Dear all,

I had a chat with Maria yesterday and she is keen to present the final results (which are part of her PhD). We discussed a bit how to do it and she is coordinating it with Nukri and Emmanuel to have a contribution on LMC/SMC physics (diffuse and population) just after the Diffuse Galactic talk. She is not coming to Obergurgl, so either she does it online (if possible) or someone gives the talk for her.
Cheers
e


On 3 Mar 2020, at 10:32, Jacco Vink <j.vink@uva.nl> wrote:

Hi All,

I am catching up with my emails now.

Some comment on the SNR topics: I would like to include N132D. Maria Haupt emailed me she is not attending.
She is currently leading the SN1987A and LMC efforts (I think sources not the diffuse part, but I need to check). But she told me she can provide some slides.

Jacco

On 25 Feb 2020, at 17:08, Emma de Ona Wilhelmi <wilhelmi@ice.csic.es> wrote:

Updated version. To be discussed on the context of the Agenda:

1/ Session on Future with HESS – Priorities on the Science Topics 

 

2/ Session on Selected Projects 

 

·       Galactic Center / CR diffusion:

o   Astrophysics (could include variability)

o   Dark Matter

o   Diffuse (could include  LMC / SMC)

 

·       PeVatrons

o   SNR evolution (could include Kepler/SN1987a)

o   Unidentified (could include Wd1 / J1908)

o   Leptonic PeVatrons (could include Binary / PWNe  / Geminga)

·       Compact Objects

o   Pulsars (could include Vela/PSRJ1706/Crab + LIV)

o   Microquasars – SS 433

o   Jets M87

o   Jets monitoring / flares

·       Pair-halo EBL

·       GW Follow-up

·       Fast variability:

o   FRBs  

o   Fast variability related to DM – Primordial Black Holes (?)

·       DM Clumps (?)

·       MWL coverage (?)

  

3/ Special Sessions on Individual Projects (and report on the general meeting?)

  



On 25 Feb 2020, at 16:58, Emma de Ona Wilhelmi <wilhelmi@ice.csic.es> wrote:

Session on Future with HESS – Priorities on the Science

 

Session on Selected Topics 

 

·       Galactic Center:

o   Astrophysics (could include variability)

o   Diffuse (could include  LMC / SMC)

o   Dark Matter

 

·       PeVatrons

o   SNR evolution (could include Kepler/SN1987a)

o   Unidentified (could include Wd1 / J1908)

o   Leptonic PeVatrons (could include Binary / PWNe  / Geminga)

·       Compact Objects

o   Pulsars (could include Vela/PSRJ1706/Crab + LIV)

o   Microquasars – SS 433

o   Jets M87

o   Jets monitoring / flares

·       Pair-halo EBL

·       GW Follow-up

·       Fast variability:

o   FRBs  

o   Fast variability related to DM – Primordial Black Holes (?)

·       DM Clumps (?)

·       MWL coverage (?)

 

 

 


On 25 Feb 2020, at 14:47, Anita Reimer <anita.reimer@uibk.ac.at> wrote:


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