Hi all,
I would like to better understand the procedure. I had thought that we
concluded during the F2F meeting to define the most important topics to
be discussed during the Obergurgl meeting (represented by the list put
together by Emma) and then ask the different WGs and task forces to
propose speakers for these talks. Is this correct? Or, as I understand
Dieter, is there still time for contributed talks proposed by members of
the different WGs?
Cheers,
Fabian
---------------------------------------------
Fabian Schüssler
CEA Irfu DPhP
Bât. 141, 153b
91191 Gif-sur-Yvette Cedex, France
Tel.: +33 1 69 08 30 20
Le 1 mars 2020 à 19:35, Horns, Dieter
<dieter.horns(a)desy.de
<mailto:dieter.horns@desy.de>> a écrit :
Hi Anita- we are having a short call in the PBSM working group on
Wednesday to finalize the program. We have already a table with the
talks collected on the PBSM confluence page. I hope it will be ok to
have the final schedule ready by Wednesday afternoon,
best wishes,
Dieter
------------------------------------------------------------------------
*From: *"Anita Reimer" <anita.reimer(a)uibk.ac.at
<mailto:anita.reimer@uibk.ac.at>>
*To: *"Emma de Ona Wilhelmi" <wilhelmi(a)ice.csic.es
<mailto:wilhelmi@ice.csic.es>>
*Cc: *"Hess-ap" <hess-ap(a)lsw.uni-heidelberg.de
<mailto:hess-ap@lsw.uni-heidelberg.de>>
*Sent: *Friday, 28 February, 2020 17:03:19
*Subject: *Re: [Hess-ap] Agenda: Mail to the WGs
Dear Emma, All,
first I'd like to thank you all for all your contributions to the
(I think) a fruitful F2F-meeting with lively discussions that we had
last Tuesday/Wednesday in Heidelberg.
Thanks so much, Emma, for drafting this email below. While I think it
is important to transport our envisioned structure for the AP program
of the collaboration meeting to all WGs so that everybody sees the
flow of topics, it might be difficult to coordinate it the way you
propose as some of the WGs have (wisely) already started with
collecting the talks that shall be presented at the collaboration
meeting. However, I might be wrong. Please (all) comment.
Nevertheless I have edited (below) a bit your draft email on the AP
program at the upcoming collaboration meeting to all WGs. Please
change where you find appropriate.
Meanwhile I have created a confluence page for the preparation of the
AP program at the collaboration meeting:
https://hess-confluence.desy.de/confluence/pages/viewpage.action?pageId=103…
Please fill in the talks as soon as possible. More urgent is to get a
time estimate for each topic, and for the total AP program (until
Tuesday evening if possible), so that it can be communicated to the EC
as soon as possible.
All the best,
Anita
===============================================================================================
Dear colleagues,
we had an efficient AP F2F meeting in Heidelberg beginning of this
week, where we discussed several issues, amongst others on how to
make an efficient and engaging AP program for the upcoming
collaboration meeting. We would like to change a bit the previous
structure which typically had many contributions for (sometimes not
very incremental) status reports. Rather than that, we propose to ask
the different Task/Project groups to collectively prepare a general
talk and choose a speaker that would give a scientific context and a
summary of the results. We encourage you too to include also the MWL
needs in each of the presentations.
We understand it is also important to have detailed discussions on
particular aspects of the project or analysis, therefore we also
propose to use some of the Free Time/Special Sessions slots to get
together and discuss some of these particular projects.
As preliminary agenda, we would like to have the following
contributions. You can find for each WG, some of the topics that
*could* be included, if you would like to share the status of the
project on the Col. Mtg..
*a/ Session on Galactic Center / CR diffusion *
* We envision 3 contributions including: *
o*Astrophysics *
o*Dark Matter *
o*Diffuse *
*For****"Astrophysics"
*
*- Topics under the Diffuse WG: …..*
*- Topics under the Stellar WG: Variability of the GC*
We would like to encourage those working on the Astrophysics aspects
of the GC region to organize such talk.
Please add Sabrina and Emma in the loop, we can give you more detailed
information on the expectation from this talk.
*For "Dark Matter"
*
*
*
Please add Dieter in the loop, he can give you more detailed
information on the expectation from this talk. *
*
*For "Diffuse"
*
*- Topics under the Stellar WG: LMC/SMC. *
*- Topics under the CR propagation WG: *
*
*
Please add Sabrina and Emma in the loop, we can give you more detailed
information on the expectation from this talk. **
*
*
*b/ Session on non-compact CRs Accelerators: *
o*SNR evolution *
o*Unidentified /CR PeVatrons *
o*Leptonic PeVatrons *
*For **"SNR evolution (young / old SNRs )"*
*- Topics under the SNR/PWN WG: *
***For **"Unidentified / PeVatrons"
*
*- Topics under the Stellar WG: Unidentified PeVatrons / Stellar Clusters*
*- Topics under the SNR/PWN WG: *
*
*
Please add Jacco and Emma in the loop, we can give you more detailed
information on the expectation from this talk. *
*
*
*
*For "Leptonic PeVatrons"
*
*- Topics under the Stellar WG: Binary*
*- Topics under the SNR/PWN WG: *
Please add Jacco and Emma in the loop, we can give you more detailed
information on the expectation from this talk. *
*
*
*
*c/ **Compact Objects*
o*Pulsars*
o*Microquasars *
o*Jets M87*
o*Jets monitoring / flares*
*For "Pulsars"*
*- Topics under the Stellar WG: Vela / Crab / LIV/ J1706*
Please add Emma in the loop, she can give you more detailed
information on the expectation from this talk. *
*
*For "Microquasars"*
*- Topics under the Jets: SS433*
Please add Garret and Emma in the loop, we can give you more detailed
information on the expectation from this talk. *
*
*For "Jets-M87"*
*- Topics under the Jets:
*
Please add Garret in the loop, he can give you more detailed
information on the expectation from this talk. *
*
*For "Jets monitoring/flares"*
*- Topics under the Jets: *
Please add Garret in the loop, he can give you more detailed
information on the expectation from this talk. *
*
**
*
*
*d/ Pair-halo, EBL*
*e/ GW Follow-up*
Please add Fabian in the loop, he can give you more detailed
information on the expectation from this talk. *
*
*
*
*f/ Fast variability:*
o*FRBs *
o*Primordial Black Holes
*
**For "FRBs"**
Please add Fabian in the loop, he can give you more detailed
information on the expectation from this talk. *
*
*
*
***For "Primordial Black Holes"***
**
Please add Dieter in the loop, he can give you more detailed
information on the expectation from this talk. *
*
*
*
**
**
oAnyone in the WGs is of course welcome to suggest another contributed
talk, if you think the topic is relevant and should be discussed.
