| Preprints | |
| Report number | arXiv:1702.00786 |
| Title | Laser Interferometer Space Antenna |
| Related title | Laser Interferometer Space Antenna |
| Author(s) |
Amaro-Seoane, Pau (Hannover, Max Planck Inst. Grav.) ; Audley, Heather (Hannover, Max Planck Inst. Grav.) ; Babak, Stanislav (Potsdam, Max Planck Inst.) ; Baker, John (LBL, Berkeley ; UC, San Francisco) ; Barausse, Enrico (Paris, Inst. Astrophys.) ; Bender, Peter (Colorado U. ; NIST, Boulder) ; Berti, Emanuele (Lisbon, CENTRA ; Mississippi U.) ; Binetruy, Pierre (Annecy, LAPP ; CERN) ; Born, Michael (Hannover U. ; Hannover, Max Planck Inst. Grav.) ; Bortoluzzi, Daniele (INFN, Trento ; TIFPA-INFN, Trento ; Trento U.) ; Camp, Jordan (NASA, Goddard) ; Caprini, Chiara (Saclay, SPhT) ; Cardoso, Vitor (McMaster U. ; Perimeter Inst. Theor. Phys. ; Waterloo U.) ; Colpi, Monica (INFN, Milan Bicocca ; Milan Bicocca U.) ; Conklin, John (Florida U.) ; Cornish, Neil (Montana State U.) ; Cutler, Curt (Caltech, JPL) ; Danzmann, Karsten (Munich, Max Planck Inst. Quantenopt.) ; Dolesi, Rita (TIFPA-INFN, Trento ; Trento U.) ; Ferraioli, Luigi (Zurich, ETH) ; Ferroni, Valerio (INFN, Rome3 ; Trento U.) ; Fitzsimons, Ewan (Airbus, Immenstaad) ; Gair, Jonathan (Cambridge U., Inst. of Astron.) ; Gesa, Lluis ; Giardini, Domenico (Zurich, ETH) ; Gibert, Ferran (ICE, Bellaterra) ; Grimani, Catia (Urbino U.) ; Halloin, Hubert (APC, Paris) ; Heinzel, Gerhard (Hannover, Max Planck Inst. Grav.) ; Hertog, Thomas (APC, Paris ; Leuven U.) ; Hewitson, Martin (Hannover, Max Planck Inst. Grav.) ; Holley-Bockelmann, Kelly (Vanderbilt U.) ; Hollington, Daniel ; Hueller, Mauro (TIFPA-INFN, Trento) ; Inchauspe, Henri (APC, Paris) ; Jetzer, Philippe (PSI, Villigen ; Zurich U.) ; Karnesis, Nikos ; Killow, Christian (Glasgow U.) ; Klein, Antoine (Mississippi U. ; Montana State U.) ; Klipstein, Bill ; Korsakova, Natalia (Hannover, Max Planck Inst. Grav.) ; Larson, Shane L. ; Livas, Jeffrey (NASA, Goddard) ; Lloro, Ivan (ICE, Bellaterra) ; Man, Nary (Cote d'Azur Observ., Nice) ; Mance, Davor (Zurich, ETH) ; Martino, Joseph (Diderot U., Paris) ; McKenzie, Kirk (Caltech, JPL) ; McWilliams, Sean T. (West Virginia U.) ; Miller, Cole ; Mueller, Guido (Cornell U., LNS) ; Nardini, Germano (Bern U.) ; Nelemans, Gijs (Leuven U. ; Nijmegen U., IMAPP ; NIKHEF, Amsterdam) ; Nofrarias, Miquel (ICE, Bellaterra) ; Petiteau, Antoine (APC, Paris) ; Pivato, Paolo ; Plagnol, Eric (APC, Paris) ; Porter, E. (APC, Paris) ; Reiche, Jens (Hannover, Max Planck Inst. Grav.) ; Robertson, David (Glasgow U.) ; Robertson, Norna ; Rossi, Elena (INFN, Naples ; Naples U.) ; Russano, Giuliana ; Schutz, Bernard (Cardiff U. ; Potsdam, Max Planck Inst.) ; Sesana, Alberto (Birmingham U.) ; Shoemaker, David (MIT) ; Slutsky, Jacob (Hannover, Max Planck Inst. Grav.) ; Sopuerta, Carlos F. (ICE, Bellaterra) ; Sumner, Tim (Imperial Coll., London) ; Tamanini, Nicola (Saclay, SPhT) ; Thorpe, Ira ; Troebs, Michael (Hannover U. ; Hannover, Max Planck Inst. Grav.) ; Vallisneri, Michele (Caltech, JPL) ; Vecchio, Alberto (Birmingham U.) ; Vetrugno, Daniele (TIFPA-INFN, Trento) ; Vitale, Stefano (Naples U.) ; Wanner, Gudrun (Hannover, Max Planck Inst. Grav.) ; Ward, Harry (Glasgow U.) ; Wass, Peter (Imperial Coll., London) ; Weber, William ; Ziemer, John ; Zweifel, Peter (Zurich, ETH) |
| Publication | 2017 |
| Imprint | 2017-02-02 |
| Number of pages | 41 |
| Note | Submitted to ESA on January 13th in response to the call for missions for the L3 slot in the Cosmic Vision Programme |
| Subject category | astro-ph.IM ; Astrophysics and Astronomy |
| Abstract | Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missions for L3. The observatory will be based on three arms with six active laser links, between three identical spacecraft in a triangular formation separated by 2.5 million km. LISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using Gravitational Waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the infant Universe at TeV energy scales, has known sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales near the horizons of black holes, all the way to cosmological scales. The LISA mission will scan the entire sky as it follows behind the Earth in its orbit, obtaining both polarisations of the Gravitational Waves simultaneously, and will measure source parameters with astrophysically relevant sensitivity in a band from below $10^{-4}\,$Hz to above $10^{-1}\,$Hz. |
| Other source | Inspire |
| Copyright/License | arXiv nonexclusive-distrib. 1.0 |
Element opprettet 2017-04-05, sist endret 2024-10-02