New Limits on Gravitational Radiation using Pulsars
| dc.creator | Lommen, A. N. | |
| dc.date | 2002-08-30 | |
| dc.date.accessioned | 2026-07-07T02:04:53Z | |
| dc.date.available | 2026-07-07T02:04:53Z | |
| dc.description | We calculate a new gravitational wave background limit using timing residuals from PSRs J1713+0747, B1855+09, and B1937+21. The new limit is based on 17 years of continuous data pieced together from 3 different observing projects: 2 at the Arecibo Observatory and 1 at the 140ft Green Bank Telescope. This project represents the earliest results from the `Pulsar Timing Array' which will soon be able detect the stochastic background from early massive black hole mergers. | |
| dc.description | 12 pages, 11 figures, 3 tables. To appear in the Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef, eds W. Becker, H. Lesch & J. Truemper. Proceedings are available as MPE-Report 278 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0208572 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0208572 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4935 | |
| dc.subject | Astrophysics | |
| dc.title | New Limits on Gravitational Radiation using Pulsars | |
| dc.type | text |