Aufsatz(elektronisch)#114. Februar 2012
When Things Go Wrong: Account Strategy Following a Corporate Crisis Event
In: Corporate reputation review, Band 15, Heft 1, S. 35-51
ISSN: 1479-1889
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Aufsatz(elektronisch)#218. Mai 2009
It Depends: Moderating the Relationships Among Perceived Waiting Time, Anger, and Regret
In: Journal of service research, Band 12, Heft 2, S. 138-155
ISSN: 1552-7379
When consumers have to wait, the service delivery process is frequently compromised. The literature suggests that reducing waiting time is beneficial, but for service firms faced with scarce resources this is not always an option. As an alternative strategy, this study identifies and tests the mitigating effects of three factors that moderate the waiting time—anger and waiting time—regret relationships. Results show that in four service industries, affective commitment, perceived justice, and physical environment quality affect negative evaluations of a service experience and attenuate the effects of waiting time on both anger and regret. The authors discuss implications for researchers and service marketers in light of the results.
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Open Access#32018
The THESEUS space mission concept: science case, design and expected performances
Amati, L; O'Brien, P; Götz, D; Bozzo, E; Tenzer, C; Frontera, F; Ghirlanda, G; Labanti, C; Osborne, J. P; Stratta, G; Tanvir, N; Willingale, R; Attina, P; Campana, R; Castro-Tirado, A. J; Contini, C; Fuschino, F; Gomboc, A; Hudec, R; Orleanski, P; Renotte, E; Rodic, T; Bagoly, Z; Blain, A; Callanan, P; Covino, S; Ferrara, A; Le Floch, E; Marisaldi, M; Mereghetti, S; Rosati, P; Vacchi, A; D'Avanzo, P; Giommi, P; Piranomonte, S; Piro, L; Reglero, V; Rossi, A; Santangelo, A; Salvaterra, R; Tagliaferri, G; Vergani, S; Vinciguerra, S; Briggs, M; Campolongo, E; Ciolfi, R; Connaughton, V; Cordier, B; Morelli, B; Orlandini, M; Adami, C; Argan, A; Atteia, J. L; Auricchio, N; Balazs, L; Baldazzi, G; Basa, S; Basak, R; Bellutti, P; Bernardini, M. G; Bertuccio, G; Braga, J; Branchesi, M; Brandt, S; Brocato, E; Budtz-Jorgensen, C; Bulgarelli, A; Burderi, L; Camp, J; Capozziello, S; Caruana, J; Casella, P; Cenko, B; Chardonnet, P; Ciardi, B; Colafrancesco, S; Dainotti, M. G; D'Elia, V; De Martino, D; De Pasquale, M; Del Monte, E; Della Valle, M; Drago, A; Evangelista, Y
The file associated with this record is under embargo until 12 months after publication, in accordance with the publisher's self-archiving policy. The full text may be available through the publisher links provided above. ; THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5–1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift ∼10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late '20s/early '30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA). ; S.E. acknowledges the financial support from contracts ASI-INAF I/009/10/0, NARO15 ASI-INAF I/037/12/0 and ASI 2015-046-R.0. R.H. acknowledges GACR grant 13-33324S. S.V. research leading to these results has received funding from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no 606176. D.S. was supported by the Czech grant 16-01116S GA ČR. Maria Giovanna Dainotti acknowledges funding from the European Union through the Marie Curie Action FP7-PEOPLE-2013-IOF, under grant agreement No. 626267 ("Cosmological Candles"). ; Peer-reviewed ; Post-print
