Gravitational lens models based on Submillimeter Array Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.-selected strongly lensed sub-millimeter galaxies at z > 1.5
Astrophysical Journal 779:1 (2013)
Authors:
RS Bussmann, I Pérez-Fournon, S Amber, J Calanog, MA Gurwell, H Dannerbauer, F De Bernardis, H Fu, AI Harris, M Krips, A Lapi, R Maiolino, A Omont, D Riechers, J Wardlow, AJ Baker, M Birkinshaw, J Bock, N Bourne, DL Clements, A Cooray, G De Zotti, L Dunne, S Dye, S Eales, D Farrah, R Gavazzi, J González Nuevo, R Hopwood, E Ibar, RJ Ivison, N Laporte, S Maddox, P Martínez-Navajas, M Michalowski, M Negrello, SJ Oliver, IG Roseboom, D Scott, S Serjeant, AJ Smith, M Smith, A Streblyanska, E Valiante, P Van Der Werf, A Verma, JD Vieira, L Wang, D WilnerAbstract:
Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub-)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution imaging and Gemini-South and Multiple Mirror Telescope optical spectroscopy of strong lens candidates discovered in the two widest extragalactic surveys conducted by the Herschel Space Observatory: the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) and the Herschel Multi-tiered Extragalactic Survey (HerMES). From a sample of 30 Herschel sources with S 500 > 100 mJy, 21 are strongly lensed (i.e., multiply imaged), 4 are moderately lensed (i.e., singly imaged), and the remainder require additional data to determine their lensing status. We apply a visibility-plane lens modeling technique to the SMA data to recover information about the masses of the lenses as well as the intrinsic (i.e., unlensed) sizes (r half) and far-infrared luminosities (L FIR) of the lensed submillimeter galaxies (SMGs). The sample of lenses comprises primarily isolated massive galaxies, but includes some groups and clusters as well. Several of the lenses are located at z lens > 0.7, a redshift regime that is inaccessible to lens searches based on Sloan Digital Sky Survey spectroscopy. The lensed SMGs are amplified by factors that are significantly below statistical model predictions given the 500 μm flux densities of our sample. We speculate that this may reflect a deficiency in our understanding of the intrinsic sizes and luminosities of the brightest SMGs. The lensed SMGs span nearly one decade in L FIR (median L FIR = 7.9 × 10 12 L ) and two decades in FIR luminosity surface density (median ΣFIR = 6.0 × 1011 L kpc-2). The strong lenses in this sample and others identified via (sub-)mm surveys will provide a wealth of information regarding the astrophysics of galaxy formation and evolution over a wide range in redshift. © 2013. The American Astronomical Society. All rights reserved..Uncovering the deeply embedded active galactic nucleus activity in the nuclear regions of the interacting galaxy Arp 299
Astrophysical Journal Letters 779:1 (2013)
Authors:
