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Challenges in Panchromatic Modelling With Next Generation Facilities: Proceedings of the 341St Symposium of the International Astronomical Union Held in Osaka, Japan 12-16 November 2016 (en Inglés)
Boquien, Médéric (Edt); Lusso, Elisabetta (Edt); Gruppioni, Carlotta (Edt); Tissera, Patricia (Edt) (Autor)
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Cambridge Univ Pr
· Tapa Dura
Challenges in Panchromatic Modelling With Next Generation Facilities: Proceedings of the 341St Symposium of the International Astronomical Union Held in Osaka, Japan 12-16 November 2016 (en Inglés) - Boquien, Médéric (Edt); Lusso, Elisabetta (Edt); Gruppioni, Carlotta (Edt); Tissera, Patricia (Edt)
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Reseña del libro "Challenges in Panchromatic Modelling With Next Generation Facilities: Proceedings of the 341St Symposium of the International Astronomical Union Held in Osaka, Japan 12-16 November 2016 (en Inglés)"
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.