Advanced localization of massive black hole coalescences with LISA
The coalescence of massive black holes is one of the primary sources of gravitational waves (GWs) for LISA. Measurements of the GWs can localize the source on the sky to an ellipse with a major axis of a few tens of arcminutes to a few degrees, depending on source redshift, and a minor axis which is...
| Päätekijät: | , |
|---|---|
| Muut tekijät: | |
| Aineistotyyppi: | Artikkeli |
| Kieli: | en_US |
| Julkaistu: |
Institute of Physics
2010
|
| Linkit: | http://hdl.handle.net/1721.1/51796 https://orcid.org/0000-0001-6211-1388 |