A Alonso-Herrero, PF Roche, P Esquej, O González-Martín, M Pereira-Santaella, C Ramos Almeida, NA Levenson, C Packham, A Asensio Ramos, RE Mason, JM Rodríguez Espinosa, C Alvarez, L Colina, I Aretxaga, T Díaz-Santos, E Perlman, CM TelescoAbstract:
We present mid-infrared (MIR) 8-13 μm spectroscopy of the nuclear regions of the interacting galaxy Arp 299 (IC 694+NGC 3690) obtained with CanariCam (CC) on the 10.4 m Gran Telescopio Canarias (GTC). The high angular resolution (∼0.″3-0.″6) of the data allows us to probe nuclear physical scales between 60 and 120 pc, which is a factor of 10 improvement over previous MIR spectroscopic observations of this system. The GTC/CC spectroscopy displays evidence of deeply embedded active galactic nucleus (AGN) activity in both nuclei. The GTC/CC nuclear spectrum of NGC 3690/Arp 299-B1 can be explained as emission from AGN-heated dust in a clumpy torus with both a high covering factor and high extinction along the line of sight. The estimated bolometric luminosity of the AGN in NGC 3690 is 3.2 ± 0.6 × 1044 erg s-1. The nuclear GTC/CC spectrum of IC 694/Arp 299-A shows 11.3 μm polycyclic aromatic hydrocarbon emission stemming from a deeply embedded (AV ∼ 24 mag) region of less than 120 pc in size. There is also a continuum-emitting dust component. If associated with the putative AGN in IC 694, we estimate that it would be approximately five times less luminous than the AGN in NGC 3690. The presence of dual AGN activity makes Arp 299 a good example to study such phenomena in the early coalescence phase of interacting galaxies. © 2013. The American Astronomical Society. All rights reserved.Herschel observations and a model for IRAS 08572+3915: A candidate for the most luminous infrared galaxy in the local (z < 0.2) Universe
Monthly Notices of the Royal Astronomical Society: Letters 437:1 (2013)
Authors:
A Efstathiou, C Pearson, D Farrah, D Rigopoulou, J Gracía-Carpio, A Verma, HWW Spoon, J Afonso, J Bernard-Salas, DL Clements, A Cooray, D Cormier, M Etxaluze, J Fischer, E Gonźalez-Alfonso, P Hurley, V Lebouteiller, SJ Oliver, M Rowan-Robinson, E SturmAbstract:
We present Herschel photometry and spectroscopy, carried out as part of the Herschel ultraluminous infrared galaxy (ULIRG) survey, and a model for the infrared to submillimetre emission of the ULIRG IRAS 08572+3915. This source shows one of the deepest known silicate absorption features and no polycyclic aromatic hydrocarbon emission. The model suggests that this object is powered by an active galactic nucleus (AGN) with a fairly smooth torus viewed almost edge-on and a very young starburst. According to our model, the AGN contributes about 90 per cent of the total luminosity of 1.1 × 1013 L⊙, which is about a factor of 5 higher than previous estimates. The large correction of the luminosity is due to theanisotropy of the emission of the best-fitting torus. Similar corrections may be necessary for other local and high-z analogues. This correction implies that IRAS 08572+3915 at a redshift of 0.058 35 may be the nearest hyperluminous