Challenges in Panchromatic Modelling With Next Generation Facilities - Proceedings of the International Astronomical Union Symposia and Colloquia

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.

ISBN:	9781108471473
Publisher:	Cambridge University Press
Imprint:	Cambridge University Press
Published date:	30 Jul 2020
DEWEY:	523.112
DEWEY edition:	23
Language:	English
Number of pages:	xvii, 329
Weight:	710g
Height:	254mm
Width:	180mm
Spine width:	17mm

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