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{ "item_title" : "Challenges in Panchromatic Modelling with Next Generation Facilities (Iau S341)", "item_author" : [" Médéric Boquien", "Elisabeta Lusso", "Carlotta Gruppioni "], "item_description" : "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.", "item_img_path" : "https://covers2.booksamillion.com/covers/bam/1/10/847/147/1108471471_b.jpg", "price_data" : { "retail_price" : "168.00", "online_price" : "168.00", "our_price" : "168.00", "club_price" : "168.00", "savings_pct" : "0", "savings_amt" : "0.00", "club_savings_pct" : "0", "club_savings_amt" : "0.00", "discount_pct" : "10", "store_price" : "" } }
Challenges in Panchromatic Modelling with Next Generation Facilities (Iau S341)|Médéric Boquien

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

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Overview

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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Details

  • ISBN-13: 9781108471473
  • ISBN-10: 1108471471
  • Publisher: Cambridge University Press
  • Publish Date: July 2020
  • Dimensions: 9.87 x 7.05 x 0.69 inches
  • Shipping Weight: 1.5 pounds
  • Page Count: 346

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