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] > <javascript:_e(%7B%7D,'cvml','[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