BASE
Open Access#42018
The THESEUS space mission concept: science case, design and expected performances
Amati, L; O'Brien, P; Götz, D; Bozzo, E; Tenzer, C; Frontera, F; Ghirlanda, G; Labanti, C; Osborne, J. P; Stratta, G; Tanvir, N; Caruana, J; Casella, P; Cenko, B; Chardonnet, P; Ciardi, B; Colafrancesco, S; Dainotti, M. G; D'Elia, V; De Martino, D; Margutti, R; Kawai, N; De Pasquale, M; Del Monte, E; Della Valle, M; Drago, A; Evangelista, Y; Feroci, M; Finelli, F; Fiorini, M; Fynbo, J; Gal-Yam, A; Wiersema, K; Martin-Carrillo, A; Gendre, B; Ghisellini, G; Grado, A; Guidorzi, C; Hafizi, M; Hanlon, L; Hjorth, J; Izzo, L; Kiss, L; Korpela, S; Kumar, P; Willingale, R; Kuvvetli, I; Masetti, N; McBreen, S; Mignani, R; Morgante, G; Mundell, C; Nargaard-Nielsen, H. U; Nicastro, L; Lebrun, V; Palazzi, E; Paltani, S; Panessa, F; Attina, P; Pareschi, G; Pe'er, A; Penacchioni, A. V; Pian, E; Piedipalumbo, E; Piran, T; Lu, F; Rauw, G; Razzano, M; Read, A; Rezzolla, L; Campana, R; Romano, P; Ruffini, R; Savaglio, S; Sguera, V; Schady, P; MacFadyen, A; Skidmore, W; Song, L; Stanway, E; Starling, R; Topinka, M; Castro-Tirado, Alberto J; Troja, E; van Putten, M; Vanzella, E; Vercellone, S; Malaguti, G; Wilson-Hodge, C; Yonetoku, D; Zampa, G; Zampa, N; Zhang, B; Zhang, B. B; Contini, C; Zhang, S; Zhang, S. -N; Antonelli, A; Maraschi, L; Bianco, F; Boci, S; Boer, M; Botticella, M.T; Boulade, O; Butler, C; Campana, S; Fuschino, F; Capitanio, F; Celotti, A; Melandri, A; Chen, Y; Colpi, M; Comastri, A; Cuby, Jean-Gabriel; Dadina, M; De Luca, A; Dong, Y. -W; Ettori, S; Gomboc, A; Gandhi, P; Orleanski, P; Geza, E; Greiner, J; Guiriec, S; Harms, J; Hernanz, M; Hornstrup, A; Hutchinson, I; Israel, G; Jonker, P; Hudec, R; Lavagna, M; Kaneko, Y; Modjaz, M; Morris, D; Omodei, N; Paizis, A; Páta, P; Petrosian, V; Rachevski, A; Rhoads, J; Ryde, F; Sabau-Graziati, L; Li, T; Renotte, E; Shigehiro, N; Sims, M; Soomin, J; Szécsi, D; Urata, Y; Uslenghi, M; Valenziano, L; Vianello, G; Vojtech, S; Longo, F; Watson, D; Rodic, T; Zicha, J; Bagoly, Z; Blain, A; Callanan, P; Covino, S; Ferrara, A; Le Floch, E; Marisaldi, M; Lyutikov, M; Mereghetti, S; Rosati, P; Vacchi, A; D'Avanzo, P; Giommi, P; Piranomonte, S; Piro, L; Reglero, V; Rossi, A; Santangelo, A; Maio, U; Salvaterra, R; Tagliaferri, G; Vergani, S; Vinciguerra, S; Briggs, M; Campolongo, E; Ciolfi, R; Connaughton, V; Cordier, B; Morelli, B; Maiorano, E; Orlandini, M; Adami, C; Argan, A; Atteia, J.L; Auricchio, N; Balazs, L; Baldazzi, G; Basa, S; Basak, R; Bellutti, P; Malcovati, P; Bernardini, M. G; Bertuccio, G; Braga, J; Branchesi, M; Brandt, S; Brocato, E; Budtz-Jørgensen, C; Bulgarelli, A; Burderi, L; Camp, J; Malesani, D; Capozziello, S
THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift 10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ¿20s/early ¿30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).© 2018 COSPAR ; S.E. acknowledges the financial support from contracts ASI-INAF 1/009/10/0, NARO15 ASI-INAF 1/037/12/0 and ASI 2015-046-R.0. R.H. acknowledges GACR grant 13-33324S. S.V. research leading to these results has received funding from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no 606176. D.S. was supported by the Czech grant 1601116S GA CR. Maria Giovanna Dainotti acknowledges funding from the European Union through the Marie Curie Action FP7-PEOPLE-2013-IOF, under grant agreement No. 626267 (>Cosmological Candles>).