Please discuss it with your WG coordinator as soon as possible.
The Free Time/Special session should be discussed in each of the WG
mailing list. Likewise you are invited to contact your WG coordinator
to suggest any relevant topic.
Am 27.02.20 um 15:54 schrieb Emma de Ona Wilhelmi:
Dear all,
I was drafting an email to the Stellar WG, but I realised that we
need a lot of coordination between different groups, if we want to
have the talks we proposed in the Agenda. I wonder then if it is
better to write a common email that we can all draft together, to
organise the contributions?
I came out with the following email. Please feel free to modify
and critisize, it is just a first draft and I didn’t even read it
twice…
Cheers
e
Dear colleagues,
we had an efficient AP F2F meeting in Heidelberg beginning of this
week, where we discussed several issues, including the new
publication policy and structure for the collaboration meeting.
Regarding the first point, publication policy, the previous
procedure has been modified to try to make the process of paper
publishing more efficient. The new structure can be found
here:*(LINK TO CONFLUENCE)*
The basic steps are the following:
New Idea -> Present it on the WG (and approved) -> Work/DATA &
presentation of (semi)final results -> Draft and circulation among
WG -> Paper Review by internal referees -> Collaboration Review ->
Paper submission
We also had a long discussion on how to make an efficient and
engaging AP program during the collaboration meeting. We would
like to somehow change a bit the previous structure with many
contributions for (sometimes not very incremental) status report.
Rather than that, we propose to ask the different Task/Project
groups to collectively prepare a general talk and choose a speaker
that would give a scientific context and a summary of the results.
We understand it is also important to have detailed discussions on
particular aspects of the analysis or project, therefore we also
propose to use some of the Free Time/Special Sessions slots to get
together and discuss some of these particular projects.
As preliminary agenda, we would like to have the following
contributions. You can find for each WG, some of the topics that
*could* be included, if you would like to share the status of the
project on the Col. Mtg.. We encourage you too to include also the
MWL needs in each of the presentations.
*1/ Session on Galactic Center / CR diffusion *
* We envision 3 contributions including: *
o*Astrophysics *
o*Dark Matter *
o*Diffuse *
*Astrophysics *
*- Topics under the Diffuse WG: …..*
*- Topics under the Stellar WG: Variability of the GC*
*We would like to encourage people working on the Astrophysics
aspects of the GC region to organise such talk. *
*Please add Sabrina and Emma in the loop, we can give you more
detailed instructions of what we expect from this talk. *
*Dark Matter *
*
*
*Diffuse *
*- Topics under the Stellar WG: LMC/SMC. *
*- Topics under the CR propagation WG: *
*
*
*Please add Sabrina and Emma in the loop, we can give you more
detailed instructions of what we expect from this talk. *
*
*
*
*
*2/ Session on CRs Accelerators: *
o*SNR evolution *
o*Unidentified /CR PeVatrons *
o*Leptonic PeVatrons *
*SNR evolution: (young / old SNRs )*
*- Topics under the SNR/PWN WG: *
***Unidentified / PeVatrons *
*- Topics under the Stellar WG: Unidentified PeVatrons / Stellar
Clusters*
*- Topics under the SNR/PWN WG: *
*
*
*Please add Jacco and Emma in the loop, we can give you more
detailed instructions of what we expect from this talk. *
*
*
*Leptonic PeVatrons *
*- Topics under the Stellar WG: Binary*
*- Topics under the SNR/PWN WG: *
*Please add Jacco and Emma in the loop, we can give you more
detailed instructions of what we expect from this talk. *
*3/ **Compact Objects*
o*Pulsars*
o*Microquasars *
o*Jets M87*
o*Jets monitoring / flares*
*Pulsars*
*- Topics under the Stellar WG: Vela / Crab / LIV/ J1706*
*Microquasars*
*- Topics under the Jets: SS433*
*
*
*Please add Garret and Emma in the loop, we can give you more
detailed instructions of what we expect from this talk. *
*Jets M87*
*- Topics under the Jets: *
*Jets monitoring/flares*
*- Topics under the Jets: *
*
*
*
*
*4/ Pair-halo EBL*
*5/GW Follow-up*
*
*
*6/ Fast variability:*
o*FRBs *
o*Fast variability related to DM – Primordial Black Holes (?)*
*7/ DM Clumps (?)***
Anyone in the WGs is of course welcome to suggest another
contributed talk, if you think the topic is relevant and should be
discussed. Please discuss it with your WG coordinator as soon as
possible.
The Free Time/Special session should be discussed in each of the
WG mailing list. Likewise you are invited to contact your WG
coordinator to suggest any relevant topic.
**
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