Re: [Hess-ap] Agenda: Mail to the WGs

2 Mar 2020

Hi Dieter,
to have the final schedule by Wednesday afternoon is perfectly fine. If
I could get a rough estimate of the total time (no exact breakdown nor
titles nor corresponding speakers must be known at this stage) by
Tuesday evening though, would be very helpful for me to give the EC at
the Wednesday morning meeting a rough estimate of the total time the
Astrophysics Department would need at the collaboration meeting. Would
this be possible?
All the best,
Anita
On 01/03/2020 19:35, Horns, Dieter wrote:
...
  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" &lt;anita.reimer(a)uibk.ac.at&gt;
 *To: *"Emma de Ona Wilhelmi" &lt;wilhelmi(a)ice.csic.es&gt;
 *Cc: *"Hess-ap" &lt;hess-ap(a)lsw.uni-heidelberg.de&gt;
 *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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Re: [Hess-ap] Agenda: Mail to the WGs