[Astronomy seminar] Reminder: Astronomy seminar today at 10:30 in FC61
Astronomy seminar announcements
seminars-announce.astro-at-su.se at lists.su.se
Fri Aug 31 08:30:22 CEST 2018
A kind reminder of today seminar.
Alexis and Angela
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Angela Adamo
Department of Astronomy
Stockholm University and Oskar Klein Centre
SE-10691 Stockholm - Sweden
tel: +46 (0)8 5537 8556
email: angela.adamo at astro.su.se
http://ttt.astro.su.se/~adamo
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> On 29 Aug 2018, at 19:06, Angela Adamo <angela.adamo at astro.su.se> wrote:
>
> Dear all,
> thanks to the prompt reply of Prof. Erb we have actually managed to schedule an excellent seminar for this coming Friday.
> Dr. Lluis Mas-Ribas has recently got his PhD in Oslo University and will move in a couple of weeks in California where he will start a post-doc a Caltech.
> He is visiting our Institute and will be around Thursday and Friday in case you are interested in talking to him.
>
> We hope you can make it! Title and abstract will follow.
> The agenda of our seminars is currently being updated on the www.astro.su.se webpage.
> We are experiencing difficulties in using the Albanova agenda, but it will be fixed soon.
>
> Kind regards,
> Alexis and Angela
>
> TITLE - Extended Diffuse Emission as a Probe of Galaxy and Reionization Physics
>
> ABSTRACT
> Two of the main questions for the Epoch or Reionzation are: (i) what sources reionized the Universe? and (ii) what is the escape fraction of ionizing
> photons from galaxies into the IGM? I will present our results demonstrating the use of the spatially extended Lya, Ha, and stellar continuum emission
> observed around star-forming galaxies from z~2 and up to z~7, and its comparison to future feasible JWST observations, to answer these two questions.
> Furthermore, I will show our recent calculations that indicate the JWST observability of the warm and hot CGM gas via the Thomson scattering of quasar
> radiation in massive galaxies, which appears to be redshift independent and thus enables measurements of the warm and hot halo gas properties, the
> baryonic content, and the impact of quasar feedback from z~0 to (at least) z~6.5 during Reionization.
>
>
> -------------------------------------------------------
> Angela Adamo
>
> Department of Astronomy
> Stockholm University and Oskar Klein Centre
> SE-10691 Stockholm - Sweden
> tel: +46 (0)8 5537 8556
> email: angela.adamo at astro.su.se
> http://ttt.astro.su.se/~adamo
> -------------------------------------------------------
>
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