infrared galaxy and probably the most luminous infrared galaxy in the local (z < 0.2) Universe. IRAS 08572+3915 shows a low ratio of [C II] to IR luminosity (log L[C II]/LIR < -3.8) and a [OI]63 μm to [CII]158 μm line ratio of about 1 that supports the model presented in this Letter ©2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.Search for charginos nearly mass degenerate with the lightest neutralino based on a disappearing-track signature in pp collisions at (s)=8 TeV with the ATLAS detector
Physical Review D American Physical Society (APS) 88:11 (2013) 112006
Authors:
G Aad, T Abajyan, B Abbott, J Abdallah, S Abdel Khalek, O Abdinov, R Aben, B Abi, M Abolins, OS AbouZeid, H Abramowicz, H Abreu, Y Abulaiti, BS Acharya, L Adamczyk, DL Adams, TN Addy, J Adelman, S Adomeit, T Adye, S Aefsky, T Agatonovic-Jovin, JA Aguilar-Saavedra, M Agustoni, SP Ahlen, A Ahmad, F Ahmadov, M Ahsan, G Aielli, TPA Åkesson, G Akimoto, AV Akimov, MA Alam, J Albert, S Albrand, MJ Alconada Verzini, M Aleksa, IN Aleksandrov, F Alessandria, C Alexa, G Alexander, G Alexandre, T Alexopoulos, M Alhroob, M Aliev, G Alimonti, L Alio, J Alison, BMM Allbrooke, LJ Allison, PP Allport, SE Allwood-Spiers, J Almond, A Aloisio, R Alon, A Alonso, F Alonso, A Altheimer, B Alvarez Gonzalez, MG Alviggi, K Amako, Y Amaral Coutinho, C Amelung, VV Ammosov, SP Amor Dos Santos, A Amorim, S Amoroso, N Amram, G Amundsen, C Anastopoulos, LS Ancu, N Andari, T Andeen, CF Anders, G Anders, KJ Anderson, A Andreazza, V Andrei, XS Anduaga, S Angelidakis, P Anger, A Angerami, F Anghinolfi, AV Anisenkov, N Anjos, A Annovi, A Antonaki, M Antonelli, A Antonov, J Antos, F Anulli, M Aoki, L Aperio Bella, R Apolle, G Arabidze, I Aracena, Y Arai, ATH Arce, S Arfaoui, J-F Arguin, S Argyropoulos, E Arik, M Arik, AJ Armbruster, O Arnaez, V Arnal, O Arslan, A Artamonov, G Artoni, S Asai, N Asbah, S Ask, B Åsman, L Asquith, K Assamagan, R Astalos, A Astbury, M Atkinson, NB Atlay, B Auerbach, E Auge, K Augsten, M Aurousseau, G Avolio, G Azuelos, Y Azuma, MA Baak, C Bacci, AM Bach, H Bachacou, K Bachas, M Backes, M Backhaus, J Backus Mayes, E Badescu, P Bagiacchi, P Bagnaia, Y Bai, DC Bailey, T Bain, JT Baines, OK Baker, S Baker, P Balek, F Balli, E Banas, Sw Banerjee, D Banfi, A Bangert, V Bansal, HS Bansil, L Barak, SP Baranov, T Barber, EL Barberio, D Barberis, M Barbero, DY Bardin, T Barillari, M Barisonzi, T Barklow, N Barlow, BM Barnett, RM Barnett, A Baroncelli, G Barone, AJ Barr, F Barreiro, J Barreiro Guimarães da Costa, R Bartoldus, AE Barton, V Bartsch, A Bassalat, A Basye, RL Bates, L Batkova, JR Batley, M Battistin, F Bauer, HS Bawa, T Beau, PH Beauchemin, R Beccherle, P Bechtle, HP Beck, K Becker, S Becker, M Beckingham, AJ Beddall, A Beddall, S Bedikian, VA Bednyakov, CP Bee, LJ Beemster, TA Beermann, M Begel, K Behr, C Belanger-Champagne, PJ Bell, WH Bell, G Bella, L Bellagamba, A Bellerive, M Bellomo, A Belloni, OL Beloborodova, K Belotskiy, O Beltramello, O