Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT

Freigegeben

Konferenzband

JWST-MIRI Integral Field Spectroscopy of high-z galaxies

MPG-Autoren

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;

Externe Ressourcen
Volltexte (beschränkter Zugriff)
Für Ihren IP-Bereich sind aktuell keine Volltexte freigegeben.
Volltexte (frei zugänglich)
Es sind keine frei zugänglichen Volltexte in PuRe verfügbar
Ergänzendes Material (frei zugänglich)
Es sind keine frei zugänglichen Ergänzenden Materialien verfügbar
Zitation

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.


Zitierlink: https://hdl.handle.net/21.11116/0000-0005-D096-6
Zusammenfassung
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.