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JWST-MIRI Integral Field Spectroscopy of high-z galaxies

MPS-Authors

Labiano,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Álvarez-Márquez,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Colina,  L.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Alonso-Herrero,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Azzolini,  R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Böker,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Caputi,  K.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Eckart,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

García-Marín,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kendrew,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Le Fèvre,  O.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Norgaard-Nielsen,  H. U.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ostlin,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pérez-González,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pye,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Van der Werf,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Walter,  F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ward,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Wright,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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Citation

Labiano, A., Álvarez-Márquez, J., Colina, L., Alonso-Herrero, A., Azzolini, R., Böker, T., et al. (2019). JWST-MIRI Integral Field Spectroscopy of high-z galaxies.


Cite as: https://hdl.handle.net/21.11116/0000-0005-D096-6
Abstract
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.