BASE
Open Access#52016
SUPPLEMENT: LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914 (2016, ApJL, 826, L13)
Abbott, B. P; Abbott, R; Abbott, T. D; Abernathy, M. R; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, R. X; Adya, V. B; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, O. D; Aiello, L; Ain, A; Ajith, P; Allen, B; Allocca, A; Altin, P. A; Anderson, S. B; Anderson, W. G; Arai, K; Araya, M. C; Arceneaux, C. C; Areeda, J. S; Arnaud, N; Arun, K. G; Ascenzi, S; Ashton, G; Ast, M; Aston, S. M; Astone, P; Aufmuth, P; Aulbert, C; Babak, S; Bacon, P; Bader, M. K. M; Baker, P. T; Baldaccini, F; Ballardin, G; Ballmer, S. W; Barayoga, J. C; Barclay, S. E; Barish, B. C; Barker, D; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Barta, D; Barthelmy, S; Bartlett, J; Bartos, I; Bassiri, R; Basti, A; Batch, J. C; Baune, C; Bavigadda, V; Bazzan, M; Behnke, B; Bejger, M; Bell, A. S; Bell, C. J; Berger, B. K; Bergman, J; Bergmann, G; Berry, C. P. L; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; Bilenko, I. A; Billingsley, G; Birch, J; Birney, R; Biscans, S; Bisht, A; Bitossi, M; Biwer, C; Bizouard, M. A; Blackburn, J. K; Blair, C. D; Blair, D. G; Blair, R. M; Bloemen, S; Bock, O; Bodiya, T. P; Boer, M; Bogaert, G; Bogan, C; Bohe, A; Bojtos, P; Bond, C; Bondu, F; Bonnand, R; Boom, B. A; Bork, R; Boschi, V; Bose, S; Bouffanais, Y; Bozzi, A; Bradaschia, C; Brady, P. R; Braginsky, V. B; Branchesi, M; Brau, J. E; Briant, T; Brillet, A; Brinkmann, M; Brisson, V; Brockill, P; Brooks, A. F; Brown, D. A; Brown, D. D; Brown, N. M; Buchanan, C. C; Buikema, A; Bulik, T; Bulten, H. J; Buonanno, A; Buskulic, D; Buy, C; Byer, R. L; Cadonati, L; Cagnoli, G; Cahillane, C; Bustillo, J. C; Callister, T; Calloni, E; Camp, J. B; Cannon, K. C; Cao, J; Capano, C. D; Capocasa, E; Carbognani, F; Caride, S; Diaz, J. C; Casentini, C; Caudill, S; Cavaglia, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, C. B; Baiardi, L. C; Cerretani, G; Cesarini, E; Chakraborty, R; Chalermsongsak, T; Chamberlin, S. J; Chan, M; Chao, S; Charlton, P; Chassande-Mottin, E; Chen, H. Y; Chen, Y; Cheng, C; Chincarini, A; Chiummo, A; Cho, H. S; Cho, M; Chow, J. H; Christensen, N; Chu, Q; Chua, S; Chung, S; Ciani, G; Clara, F; Clark, J. A; Cleva, F; Coccia, E; Cohadon, P. -F; Colla, A; Collette, C. G; Cominsky, L; Constancio, M; Conte, A; Conti, L; Cook, D; Corbitt, T. R; Cornish, N; Corsi, A; Cortese, S; Costa, C. A; Coughlin, M. W; Coughlin, S. B; Coulon, J. -P; Countryman, S. T; Couvares, P; Cowan, E. E; Coward, D. M; Cowart, M. J; Coyne, D. C; Coyne, R; Craig, K; Creighton, J. D. E; Cripe, J; Crowder, S. G; Cumming, A; Cunningham, L; Cuoco, E; Dal