JWST-MIRI Integral Field Spectroscopy of high-z galaxies

Labiano, A., Álvarez-Márquez, J., Colina, L., Alonso-Herrero, A., Azzolini, R., Böker, T., Caputi, K., Eckart, A., García-Marín, M., Kendrew, S., Le Fèvre, O., Norgaard-Nielsen, H. U., Ostlin, G., Pérez-González, P., Pye, J., Van der Werf, P., Walter, F., Ward, M. & Wright, G., 1-Mar-2019, p. 218. 1 p.

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  • JWST-MIRI Integral Field Spectroscopy of high-zgalaxies

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  • A. Labiano
  • J. Álvarez-Márquez
  • L. Colina
  • A. Alonso-Herrero
  • R. Azzolini
  • T. Böker
  • K. Caputi
  • A. Eckart
  • M. García-Marín
  • S. Kendrew
  • O. Le Fèvre
  • H. U. Norgaard-Nielsen
  • G. Ostlin
  • P. Pérez-González
  • J. Pye
  • P. Van der Werf
  • F. Walter
  • M. Ward
  • G. Wright
Due to its sensitivity and spectral coverage, the James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) is optimum to detect the H_α emission line on sources at redshifts beyond 6.7. The European MIRI Guaranteed Time Observations (GTO, PI: G. Wright) will dedicate 65 hours to observe three Ly_α emitters (LAEs) and two quasars in the Epoch of Reionization (EoR), plus two dusty star-forming galaxies (DSFG) at z̃4-7. We present the realistic simulations we created in preparation for the MRS data expected for the High- z GTO program.
Original languageEnglish
Number of pages1
Publication statusPublished - 1-Mar-2019
EventThe XIII Scientific Meeting of the Spanish Astronomical Society - Salamanca, Spain
Duration: 16-Jul-201820-Jul-2018


ConferenceThe XIII Scientific Meeting of the Spanish Astronomical Society


The XIII Scientific Meeting of the Spanish Astronomical Society


Salamanca, Spain

Event: Conference

ID: 119049276