{ "id": "1905.02759", "version": "v1", "published": "2019-05-07T18:29:20.000Z", "updated": "2019-05-07T18:29:20.000Z", "title": "Dark-ages Reionization and Galaxy Formation Simulation - XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations", "authors": [ "Yisheng Qiu", "Simon J. Mutch", "Elisabete da Cunha", "Gregory B. Poole", "J. Stuart B. Wyithe" ], "comment": "15 pages, 10 figure. Submited to MNRAS", "categories": [ "astro-ph.GA" ], "abstract": "We present a new analysis of high-redshift UV observations using a semi-analytic galaxy formation model, and provide self-consistent predictions of the infrared excess (IRX) - $\\beta$ relations and cosmic star formation rate density. We combine the Charlot & Fall dust attenuation model with the Meraxes semi-analytic model, and explore three different parametrisations for the dust optical depths, linked to star formation rate, dust-to-gas ratio and gas column density respectively. A Bayesian approach is employed to statistically calibrate model free parameters including star formation efficiency, mass loading factor, dust optical depths and reddening slope directly against UV luminosity functions and colour-magnitude relations at z ~ 4 - 7. The best-fit models show excellent agreement with the observations. We calculate IRX using energy balance arguments, and find that the large intrinsic scatter in the IRX -$\\beta$ plane is driven by the specific star formation rate. Additionally, the difference among the three dust models suggests a factor of two systematic uncertainty in the dust-corrected star formation rate when using the Meurer IRX - $\\beta$ relation at z > 4.", "revisions": [ { "version": "v1", "updated": "2019-05-07T18:29:20.000Z" } ], "analyses": { "keywords": [ "cosmic star formation rate density", "galaxy formation simulation", "uv observations", "infrared excess", "calibrate model free parameters" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable" } } }