The Lyman-alpha forest according to LUQAS
| dc.creator | Viel, M. | |
| dc.creator | Haehnelt, M. | |
| dc.creator | Kim, T. -S. | |
| dc.creator | Carswell, B. | |
| dc.creator | Cristiani, S. | |
| dc.creator | Heavens, A. | |
| dc.creator | Hernquist, L. | |
| dc.creator | Matarrese, S. | |
| dc.creator | Springel, V. | |
| dc.date | 2004-05-28 | |
| dc.date.accessioned | 2026-07-07T02:13:20Z | |
| dc.date.available | 2026-07-07T02:13:20Z | |
| dc.description | We use the LUQAS sample of 27 high resolution, high signal-to-noise QSO absorption spectra (Kim et al. 2004) and the results from Croft et al. (2002) together with a suite of high-resolution hydro-dynamical simulations run with the GADGET-II code, to infer the linear dark matter power spectrum on scales of \~ 0.3-30 Mpc at z=2.125 and at z=2.72. | |
| dc.description | 4 pages, 2 figures; Talk given by M. Viel at the XXXIXth Rencontres de Moriond on "Exploring the Universe", La Thuile, Italy, March 28 - April 4, 2004 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0405584 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0405584 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7781 | |
| dc.subject | Astrophysics | |
| dc.title | The Lyman-alpha forest according to LUQAS | |
| dc.type | text |