Benary, D Benchekroun, K Bendtz, N Benekos, Y Benhammou, E Benhar Noccioli, JA Benitez Garcia, DP Benjamin, JR Bensinger, K Benslama, S Bentvelsen, D Berge, E Bergeaas Kuutmann, N Berger, F Berghaus, E Berglund, J Beringer, C Bernard, P Bernat, R Bernhard, C Bernius, FU Bernlochner, T Berry, P Berta, C Bertella, F Bertolucci, MI Besana, GJ Besjes, O Bessidskaia, N Besson, S Bethke, W Bhimji, RM Bianchi, L Bianchini, M Bianco, O Biebel, SP Bieniek, K Bierwagen, J Biesiada, M Biglietti, J Bilbao De Mendizabal, H Bilokon, M Bindi, S Binet, A Bingul, C Bini, B Bittner, CW Black, JE Black, KM Black, D Blackburn, RE Blair, J-B Blanchard, T Blazek, I Bloch, C Blocker, J Blocki, W Blum, U Blumenschein, GJ Bobbink, VS Bobrovnikov, SS Bocchetta, A Bocci, CR Boddy, M Boehler, J Boek, TT Boek, N Boelaert, JA Bogaerts, AG Bogdanchikov, A Bogouch, C Bohm, J Bohm, V Boisvert, T Bold, V Boldea, AS Boldyrev, NM Bolnet, M Bomben, M Bona, M Boonekamp, S Bordoni, C Borer, A Borisov, G Borissov, M Borri, S Borroni, J Bortfeldt, V Bortolotto, K Bos, D Boscherini, M Bosman, H Boterenbrood, J Bouchami, J Boudreau, EV Bouhova-Thacker, D Boumediene, C Bourdarios, N Bousson, S Boutouil, A Boveia, J Boyd, IR Boyko, I Bozovic-Jelisavcic, J Bracinik, P Branchini, A Brandt, G Brandt, O Brandt, U Bratzler, B Brau, JE Brau, HM Braun, SF Brazzale, B Brelier, K Brendlinger, R Brenner, S Bressler, TM Bristow, D Britton, FM Brochu, I Brock, R Brock, F Broggi, C Bromberg, J Bronner, G Brooijmans, T Brooks, WK Brooks, J Brosamer, E Brost, G Brown, J Brown, PA Bruckman de Renstrom, D Bruncko, R Bruneliere, S Brunet, A Bruni, G Bruni, M Bruschi, L Bryngemark, T Buanes, Q Buat, F Bucci, J Buchanan, P Buchholz, RM Buckingham, AG Buckley, SI Buda, IA Budagov, B Budick, F Buehrer, L Bugge, O Bulekov, AC Bundock, M Bunse, H Burckhart, S Burdin, T Burgess, S Burke, I Burmeister, E Busato, V Büscher, P Bussey, CP Buszello, B Butler, JM Butler, AI Butt, CM Buttar, JM Butterworth, W Buttinger, A Buzatu, M Byszewski, S Cabrera Urbán, D Caforio, O Cakir, P Calafiura, G Calderini, P Calfayan, R Calkins, LP Caloba, R Caloi, D Calvet, S Calvet, R Camacho Toro, P Camarri, D Cameron, LM Caminada, R Caminal Armadans, S Campana, M Campanelli, V Canale, F Canelli, A Canepa, J Cantero, R Cantrill, T Cao, MDM Capeans Garrido, I Caprini, M Caprini, M Capua, R Caputo, R Cardarelli, T Carli, G Carlino, L Carminati, S Caron, E Carquin, GD Carrillo-Montoya, AA Carter, JR Carter, J Carvalho, D Casadei, MP Casado, C Caso, E Castaneda-Miranda, A Castelli, V Castillo Gimenez, NF Castro, P Catastini, A Catinaccio, JR Catmore, A Cattai, G Cattani, S Caughron, V Cavaliere, D Cavalli, M Cavalli-Sforza, V Cavasinni, F Ceradini, B Cerio, AS Cerqueira, A Cerri, L Cerrito, F Cerutti, A Cervelli, SA Cetin, A Chafaq, D Chakraborty, I Chalupkova, K Chan, P Chang, B Chapleau, JD Chapman, JW Chapman, D Charfeddine, DG Charlton, V Chavda, CA Chavez Barajas, S Cheatham, S Chekanov, SV Chekulaev, GA