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dc.contributor.authorViel, Men
dc.contributor.authorHaehnelt, Martinen
dc.contributor.authorKim, T-Sen
dc.contributor.authorCarswell, Ben
dc.contributor.authorCristiani, Sen
dc.contributor.authorHeavens, Aen
dc.contributor.authorHernquist, Len
dc.contributor.authorMatarrese, Sen
dc.contributor.authorSpringel, Ven
dc.date.accessioned2018-09-05T12:44:56Z
dc.date.available2018-09-05T12:44:56Z
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/279468
dc.description.abstractWe 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.subjectastro-phen
dc.subjectastro-phen
dc.titleThe Lyman-alpha forest according to LUQASen
dc.typeConference Object
dc.identifier.doi10.17863/CAM.26842
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserveden
dc.contributor.orcidHaehnelt, Martin [0000-0001-8443-2393]
rioxxterms.typeConference Paper/Proceeding/Abstracten
rioxxterms.freetoread.startdate2019-08-28


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