20 or 30 mK or mK^2? On Wed, Dec 2, 2015 at 11:47 PM, Adrian Liu <[email protected]> wrote:
> Yes. They have both P(kperp,kpara) limits as well as P(k) limits. No > mention of the variance method today. > > On Dec 2, 2015, at 9:42 PM, danny jacobs <[email protected]> wrote: > > But this is a power spectrum limit rather than with the variance method? > > On Wednesday, December 2, 2015, Saul Kohn <[email protected]> wrote: > >> Hi all, >> >> To follow this up, Ger made a LOFAR EoR project overview presentation >> (probably the same one as Dave was mentioning) in Albuquerque this >> afternoon. >> >> They were hazy on the details of power spectrum estimation from their >> images, but he quoted *preliminary* limits of between 20 and 30mK for >> redshifts 7.5 to 10, k~0.05 Mpc^-1 using 155 hours of data. Their estimate >> on systematics comes from Stokes V, which was at levels ~ 10mK, so >> intersecting with the higher-power EoR models. On the slide it quoted >> "Zaroubi et al. 2016", so I guess we can expect to see something official >> next year. >> >> Saul >> >> On Wed, Nov 11, 2015 at 5:06 PM, DAVID DEBOER <[email protected]> >> wrote: >> >>> To clarify a bit, I’m not sure that Michiel’s statement applies to >>> anything new, but rather that there was some possibility that Ger had made >>> a presentation somewhere regarding a limit. >>> >>> Dave >>> >> >> > > -- > Sent from Gmail Mobile > > >