Chelkov, MA Chelstowska, C Chen, H Chen, K Chen, S Chen, X Chen, Y Chen, Y Cheng, A Cheplakov, R Cherkaoui El Moursli, V Chernyatin, E Cheu, L Chevalier, V Chiarella, G Chiefari, JT Childers, A Chilingarov, G Chiodini, AS Chisholm, RT Chislett, A Chitan, MV Chizhov, G Choudalakis, S Chouridou, BKB Chow, IA Christidi, D Chromek-Burckhart, ML Chu, J Chudoba, G Ciapetti, AK Ciftci, R Ciftci, D Cinca, V Cindro, A Ciocio, M Cirilli, P Cirkovic, ZH Citron, M Citterio, M Ciubancan, A Clark, PJ Clark, RN Clarke, JC Clemens, B Clement, C Clement, Y Coadou, M Cobal, A Coccaro, J Cochran, S Coelli, L Coffey, JG Cogan, J Coggeshall, J Colas, B Cole, S Cole, AP Colijn, C Collins-Tooth, J Collot, T Colombo, G Colon, G Compostella, P Conde Muiño, E Coniavitis, MC Conidi, SM Consonni, V Consorti, S Constantinescu, C Conta, G Conti, F Conventi, M Cooke, BD Cooper, AM Cooper-Sarkar, NJ Cooper-Smith, K Copic, T Cornelissen, M Corradi, F Corriveau, A Corso-Radu, A Cortes-Gonzalez, G Cortiana, G Costa, MJ Costa, D Costanzo, D Côté, G Cottin, L Courneyea, G Cowan, BE Cox, K Cranmer, G Cree, S Crépé-Renaudin, F Crescioli, M Cristinziani, G Crosetti, C-M Cuciuc, C Cuenca Almenar, T Cuhadar Donszelmann, J Cummings, M Curatolo, C Cuthbert, H Czirr, P Czodrowski, Z Czyczula, S D’Auria, M D’Onofrio, A D’Orazio, MJ Da Cunha Sargedas De Sousa, C Da Via, W Dabrowski, A Dafinca, T Dai, F Dallaire, C Dallapiccola, M Dam, DS Damiani, AC Daniells, M Dano Hoffmann, V Dao, G Darbo, GL Darlea, S Darmora, JA Dassoulas, W Davey, C David, T Davidek, E Davies, M Davies, O Davignon, AR Davison, Y Davygora, E Dawe, I Dawson, RK Daya-Ishmukhametova, K De, R de Asmundis, S De Castro, S De Cecco, J de Graat, N De Groot, P de Jong, C De La Taille, H De la Torre, F De Lorenzi, L De Nooij, D De Pedis, A De Salvo, U De Sanctis, A De Santo, JB De Vivie De Regie, G De Zorzi, WJ Dearnaley, R Debbe, C Debenedetti, B Dechenaux, DV Dedovich, J Degenhardt, J Del Peso, T Del Prete, T Delemontex, F Deliot, M Deliyergiyev, A Dell’Acqua, L Dell’Asta, M Della Pietra, D della Volpe, M Delmastro, PA Delsart, C Deluca, S Demers, M Demichev, A Demilly, B Demirkoz, SP Denisov, D Derendarz, JE Derkaoui, F Derue, P Dervan, K Desch, PO Deviveiros, A Dewhurst, B DeWilde, S Dhaliwal, R Dhullipudi, A Di Ciaccio, L Di Ciaccio, C Di Donato, A Di Girolamo, B Di Girolamo, A Di Mattia, B Di Micco, R Di Nardo, A Di Simone, R Di Sipio, D Di Valentino, MA Diaz, EB Diehl, J Dietrich, TA Dietzsch, S Diglio, K Dindar Yagci, J Dingfelder, C Dionisi, P Dita, S Dita, F Dittus, F Djama, T Djobava, MAB do Vale, A Do Valle Wemans, TKO Doan, D Dobos, E Dobson, J Dodd, C Doglioni, T Doherty, T Dohmae, Y Doi, J Dolejsi, Z Dolezal, BA Dolgoshein, M Donadelli, S Donati, J Donini, J Dopke, A Doria, A Dos Anjos, A Dotti, MT Dova, AT Doyle, M Dris, J Dubbert, S Dube, E Dubreuil, E Duchovni, G Duckeck, OA Ducu, D Duda, A Dudarev, F Dudziak, L Duflot, L Duguid, M Dührssen, M Dunford, H Duran Yildiz, M Düren, M