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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