Challenges in Panchromatic Modelling with Next Generation Facilities (IAU S341)

Challenges in Panchromatic Modelling with Next Generation Facilities (IAU S341)
Mederic Boquien, Elisabetta Lusso, Carlotta Gruppioni, Patricia Tissera
RRP:
NZ$ 186.95
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NZ$ 168.26
Hardback
Not defined - 500pg
30 Jun 2020 UK
International import eta 7-19 days
9781108471473
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Over the past decade, modelling the panchromatic emission of galaxies has become one of the key tools in measuring their properties. As new and next-generation facilities progressively herald a new era in observational astronomy, we face new and specific challenges: LSST (recently named the Vera C. Rubin Observatory) and SKA will provide us with an avalanche of data; the advent of e-ROSITA and the preparation for Athena make it ever more pressing to include X-ray emission into the standard UV to radio panchromatic models; JWST will observe the first galaxies with extreme stellar populations; and, in the meantime, ALMA is already starting to provide us with remarkable dust and metal observations at high redshift. The proceedings of IAU Symposium 341 offer a broad overview of the state of the field from theoreticians, modellers, and observers to present and discuss the current frontier in the panchromatic modelling of galaxies.

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