The construction and use of LISA sensitivity curves
The Laser Interferometer Space Antenna (LISA) will open the mHz band of the gravitational wave spectrum for exploration. Sensitivity curves are a useful tool for surveying the types of sources that can be detected by the LISA mission. Here we describe how the sensitivity curve is constructed, and ho...
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| Published in | Classical and quantum gravity Vol. 36; no. 10; pp. 105011 - 105026 |
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| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
IOP Publishing
23.05.2019
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| Subjects | |
| Online Access | Get full text |
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| Abstract | The Laser Interferometer Space Antenna (LISA) will open the mHz band of the gravitational wave spectrum for exploration. Sensitivity curves are a useful tool for surveying the types of sources that can be detected by the LISA mission. Here we describe how the sensitivity curve is constructed, and how it can be used to compute the signal-to-noise ratio for a wide range of binary systems. We adopt the 2018 LISA mission performance requirement design parameters. We consider both sky-averaged sensitivities, and the sensitivity to sources at particular sky locations. The calculations are included in a publicly available Python notebook. |
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| AbstractList | The Laser Interferometer Space Antenna (LISA) will open the mHz band of the gravitational wave spectrum for exploration. Sensitivity curves are a useful tool for surveying the types of sources that can be detected by the LISA mission. Here we describe how the sensitivity curve is constructed, and how it can be used to compute the signal-to-noise ratio for a wide range of binary systems. We adopt the 2018 LISA mission performance requirement design parameters. We consider both sky-averaged sensitivities, and the sensitivity to sources at particular sky locations. The calculations are included in a publicly available Python notebook. |
| Author | Robson, Travis Cornish, Neil J Liu, Chang |
| Author_xml | – sequence: 1 givenname: Travis orcidid: 0000-0001-9076-5055 surname: Robson fullname: Robson, Travis organization: Montana State University Department of Physics, eXtreme Gravity Institute, Bozeman, MT 59717, United States of America – sequence: 2 givenname: Neil J orcidid: 0000-0002-7435-0869 surname: Cornish fullname: Cornish, Neil J email: ncornish@montana.edu organization: Montana State University Department of Physics, eXtreme Gravity Institute, Bozeman, MT 59717, United States of America – sequence: 3 givenname: Chang orcidid: 0000-0002-3111-5957 surname: Liu fullname: Liu, Chang organization: University of Chinese Academy of Sciences School of Physical Sciences, Beijing 100049, People's Republic of China |
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| CODEN | CQGRDG |
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| Cites_doi | 10.1088/2041-8205/757/2/L21 10.1103/PhysRevD.66.122002 10.1088/0264-9381/14/6/020 10.1103/PhysRevD.47.2198 10.1103/PhysRevD.96.044005 10.1103/PhysRevD.65.022004 10.1103/PhysRevD.74.041501 10.1103/PhysRevD.91.024043 10.1088/0264-9381/29/12/124015 10.1103/PhysRevD.52.821 10.1103/PhysRevD.64.124013 10.1103/PhysRevD.69.082003 10.1103/PhysRevD.62.062001 10.1103/PhysRevD.57.4535 10.1088/0264-9381/24/19/S31 10.1007/s10714-014-1767-2 10.1103/PhysRevD.57.7089 10.1088/1742-6596/840/1/012024 10.1103/PhysRevD.62.042002 10.1093/mnras/289.1.185 |
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| References | 23 26 Moore C J (2) 2015; 32 Hermes J J (22) 2012; 757 27 Schilling R (6) 1997; 14 Chua A J K (24) 2017 Hewiston M (13) 2018 Robson T (3) 2018 Vallisneri M (25) 2012; 29 Thorne K S ed Hawking S W (9) 1987 10 11 12 15 16 17 18 Robson T (4) 2018 Cornish N (14) 2017; 840 Ajith P (19) 2007; 24 Audley H (1) 2017 5 7 8 20 21 |
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| Snippet | The Laser Interferometer Space Antenna (LISA) will open the mHz band of the gravitational wave spectrum for exploration. Sensitivity curves are a useful tool... |
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| Title | The construction and use of LISA sensitivity curves |
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