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Labiano, A.; Alvarez-Marquez, J.; Colina, L.; Alonso-Herrero, A.; Azzolini, R.; Boker, T.; Caputi, K.; Eckart, A.; Garcia-Marin, M.; Kendrew, S.; Le Fevre, O.; Norgaard- Nielsen, H.U.; Ostlin, G.; Perez-Gonzalez, P.; Pye, J.; Van der Werf, P.; Walter, F.; Ward, M.; Wright, G.
Proceedings of the 13th Scientific Meeting of the Spanish Astronomical Society (XIII SEA 2018)2018
Proceedings of the 13th Scientific Meeting of the Spanish Astronomical Society (XIII SEA 2018)2018
AbstractAbstract
[en] Due to its sensitivity and spectral coverage, the James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) is optimum to detect the H 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 emitters (LAEs) and two quasars in the Epoch of Reionization (EoR), plus two dusty star-forming galaxies (DSFG) at z4-7. We present the realistic simulations we created in preparation for the MRS data expected for the High- z GTO program.
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675 p; 2018; 1 p; XIII SEA: 13. Scientific Meeting of the Spanish Astronomical Society; XIII SEA: Reunion cientifica de la Sociedad Española de Astronomia; Salamanca (Spain); 16-20 Jul 2018; Available from https://www.sea-astronomia.es/publicaciones/proceeding#2018
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