Dwuznik, J Ebke, W Edson, CA Edwards, NC Edwards, W Ehrenfeld, T Eifert, G Eigen, K Einsweiler, E Eisenhandler, T Ekelof, M El Kacimi, M Ellert, S Elles, F Ellinghaus, K Ellis, N Ellis, J Elmsheuser, M Elsing, D Emeliyanov, Y Enari, OC Endner, M Endo, R Engelmann, J Erdmann, A Ereditato, D Eriksson, G Ernis, J Ernst, M Ernst, J Ernwein, D Errede, S Errede, E Ertel, M Escalier, H Esch, C Escobar, X Espinal Curull, B Esposito, F Etienne, AI Etienvre, E Etzion, D Evangelakou, H Evans, L Fabbri, G Facini, RM Fakhrutdinov, S Falciano, Y Fang, M Fanti, A Farbin, A Farilla, T Farooque, S Farrell, SM Farrington, P Farthouat, F Fassi, P Fassnacht, D Fassouliotis, B Fatholahzadeh, A Favareto, L Fayard, P Federic, OL Fedin, W Fedorko, M Fehling-Kaschek, L Feligioni, C Feng, EJ Feng, H Feng, AB Fenyuk, W Fernando, S Ferrag, J Ferrando, V Ferrara, A Ferrari, P Ferrari, R Ferrari, DE Ferreira de Lima, A Ferrer, D Ferrere, C Ferretti, A Ferretto Parodi, M Fiascaris, F Fiedler, A Filipčič, M Filipuzzi, F Filthaut, M Fincke-Keeler, KD Finelli, MCN Fiolhais, L Fiorini, A Firan, J Fischer, MJ Fisher, EA Fitzgerald, M Flechl, I Fleck, P Fleischmann, S Fleischmann, GT Fletcher, G Fletcher, T Flick, A Floderus, LR Flores Castillo, AC Florez Bustos, MJ Flowerdew, T Fonseca Martin, A Formica, A Forti, D Fortin, D Fournier, H Fox, P Francavilla, M Franchini, S Franchino, D Francis, M Franklin, S Franz, M Fraternali, S Fratina, ST French, C Friedrich, F Friedrich, D Froidevaux, JA Frost, C Fukunaga, E Fullana Torregrosa, BG Fulsom, J Fuster, C Gabaldon, O Gabizon, A Gabrielli, A Gabrielli, S Gadatsch, T Gadfort, S Gadomski, G Gagliardi, P Gagnon, C Galea, B Galhardo, EJ Gallas, V Gallo, BJ Gallop, P Gallus, G Galster, KK Gan, RP Gandrajula, J Gao, YS Gao, FM Garay Walls, F Garberson, C García, JE García Navarro, M Garcia-Sciveres, RW Gardner, N Garelli, V Garonne, C Gatti, G Gaudio, B Gaur, L Gauthier, P Gauzzi, IL Gavrilenko, C Gay, G Gaycken, EN Gazis, P Ge, Z Gecse, CNP Gee, DAA Geerts, Ch Geich-Gimbel, K Gellerstedt, C Gemme, A Gemmell, MH Genest, S Gentile, M George, S George, D Gerbaudo, A Gershon, H Ghazlane, N Ghodbane, B Giacobbe, S Giagu, V Giangiobbe, P Giannetti, F Gianotti, B Gibbard, SM Gibson, M Gilchriese, TPS Gillam, D Gillberg, AR Gillman, DM Gingrich, N Giokaris, MP Giordani, R Giordano, FM Giorgi, P Giovannini, PF Giraud, D Giugni, C Giuliani, M Giunta, BK Gjelsten, I Gkialas, LK Gladilin, C Glasman, J Glatzer, A Glazov, GL Glonti, M Goblirsch-Kolb, JR Goddard, J Godfrey, J Godlewski, C Goeringer, S Goldfarb, T Golling, D Golubkov, A Gomes, LS Gomez Fajardo, R Gonçalo, J Goncalves Pinto Firmino Da Costa, L Gonella, S González de la Hoz, G Gonzalez Parra, ML Gonzalez Silva, S Gonzalez-Sevilla, JJ Goodson, L Goossens, PA Gorbounov, HA Gordon, I Gorelov, G Gorfine, B Gorini, E Gorini, A Gorišek, E Gornicki, AT Goshaw, C Gössling, MI Gostkin, I Gough Eschrich, M Gouighri, D Goujdami, MP Goulette, AG Goussiou, C Goy, S Gozpinar, HMX