| タイトル | Space Based Gravitational Wave Observatories (SGOs) |
| 本文（外部サイト） | http://hdl.handle.net/2060/20150000336 |
| 著者（英） | Livas, Jeff |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2014-11-11 |
| 言語 | eng |
| 内容記述 | Space-based Gravitational-wave Observatories (SGOs) will enable the systematic study of the frequency band from 0.0001 - 1 Hz of gravitational waves, where a rich array of astrophysical sources is expected. ESA has selected The Gravitational Universe as the science theme for the L3 mission opportunity with a nominal launch date in 2034. This will be at a minimum 15 years after ground-based detectors and pulsar timing arrays announce their first detections and at least 18 years after the LISA Pathfinder Mission will have demonstrated key technologies in a dedicated space mission. It is therefore important to develop mission concepts that can take advantage of the momentum in the field and the investment in both technology development and a precision measurement community on a more near-term timescale than the L3 opportunity. This talk will discuss a mission concept based on the LISA baseline that resulted from a recent mission architecture study. |
| NASA分類 | Astrophysics |
| レポートNO | GSFC-E-DAA-TN19381 |
| 権利 | No Copyright |
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