Sensitivity studies for third-generation gravitational wave observatories

Hild, S.; Abernathy, M.; Acernese, F.; Amaro-Seoane, P.; Andersson, N.; Arun, K.; Barone, F.; Barr, B.; Barsuglia, M.; Beker, M.; Beveridge, N.; Birindelli, S.; Bose, S.; Bosi, L.; Braccini, S.; Bradaschia, C.; Bulik, T.; Calloni, E.; Cella, G.; Chassande Mottin, E.; Chelkowski, S.; Chincarini, A.; Clark, J.; Coccia, E.; Colacino, C.; Colas, J.; Cumming, A.; Cunningham, L.; Cuoco, E.; Danilishin, S.; Danzmann, K.; De Salvo, R.; Dent, T.; De Rosa, R.; Di Fiore, L.; Di Virgilio, A.; Doets, M.; Fafone, V.; Falferi, P.; Flaminio, R.; Franc, J.; Frasconi, F.; Freise, A.; Friedrich, D.; Fulda, P.; Gair, J.; Gemme, G.; Genin, E.; Gennai, A.; Giazotto, A.; Glampedakis, K.; Gräf, C.; Granata, M.; Grote, H.; Guidi, G.; Gurkovsky, A.; Hammond, G.; Hannam, M.; Harms, J.; Heinert, D.; Hendry, M.; Heng, I.; Hennes, E.; Hough, J.; Husa, S.; Huttner, S.; Jones, G.; Khalili, F.; Kokeyama, K.; Kokkotas, K.; Krishnan, B.; Li, T.G.F.; Lorenzini, M.; Lück, H.; Majorana, E.; Mandel, I.; Mandic, V.; Mantovani, M.; Martin, I.; Michel, C.; Minenkov, Y.; Morgado, N.; Mosca, S.; Mours, B; Müller-Ebhardt, H.; Murray, P.; Nawrodt, R.; Nelson, J.; Oshaughnessy, R.; Ott, C. D.; Palomba, C.; Paoli, A.; Parguez, G.; Pasqualetti, A.; Passaquieti, R.; Passuello, D.; Pinard, L.; Plastino, W.; Poggiani, R.; Popolizio, P.; Prato, M.; Punturo, M.; Puppo, P.; Rabeling, D.; Rapagnani, P.; Read, J.; Regimbau, T.; Rehbein, H.; Reid, S.; Ricci, F.; Richard, F.; Rocchi, A.; Rowan, S.; Rüdiger, A.; Santamaría, L.; Sassolas, B.; Sathyaprakash, B.; Schnabel, R.; Schwarz, C.; Seidel, P.; Sintes, A.; Somiya, K.; Speirits, F.; Strain, K.; Strigin, S; Sutton, P.; Tarabrin, S.; Thüring, A.; van den Brand, J.; van Veggel, M.; van den Broeck, C.; Vecchio, A.; Veitch, J.; Vetrano, F.; Vicere, A.; Vyatchanin, S.; Willke, B.; Woan, G.; Yamamoto, K.

doi:10.1088/0264-9381/28/9/094013

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Sensitivity studies for third-generation gravitational wave observatories

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Amaro-Seoane, P.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Danzmann, K.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40454

Gräf, C.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40456

Grote, H.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons20661

Krishnan, B.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40475

Lück, H.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Rehbein, H.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Rüdiger, A.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Schnabel, R.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Thüring, A.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Willke, B.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Citation

Hild, S., Abernathy, M., Acernese, F., Amaro-Seoane, P., Andersson, N., Arun, K., et al. (2011). Sensitivity studies for third-generation gravitational wave observatories. Classical and quantum gravity, 28(9): 094013.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000F-0837-1

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