Canton, T; Danilishin, S. L; D'Antonio, S; Danzmann, K; Darman, N. S; Dattilo, V; Dave, I; Daveloza, H. P; Davier, M; Davies, G. S; Daw, E. J; Day, R; DeBra, D; Debreczeni, G; Degallaix, J; De Laurentis, M; Deleglise, S; Del Pozzo, W; Denker, T; Dent, T; Dereli, H; Dergachev, V; DeRosa, R. T; De Rosa, R; DeSalvo, R; Dhurandhar, S; Diaz, M. C; Di Fiore, L; Di Giovanni, M; Di Lieto, A; Di Pace, S; Di Palma, I; Di Virgilio, A; Dojcinoski, G; Dolique, V; Donovan, F; Dooley, K. L; Doravari, S; Douglas, R; Downes, T. P; Drago, M; Drever, R. W. P; Driggers, J. C; Du, Z; Ducrot, M; Dwyer, S. E; Edo, T. B; Edwards, M. C; Effler, A; Eggenstein, H. -B; Ehrens, P; Eichholz, J; Eikenberry, S. S; Engels, W; Essick, R. C; Etzel, T; Evans, M; Evans, T. M; Everett, R; Factourovich, M; Fafone, V; Fair, H; Fairhurst, S; Fan, X; Fang, Q; Farinon, S; Farr, B; Farr, W. M; Favata, M; Fays, M; Fehrmann, H; Fejer, M. M; Ferrante, I; Ferreira, E. C; Ferrini, F; Fidecaro, F; Fiori, I; Fiorucci, D; Fisher, R. P; Flaminio, R; Fletcher, M; Fournier, J. -D; Franco, S; Frasca, S; Frasconi, F; Frei, Z; Freise, A; Frey, R; Frey, V; Fricke, T. T; Fritschel, P; Frolov, V. V; Fulda, P; Fyffe, M; Gabbard, H. A. G; Gair, J. R; Gammaitoni, L; Gaonkar, S. G; Garufi, F; Gatto, A; Gaur, G; Gehrels, N; Gemme, G; Gendre, B; Genin, E; Gennai, A; George, J; Gergely, L; Germain, V; Ghosh, A; Ghosh, S; Giaime, J. A; Giardina, K. D; Giazotto, A; Gill, K; Glaefke, A; Goetz, E; Goetz, R; Gondan, L; Gonzalez, G; Castro, J. M. G; Gopakumar, A; Gordon, N. A; Gorodetsky, M. L; Gossan, S. E; Gosselin, M; Gouaty, R; Graef, C; Graff, P. B; Granata, M; Grant, A; Gras, S; Gray, C; Greco, G; Green, A. C; Groot, P; Grote, H; Grunewald, S; Guidi, G. M; Guo, X; Gupta, A; Gupta, M. K; Gushwa, K. E; Gustafson, E. K; Gustafson, R; Hacker, J. J; Hall, B. R; Hall, E. D; Hammond, G; Haney, M; Hanke, M. M; Hanks, J; Hanna, C; Hannam, M. D; Hanson, J; Hardwick, T; Haris, K; Harms, J; Harry, G. M; Harry, I. W; Hart, M. J; Hartman, M. T; Haster, C. -J; Haughian, K; Heidmann, A; Heintze, M. C; Heitmann, H; Hello, P; Hemming, G; Hendry, M; Heng, I. S; Hennig, J; Heptonstall, A. W; Heurs, M; Hild, S; Hoak, D; Hodge, K. A; Hofman, D; Hollitt, S. E; Holt, K; Holz, D. E; Hopkins, P; Hosken, D. J; Hough, J; Houston, E. A; Howell, E. J; Hu, Y. M; Huang, S; Huerta, E. A; Huet, D; Hughey, B; Husa, S; Huttner, S. H; Huynh-Dinh, T; Idrisy, A; Indik, N; Ingram, D. R; Inta, R; Isa, H. N; Isac, J. -M; Isi, M; Islas, G; Isogai, T; Iyer, B. R; Izumi, K; Jacqmin, T; Jang, H; Jani, K; Jaranowski, P; Jawahar, S; Jimenez-Forteza, F; Johnson, W. W; Jones, D. I; Jones, R; Jonker, R. J. G; Ju, L; Kalaghatgi, C. V; Kalogera, V; Kandhasamy, S; Kang, G; Kanner, J. B; Karki, S; Kasprzack, M; Katsavounidis, E; Katzman, W; Kaufer, S; Kaur, T; Kawabe, K; Kawazoe, F; Kefelian, F; Kehl, M. S; Keitel, D; Kelley, D. B; Kells, W; Kennedy, R; Key, J. S; Khalaidovski, A; Khalili, F. Y; Khan, I; Khan, S; Khan, Z; Khazanov, E. A; Kijbunchoo, N; Kim, C; Kim, J; Kim, K; Kim, N; Kim, Y. -M; King, E. J; King, P. J; Kinzel, D. L; Kissel, J. S; Kleybolte, L; Klimenko, S; Koehlenbeck, S. M; Kokeyama, K; Koley, S; Kondrashov, V; Kontos, A; Korobko, M; Korth, W. Z; Kowalska, I; Kozak, D. B; Kringel, V; Krolak, A; Krueger, C; Kuehn, G; Kumar, P; Kuo, L; Kutynia, A; Lackey, B. D; Landry, M; Lange, J; Lantz, B; Lasky, P. D; Lazzarini, A; Lazzaro, C; Leaci, P; Leavey, S; Lebigot, E. O; Lee, C. H; Lee, H. K; Lee, H. M; Lee, K; Lenon, A; Leonardi, M; Leong, J. R; Leroy, N; Letendre, N; Levin, Y; Levine, B. M; Li, T. G. F; Libson, A; Littenberg, T. B; Lockerbie, N. A; Logue, J; Lombardi, A. L; Lord, J. E; Lorenzini, M; Loriette, V; Lormand, M; Losurdo, G; Lough, J. D; Lueck, H; Lundgren, P; Luo, J; Lynch, R; Ma, Y; MacDonald, T; Machenschalk, B; MacInnis, M; Macleod, D. M; Magana-Sandoval, F; Magee, R. M; Mageswaran, M; Majorana, E; Maksimovic, I; Malvezzi, V; Man, N; Mandel, I; Mandic, V; Mangano, V; Mansell, G. L; Manske, M; Mantovani, M; Marchesoni, F; Marion, F; Marka, S; Marka, Z; Markosyan, A. S; Maros, E; Martelli, F; Martellini, L; Martin, I. W; Martin, R. M; Martynov, D. V; Marx, J. N; Mason, K; Masserot, A; Massinger, T. J; Masso-Reid, M; Matichard, F; Matone, L; Mavalvala, N; Mazumder, N; Mazzolo, G; McCarthy, R; McClelland, D. E; McCormick, S; McGuire, S. C; McIntyre, G; McIver, J; McManus, D. J; McWilliams, S. T; Meacher, D; Meadors, G. D; Meidam, J; Melatos, A; Mendell, G; Mendoza-Gandara, D; Mercer, R. A; Merilh, E; Merzougui, M; Meshkov, S; Messenger, C; Messick, C; Meyers, P. M; Mezzani, F; Miao, H; Michel, C; Middleton, H; Mikhailov, E. E; Milano, L; Miller, J; Millhouse, M; Minenkov, Y; Ming, J; Mirshekari, S; Mishra, C; Mitra, S; Mitrofanov, V. P; Mitselmakher, G; Mittleman, R; Moggi, A; Mohan, M; Mohapatra, S. R. P; Montani, M; Moore, B. C; Moore, C. J; Moraru, D; Moreno, G; Morriss, S. R; Mossavi, K; Mours, B; Mow-Lowry, C. M; Mueller, C. L; Mueller, G; Muir, A. W; Mukherjee, A; Mukherjee, D; Mukherjee, S; Mukund, N; Mullavey, A; Munch, J; Murphy, D. J; Murray, P. G; Mytidis, A; Nardecchia, I; Naticchioni, L; Nayak, R. K; Necula, V; Nedkova, K; Nelemans, G; Neri, M; Neunzert, A; Newton, G; Nguyen, T. T; Nielsen, A. B; Nissanke, S; Nitz, A; Nocera, F; Nolting, D; Normandin, M. E. N; Nuttall, L. K; Oberling, J; Ochsner, E; O'Dell, J; Oelker, E; Ogin, G. H; Oh, J. J; Oh, S. H; Ohme, F; Oliver, M; Oppermann, P; Oram, R. J; O'Reilly, B; O'Shaughnessy, R; Ottaway, D. J; Ottens