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] > <mailto:[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
