Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group
| dc.creator | Albrecht, Andreas | |
| dc.creator | Amendola, Luca | |
| dc.creator | Bernstein, Gary | |
| dc.creator | Clowe, Douglas | |
| dc.creator | Eisenstein, Daniel | |
| dc.creator | Guzzo, Luigi | |
| dc.creator | Hirata, Christopher | |
| dc.creator | Huterer, Dragan | |
| dc.creator | Kirshner, Robert | |
| dc.creator | Kolb, Edward | |
| dc.creator | Nichol, Robert | |
| dc.date | 2009-01-06 | |
| dc.date.accessioned | 2026-07-07T12:31:58Z | |
| dc.date.available | 2026-07-07T12:31:58Z | |
| dc.description | These are the findings of the Joint Dark Energy Mission (JDEM) Figure of Merit (FoM) Science Working Group (SWG), the FoMSWG. JDEM is a space mission planned by NASA and the DOE for launch in the 2016 time frame. The primary mission is to explore the nature of dark energy. In planning such a mission, it is necessary to have some idea of knowledge of dark energy in 2016, and a way to quantify the performance of the mission. In this paper we discuss these issues. | |
| dc.identifier | https://arxiv.org/abs/0901.0721 | |
| dc.identifier | http://arxiv.org/abs/0901.0721 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/216631 | |
| dc.subject | Instrumentation and Methods for Astrophysics | |
| dc.title | Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group | |
| dc.type | text |