JWST-MIRI Integral Field Spectroscopy of high-z galaxies

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

JWST-MIRI Integral Field Spectroscopy of high-z galaxies

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

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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.

Originele taal-2	English
Pagina's	218
Aantal pagina's	1
Status	Published - 1-mrt.-2019
Evenement	The XIII Scientific Meeting of the Spanish Astronomical Society - Salamanca, Spain Duur: 16-jul.-2018 → 20-jul.-2018

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Conference	The XIII Scientific Meeting of the Spanish Astronomical Society
Land/Regio	Spain
Stad	Salamanca
Periode	16/07/2018 → 20/07/2018

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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. (2019). JWST-MIRI Integral Field Spectroscopy of high-z galaxies. 218. Abstract van The XIII Scientific Meeting of the Spanish Astronomical Society , Salamanca, Spain. https://ui.adsabs.harvard.edu/abs/2019hsax.conf..218L

@conference{7080d0de7dce4887926d97769445b234,

title = "JWST-MIRI Integral Field Spectroscopy of high-z galaxies",

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 {\~z}4-7. We present the realistic simulations we created in preparation for the MRS data expected for the High- z GTO program.",

author = "A. Labiano and J. {\'A}lvarez-M{\'a}rquez and L. Colina and A. Alonso-Herrero and R. Azzolini and T. B{\"o}ker and K. Caputi and A. Eckart and M. Garc{\'i}a-Mar{\'i}n and S. Kendrew and {Le F{\`e}vre}, O. and Norgaard-Nielsen, {H. U.} and G. Ostlin and P. P{\'e}rez-Gonz{\'a}lez and J. Pye and {Van der Werf}, P. and F. Walter and M. Ward and G. Wright",

year = "2019",

month = mar,

day = "1",

language = "English",

pages = "218",

note = "The XIII Scientific Meeting of the Spanish Astronomical Society ; Conference date: 16-07-2018 Through 20-07-2018",

}

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, HU, Ostlin, G, Pérez-González, P, Pye, J, Van der Werf, P, Walter, F, Ward, M & Wright, G 2019, 'JWST-MIRI Integral Field Spectroscopy of high-z galaxies', The XIII Scientific Meeting of the Spanish Astronomical Society , Salamanca, Spain, 16/07/2018 - 20/07/2018 blz. 218. <https://ui.adsabs.harvard.edu/abs/2019hsax.conf..218L>

TY - CONF

T1 - JWST-MIRI Integral Field Spectroscopy of high-z galaxies

AU - Labiano, A.

AU - Álvarez-Márquez, J.

AU - Colina, L.

AU - Alonso-Herrero, A.

AU - Azzolini, R.

AU - Böker, T.

AU - Caputi, K.

AU - Eckart, A.

AU - García-Marín, M.

AU - Kendrew, S.

AU - Le Fèvre, O.

AU - Norgaard-Nielsen, H. U.

AU - Ostlin, G.

AU - Pérez-González, P.

AU - Pye, J.

AU - Van der Werf, P.

AU - Walter, F.

AU - Ward, M.

AU - Wright, G.

PY - 2019/3/1

Y1 - 2019/3/1

N2 - 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.

AB - 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.

M3 - Abstract

SP - 218

T2 - The XIII Scientific Meeting of the Spanish Astronomical Society

Y2 - 16 July 2018 through 20 July 2018

ER -

JWST-MIRI Integral Field Spectroscopy of high-z galaxies

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