Astronomy & Astrophysics EDP Sciences 639 (2020) a43

Authors:

A Alonso-Herrero, M Pereira-Santaella, D Rigopoulou, I García-Bernete, S García-Burillo, AJ Domínguez-Fernández, F Combes, RI Davies, T Díaz-Santos, D Esparza-Arredondo, O González-Martín, A Hernán-Caballero, EKS Hicks, SF Hönig, NA Levenson, C Ramos Almeida, PF Roche, D Rosario

K-CLASH: Strangulation and ram pressure stripping in galaxy cluster members at 0.3 < z < 0.6

Monthly Notices of the Royal Astronomical Society Oxford University Press 496:3 (2020) 3841-3861

Authors:

Sam P Vaughan, Alfred L Tiley, Roger L Davies, Laura J Prichard, Scott M Croom, Martin Bureau, John P Stott, Andrew Bunker, Michele Cappellari, Behzad Ansarinejad, Matt J Jarvis

Abstract:

Galaxy clusters have long been theorized to quench the star formation of their members. This study uses integral-field unit observations from the K-band MultiObject Spectrograph (KMOS) – Cluster Lensing And Supernova survey with Hubble (CLASH) survey (K-CLASH) to search for evidence of quenching in massive galaxy clusters at redshifts 0.3 < z < 0.6. We first construct mass-matched samples of exclusively star-forming cluster and field galaxies, then investigate the spatial extent of their H α emission and study their interstellar medium conditions using emission line ratios. The average ratio of H α half-light radius to optical half-light radius ($r_{\mathrm{e}, {\rm {H}\,\alpha }}/r_{\mathrm{e}, R_{\mathrm{c} } }$) for all galaxies is 1.14 ± 0.06, showing that star formation is taking place throughout stellar discs at these redshifts. However, on average, cluster galaxies have a smaller $r_{\mathrm{e}, {\rm {H}\alpha }}/r_{\mathrm{e}, R_{\mathrm{c} } }$ ratio than field galaxies: 〈$r_{\mathrm{e}, {\rm {H}\alpha }}/r_{\mathrm{e}, R_{\mathrm{c} } }$〉 = 0.96 ± 0.09 compared to 1.22 ± 0.08 (smaller at a 98 per cent credibility level). These values are uncorrected for the wavelength difference between H α emission and Rc-band stellar light but implementing such a correction only reinforces our results. We also show that whilst the cluster and field samples follow indistinguishable mass–metallicity (MZ) relations, the residuals around the MZ relation of cluster members correlate with cluster-centric distance; galaxies residing closer to the cluster centre tend to have enhanced metallicities (significant at the 2.6σ level). Finally, in contrast to previous studies, we find no significant differences in electron number density between the cluster and field galaxies. We use simple chemical evolution models to conclude that the effects of disc strangulation and ram-pressure stripping can quantitatively explain our observations.