, R. S; Overmier, H; Owen, B. J; Pai, A; Pai, S. A; Palamos, J. R; Palashov, O; Palliyaguru, N; Palomba, C; Pal-Singh, A; Pan, H; Pankow, C; Pannarale, F; Pant, B. C; Paoletti, F; Paoli, A; Papa, M. A; Paris, H. R; Parker, W; Pascucci, D; Pasqualetti, A; Passaquieti, R; Passuello, D; Patricelli, B; Patrick, Z; Pearlstone, B. L; Pedraza, M; Pedurand, R; Pekowsky, L; Pele, A; Penn, S; Perreca, A; Phelps, M; Piccinni, O; Pichot, M; Piergiovanni, F; Pierro, V; Pillant, G; Pinard, L; Pinto, I. M; Pitkin, M; Poggiani, R; Popolizio, P; Post, A; Powell, J; Prasad, J; Predoi, V; Premachandra, S. S; Prestegard, T; Price, L. R; Prijatelj, M; Principe, M; Privitera, S; Prodi, G. A; Prokhorov, L; Puncken, O; Punturo, M; Puppo, P; Puerrer, M; Qi, H; Qin, J; Quetschke, V; Quintero, E. A; Quitzow-James, R; Raab, F. J; Rabeling, D. S; Radkins, H; Raffai, P; Raja, S; Rakhmanov, M; Rapagnani, P; Raymond, V; Razzano, M; Re, V; Read, J; Reed, C. M; Regimbau, T; Rei, L; Reid, S; Reitze, D. H; Rew, H; Reyes, S. D; Ricci, F; Riles, K; Robertson, N. A; Robie, R; Robinet, F; Rocchi, A; Rolland, L; Rollins, J. G; Roma, V. J; Romano, R; Romanov, G; Romie, J. H; Rosinska, D; Rowan, S; Ruediger, A; Ruggi, P; Ryan, K; Sachdev, S; Sadecki, T; Sadeghian, L; Salconi, L; Saleem, M; Salemi, F; Samajdar, A; Sammut, L; Sanchez, E. J; Sandberg, V; Sandeen, B; Sanders, J. R; Sassolas, B; Sathyaprakash, B. S; Saulson, P. R; Sauter, O; Savage, R. L; Sawadsky, A; Schale, P; Schilling, R; Schmidt, J; Schmidt, P; Schnabel, R; Schofield, R. M. S; Schoenbeck, A; Schreiber, E; Schuette, D; Schutz, B. F; Scott, J; Scott, S. 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U; Malesani, D; Milvang-Jensen, B; Watson, D; Irwin, M; Fernandez, C. G; McMahon, R. G; Banerji, M; Gonzalez-Solares, E; Schulze, S; Postigo, A. de U; Thoene, C. C; Cano, Z; Rosswog, S; LIGO Sci Collaboration Virgo Colla; ASKAP Collaboration; BOOTES Collaboration; Dark Energy Survey Collaboration; Dark Energy Camera GW-EM Collabor; Fermi GBM Collaboration; FERMI LAT Collaboration; GRAvitational Wave Inaf TeAm GRAWI; INTEGRAL Collaboration; IPTF Collaboration; InterPlanetary Network; J-GEM Collaboration; LA Silla-QUEST Survey; Liverpool Telescope Collaboration; Low Frequency Array LOFAR Collabo; MASTER Collaboration; MAXI Collaboration; MWA Collaboration; Pan-STARRS Collaboration; PESSTO Collaboration; Pi Sky Collaboration; SkyMapper Collaboration; Swift Collaboration; Tarot Zadko Algerian Natl Observ C; TOROS Collaboration; VISTA Collaboration
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UK Space Agency: ST/P002196/1 ; This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands.
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