Grabas, L Graber, I Grabowska-Bold, P Grafström, K-J Grahn, J Gramling, E Gramstad, F Grancagnolo, S Grancagnolo, V Grassi, V Gratchev, HM Gray, JA Gray, E Graziani, OG Grebenyuk, ZD Greenwood, K Gregersen, IM Gregor, P Grenier, J Griffiths, N Grigalashvili, AA Grillo, K Grimm, S Grinstein, Ph Gris, YV Grishkevich, J-F Grivaz, JP Grohs, A Grohsjean, E Gross, J Grosse-Knetter, GC Grossi, J Groth-Jensen, ZJ Grout, K Grybel, F Guescini, D Guest, O Gueta, C Guicheney, E Guido, T Guillemin, S Guindon, U Gul, C Gumpert, J Gunther, J Guo, S Gupta, P Gutierrez, NG Gutierrez Ortiz, C Gutschow, N Guttman, C Guyot, C Gwenlan, CB Gwilliam, A Haas, C Haber, HK Hadavand, P Haefner, S Hageboeck, Z Hajduk, H Hakobyan, D Hall, G Halladjian, K Hamacher, P Hamal, K Hamano, M Hamer, A Hamilton, S Hamilton, L Han, K Hanagaki, K Hanawa, M Hance, C Handel, P Hanke, JR Hansen, JB Hansen, JD Hansen, PH Hansen, P Hansson, K Hara, AS Hard, T Harenberg, S Harkusha, D Harper, RD Harrington, OM Harris, PF Harrison, F Hartjes, A Harvey, S Hasegawa, Y Hasegawa, S Hassani, S Haug, M Hauschild, R Hauser, M Havranek, CM Hawkes, RJ Hawkings, AD Hawkins, T Hayashi, D Hayden, CP Hays, HS Hayward, SJ Haywood, SJ Head, T Heck, V Hedberg, L Heelan, S Heim, B Heinemann, S Heisterkamp, J Hejbal, L Helary, C Heller, M Heller, S Hellman, D Hellmich, C Helsens, J Henderson, RCW Henderson, A Henrichs, AM Henriques Correia, S Henrot-Versille, C Hensel, GH Herbert, CM Hernandez, Y Hernández Jiménez, R Herrberg-Schubert, G Herten, R Hertenberger, L Hervas, GG Hesketh, NP Hessey, R Hickling, E Higón-Rodriguez, JC Hill, KH Hiller, S Hillert, SJ Hillier, I Hinchliffe, E Hines, M Hirose, D Hirschbuehl, J 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G Jarlskog, L Jeanty, G-Y Jeng, I Jen-La Plante, D Jennens, P Jenni, J Jentzsch, C Jeske, S Jézéquel, MK Jha, H Ji, W Ji, J Jia, Y Jiang, M Jimenez Belenguer, S Jin, A Jinaru, O Jinnouchi, MD Joergensen, D Joffe, KE Johansson, P Johansson, KA Johns, K Jon-And, G Jones, RWL Jones, TJ Jones, PM Jorge, KD Joshi, J Jovicevic, X Ju, CA Jung, RM Jungst, P Jussel, A Juste Rozas, M Kaci, A Kaczmarska, P Kadlecik, M Kado, H Kagan, M Kagan, E Kajomovitz, S Kalinin, S Kama, N Kanaya, M Kaneda, S Kaneti, T Kanno, VA Kantserov, J Kanzaki, B Kaplan, A Kapliy, D Kar, K Karakostas, N Karastathis, M Karnevskiy, SN Karpov, K Karthik, V Kartvelishvili, AN Karyukhin, L Kashif, G Kasieczka, RD Kass, A Kastanas, Y Kataoka, A Katre, J Katzy, V Kaushik, K Kawagoe, T Kawamoto, G Kawamura, S Kazama, VF Kazanin, MY Kazarinov, R Keeler, PT Keener, R Kehoe, M Keil, JS Keller, H Keoshkerian, O Kepka, BP Kerševan, S Kersten, K Kessoku, J Keung, F Khalil-zada, H Khandanyan, A Khanov, D Kharchenko, A Khodinov, A 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ZwalinskiSearch for long-lived stopped R-hadrons decaying out of time with pp collisions using the ATLAS detector
Physical Review D American Physical Society (APS) 88:11 (2013) 112003