The third generation of gravitational wave observatories and their science reach

@inproceedings{Punturo2010TheTG,
  title={The third generation of gravitational wave observatories and their science reach},
  author={M. Punturo and Mengyue Abernathy and Fausto Acernese and Ben Van Allen and Nils Andersson and K. Arun and Fabrizio Barone and Breona Barr and Matteo Barsuglia and Merve Beker and Nicole Beveridge and Simona Birindelli and Sumanta Bose and L. Bosi and S. Braccini and C. Bradaschia and T. Bulik and E. Calloni and Guiseppe Cella and E Chassande Mottin and Stephan Chelkowski and Andrea Chincarini and Jenny Clark and Eugenio Coccia and Carlo Nicola Colacino and Juan Col{\'a}s and A. Cumming and Lee S. Cunningham and Elena Cuoco and S Danilishin and Karsten Danzmann and Giovanni De Luca and R De Salvo and Terrence Dent and Raffaella Derosa and L. Di Fiore and A. Di Virgilio and Mathijs Doets and Viviana Fafone and Paolo Falferi and R. Flaminio and Jacques Franc and F. Frasconi and Andreas Freise and Paul Fulda and Jonathan Gair and Gianluca Gemme and A. Gennai and A. Giazotto and Kostas Glampedakis and Massimo Granata and Hartmut Grote and Gianluca Guidi and Georgina Hammond and Mark Hannam and Jan Harms and Daniel Heinert and Morgan Hendry and Iem Heng and Eric Hennes and Stefan G. Hild and Jim Hough and Sascha Husa and Sebastian Huttner and G Jones and F Khalili and Keiko Kokeyama and Kostas Kokkotas and Balachander Krishnan and Matteo Lorenzini and Harald L{\"u}ck and E. Majorana and Igor Mandel and Vuk Mandic and Ivar Martin and Claire Michel and Yury Minenkov and N. Morgado and Simona Mosca and B. Mours and Helge M{\"u}ller-Ebhardt and P. Murray and Ronny Nawrodt and Johanna Nelson and R W Oshaughnessy and Christian D. Ott and C. Palomba and Alessandro Paoli and G Parguez and A. Pasqualetti and R. Passaquieti and D. Passuello and L. Pinard and R. Poggiani and P Popolizio and Maurizio Prato and P. Puppo and D Rabeling and P. Rapagnani and Justin I. Read and Tania Regimbau and Hagen Rehbein and Suzanne Reid and Luciano Rezzolla and F. Ricci and Fr{\'e}d{\'e}ric Richard and Alessio Rocchi and Sheila Rowan and Albrecht R{\"u}diger and Beno{\^i}t Sassolas and Bangalore S. Sathyaprakash and Ruwen Schnabel and Carsten Schwarz and Paul Seidel and Anna Sintes and Kentaro Somiya and Fiona C Speirits and K Strain and S Strigin and P. Sutton and S Tarabrin and Jeroen van den Brand and C van Leewen and M van Veggel and Christian Van den Broeck and A. Vecchio and Jennifer Veitch and F. Vetrano and Andrea Vicer{\`e} and Sergey Vyatchanin and Bradford J. Willke and Graham Woan and P Wolfango and Kazuhiro Yamamoto},
  year={2010}
}
Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview… CONTINUE READING
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