27 Feb
2020
27 Feb
'20
3:54 p.m.
Dear All,
The multi-year heritage programmes should address a science question which cannot be
answered with many single observations but requires the entire set of observations which
will amount to a very long observing time (e.g. for a study of the evolution of accreting
compact objects, you need to observe a large set of these sources). I am not sure if a
deep observation of the Norma arm or the follow-up of unidentified sources will make a
good enough science case. The Geminga halo is interesting, but I wonder if we can expect
to detect any related X-ray emission.
Best,
Manami
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Prof. Dr. Manami Sasaki
Dr. Karl Remeis Observatory
Erlangen Centre for Astroparticle Physics
Friedrich-Alexander University Erlangen-Nürnberg
Sternwartstr. 7
96049 Bamberg
Germany
Phone: +49-951-95222-19
Email: manami.sasaki(a)fau.de
On 26. Feb 2020, at 08:34, Anita Reimer
<anita.reimer(a)uibk.ac.at> wrote:
Dear Jacco, Gerd, Regis, Manami,
at the F2F-meeting of the Astrophysics WG conveners we have been discussing the
possibility of HESS submitting a proposal to the recently (beginning of this month)
announced XMM Multi-Year Heritage Programms
https://www.cosmos.esa.int/web/xmm-newton/news-20200203
and collected ideas as sketched in the pdf attached.
As you being experts and experienced in both the X-ray and VHE regime we would like to
get your opinion, and enquire whether you would be interested in and have the time to
playing a significant role in this endeavor. We need to decide quickly whether we should
give it a try (your expert opinion is here extremely important): The deadline of LoI
submission is already next Monday!
All the best,
Anita
<XMMLegacy.pdf>