Dear All,
after having finessed the H.E.S.S.-collaboration meeting, we shall
aim for our next HESS-AP call sometime during the first December week.
In order to maximize participation, I would thus like to open a poll to
probe your current availabilities:
https://framadate.uibk.ac.at/studs.php?sondage=hp1tebxs43sghimr
I'd like to ask you for filling the poll by 25 Nov.
The agenda can be found at:
https://hess-confluence.desy.de/confluence/display/HESS/Zoom+meeting+2021-1…
As always, please feel free to add further agenda items as you feel
appropriate.
Best wishes,
Anita
reminder
Meeting-ID: 954 7507 6954
Kenncode: 427024
---------------------------- Original Message ----------------------------
Subject: HESS-AP Call Friday, Feb 25, 9:30
From: "Stefan Wagner" <swagner(a)lsw.uni-heidelberg.de>
Date: Thu, February 24, 2022 20:50
To: "Hess-ap" <hess-ap(a)lsw.uni-heidelberg.de>
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Dear all,
thank you all very much for responding despite the short notice.
It appears that we will be able to run a meeting with a significant
fraction of our team. Between the slots 9-10 and 10-11 we could almost
have all groups participating. I hence suggest to meet 9:30-10:30 such
that most of you can at least attend part-time.
The zoom connection details are listed below, the agenda will be
> Items are (very brief summaries on: / your concerns regarding:)
> legacy program
> proposals 2022
> publications
> conferences 2022
> collaboration meeting 2022
> cooperation with other facilities
Best regards,
Stefan
LSW Königstuhl lädt Sie zu einem geplanten Zoom-Meeting ein.
Thema: HESS-AP
Uhrzeit: 25.Feb..2022 09:30 AM Amsterdam, Berlin, Rom, Stockholm, Wien
Zoom-Meeting beitreten
https://zoom.us/j/95475076954?pwd=YmV4U0FjcTVJRTQ5SERqWURUMnA4dz09
Meeting-ID: 954 7507 6954
Kenncode: 427024
Schnelleinwahl mobil
+496950500951,,95475076954#,,,,*427024# Deutschland
+496950500952,,95475076954#,,,,*427024# Deutschland
Einwahl nach aktuellem Standort
+49 69 5050 0951 Deutschland
+49 69 5050 0952 Deutschland
+49 695 050 2596 Deutschland
+49 69 7104 9922 Deutschland
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Meeting-ID: 954 7507 6954
Kenncode: 427024
Ortseinwahl suchen: https://zoom.us/u/ahp9pWdqS
> Dear all,
>
> following up on our last meeting, I had hoped for a while that we would
> have progress regarding the HESS governance for the extension phase. This
> appears to take more time than assumed. While this continues to affect the
> process of identifying a successor to Anita as head of the astrophysics
> dept., I would like to limit potential collateral damage to our program
> and suggest to have a brief interim meeting.
>
> While this is very short notice, I suggest to follow the 'friday morning
> slot' of the astrophysics department for a mtg. _tomorrow_ in case we can
> meet with at least half of the department.
>
> Items are (very brief summaries on: / your concerns regarding:)
> legacy program
> proposals 2022
> publications
> conferences 2022
> collaboration meeting 2022
> cooperation with other facilities
>
> There has been a spread in preferred times, and I ask for your preferences
> for tomorrow on
> https://terminplaner.dfn.de/oQvZRICvfFgbLba8
> I will set up a zoom, in case we can meet with >4 people
>
> Best regards,
> Stefan
>
>
>
Dear AP team,
I've been in discussions with Phil Edwards (Head of CSIRO Science Operations for ATNF, operating the ATCA radio facility) regarding AGN targets for their regular monitoring campaigns with the ATCA facility.
Phil has expressed a keen interest in improving or optimising the monitoring cadence for the various TeV AGN that HESS is observing. The results of this feed into the publicly available ATCA Calibrator Database
https://www.narrabri.atnf.csiro.au/calibrators/calibrator_database.html
and also to the TANAMI project, carrying out VLBI for hi-res studies of active AGN in the south.
https://pulsar.sternwarte.uni-erlangen.de/tanami/about/
As you may know, these projects are beginning to shift their focus to include TeV-detected AGN in recent times.
Would HESS be willing to share with Phil our AGN observing schedule, planned and achieved? Precise observation times are not needed.
A rough schedule on a monthly (period) or even weekly (if possible) would be sufficient. The information would be kept confidential and only appear in public in the calibrator database in the form of higher-cadence sampling for those particular AGN, in they are not already.
It's expected that major TeV flares from HESS would be communicated via ATels, but if needed, we could also consider sharing such information privately to increase the cadence for their ATCA monitoring. I'd be happy to draft a basic information sharing agreement if it's thought that is needed for these special cases.
all the best
Gavin..
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Gavin Rowell ph +61883138374
High Energy Astrophysics Group fax +61883134380
School of Physical Sciences gavin.rowell(a)adelaide.edu.au
University of Adelaide 5005, AUSTRALIA
web: http://www.physics.adelaide.edu.au/astrophysics/gpr/
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