mK On Thu, Dec 3, 2015 at 6:30 AM Jonathan Pober <[email protected]> wrote:
> 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 >> >> >> >
