[Deeppwg] Fwd: NSTAR proceedings

[Daria Sokhan]

Masking the y-scale and fit parameter, I meant. Or make it very clear that
at this stage it's a DVCS + bits of pi0 asymmetry...

Daria


On 2 December 2015 at 09:39, Daria Sokhan <daria at jlab.org> wrote:

> Dear everyone,
>
> Please also see Michel Garçon's comment below (it bounced from the list).
>
> Michel, I should have noted that the kinematics is slightly different
> between the Hall A result and mine. I will look up my average x, Q^2, t and
> also quote them.
>
> What is the general feeling on showing the BSA? I could show the plot but
> mask the y-scale, for example...
>
> Many thanks,
> Daria
>
>
> On 2 December 2015 at 08:19, Garcon Michel <Michel.Garcon at cea.fr> wrote:
>
>> Dear Daria et al.,
>>
>>
>>
>>                 I am in general in favor of waiting until there is a
>> submitted analysis note to preliminary results in proceedings, except if
>> the recognition of the work of a student or post-doc cannot wait, or if the
>> work was presented and discussed without any show stopper in the DP-PWG.
>> This being said, I accept that we have flexible rules.
>>
>>
>>
>>                 In this particular case, even for the case of BSA, the
>> fact that a number of corrections have not been done (pi0 subtraction,..),
>> combined with the observation that the result may seem at variance with
>> Hall A results where the asymmetry on the neutron was found compatible with
>> 0, should question us. You acknowledge in the text that the results may
>> still change significantly! I would then not be in favor of publishing
>> these preliminary results at this stage.
>>
>>
>>
>>                 My two cents,
>>
>>                                Michel.
>>
>>
>>
>> *_______________*
>>
>> *Michel Garçon*
>>
>> *Irfu/SPhN                                               *
>>
>> *CEA-Saclay, bât. 703                               *
>>
>> *91191 Gif-sur-Yvette cedex        *
>>
>> *France                                          *
>>
>> *Tél.:** +33 1 69 08 86 23 <%2B33%201%2069%2008%2086%2023>*
>>
>
>
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