Spatially resolved Hα and ionizing photon production efficiency in the lensed galaxy MACS1149-JD1 at a redshift of 9.11

We present MIRI/JWST medium-resolution spectroscopy (MRS) and imaging (MIRIM) of the lensed galaxy MACS1149-JD1 at a redshift of z = 9.1092 ± 0.0002, when the Universe was about 530 Myr old. We detect, for the first time, spatially resolved Hα emission in a galaxy at a redshift above nine. The struc...

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Hauptverfasser: Álvarez Márquez, Javier (VerfasserIn) , Colina, L. (VerfasserIn) , Gómez, A. Crespo (VerfasserIn) , Rinaldi, P. (VerfasserIn) , Melinder, J. (VerfasserIn) , Östlin, G. (VerfasserIn) , Annunziatella, M. (VerfasserIn) , Labiano, A. (VerfasserIn) , Bik, A. (VerfasserIn) , Bosman, Sarah (VerfasserIn) , Greve, T. R. (VerfasserIn) , Wright, G. (VerfasserIn) , Alonso-Herrero, A. (VerfasserIn) , Boogaard, Leindert A. (VerfasserIn) , Azollini, R. (VerfasserIn) , Caputi, K. I. (VerfasserIn) , Costantin, L. (VerfasserIn) , Eckart, A. (VerfasserIn) , García-Marín, M. (VerfasserIn) , Gillman, S. (VerfasserIn) , Hjorth, J. (VerfasserIn) , Iani, E. (VerfasserIn) , Ilbert, O. (VerfasserIn) , Jermann, I. (VerfasserIn) , Langeroodi, D. (VerfasserIn) , Meyer, R. (VerfasserIn) , Peißker, F. (VerfasserIn) , Pérez-González, P. (VerfasserIn) , Pye, J. P. (VerfasserIn) , Tikkanen, T. (VerfasserIn) , Topinka, M. (VerfasserIn) , Werf, P. van der (VerfasserIn) , Walter, Fabian (VerfasserIn) , Henning, Thomas (VerfasserIn) , Ray, T. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: June 2024
In: Astronomy and astrophysics
Year: 2024, Jahrgang: 686, Pages: 1-11
ISSN:1432-0746
DOI:10.1051/0004-6361/202347946
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202347946
Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2024/06/aa47946-23/aa47946-23.html
Volltext
Verfasserangaben:J. Álvarez-Márquez, L. Colina, A. Crespo Gómez, P. Rinaldi, J. Melinder, G. Östlin, M. Annunziatella, A. Labiano, A. Bik, S. Bosman, T.R. Greve, G. Wright, A. Alonso-Herrero, L. Boogaard, R. Azollini, K.I. Caputi, L. Costantin, A. Eckart, M. García-Marín, S. Gillman, J. Hjorth, E. Iani, O. Ilbert, I. Jermann, D. Langeroodi, R. Meyer, F. Peißker, P. Pérez-González, J. P. Pye, T. Tikkanen, M. Topinka, P. van der Werf, F. Walter, Th. Henning, and T. Ray

MARC

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245 1 0 |a Spatially resolved Hα and ionizing photon production efficiency in the lensed galaxy MACS1149-JD1 at a redshift of 9.11  |c J. Álvarez-Márquez, L. Colina, A. Crespo Gómez, P. Rinaldi, J. Melinder, G. Östlin, M. Annunziatella, A. Labiano, A. Bik, S. Bosman, T.R. Greve, G. Wright, A. Alonso-Herrero, L. Boogaard, R. Azollini, K.I. Caputi, L. Costantin, A. Eckart, M. García-Marín, S. Gillman, J. Hjorth, E. Iani, O. Ilbert, I. Jermann, D. Langeroodi, R. Meyer, F. Peißker, P. Pérez-González, J. P. Pye, T. Tikkanen, M. Topinka, P. van der Werf, F. Walter, Th. Henning, and T. Ray 
246 3 3 |a Spatially resolved H alpha and ionizing photon production efficiency in the lensed galaxy MACS1149-JD1 at a redshift of 9.11 
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520 |a We present MIRI/JWST medium-resolution spectroscopy (MRS) and imaging (MIRIM) of the lensed galaxy MACS1149-JD1 at a redshift of z = 9.1092 ± 0.0002, when the Universe was about 530 Myr old. We detect, for the first time, spatially resolved Hα emission in a galaxy at a redshift above nine. The structure of the Hα emitting gas consists of two clumps, S and N, carrying about 60% and 40% of the total flux, respectively. The total Hα luminosity implies an instantaneous star-formation rate in the range of 3.2 ± 0.3 and 5.3 ± 0.4 M⊙ yr−1 for sub-solar and solar metallicities. The ionizing photon production efficiency, log(ζion), shows a spatially resolved structure with values of 25.55 ± 0.03; 25.47 ± 0.03; and 25.91 ± 0.09 Hz erg−1 for the integrated galaxy and clumps S and N, respectively. The Hα rest-frame equivalent width, EW0 (Hα), is 726−182+660 Å for the integrated galaxy, but it presents extreme values of 531−96+300 Å and ≥1951 Å for clumps S and N, respectively. The spatially resolved ionizing photon production efficiency is within the range of values measured in galaxies at a redshift above six and well above the canonical value (25.2 ± 0.1 Hz erg−1). The EW0 (Hα) is a factor of two lower than the predicted value at z = 9.11 based on the extrapolation of the evolution of the EW0 (Hα) with redshifts, ∝(1 + z)2.1, including galaxies detected with JWST. The extreme difference of the EW0 (Hα) for clumps S and N indicates the presence of a recent (< 5 Myr) stellar burst in clump N and a star formation over a larger period of time (e.g., ∼50 Myr) in clump S. The different ages of the stellar population place MACS1149-JD1 and clumps N and S at different locations in the log(ζion) to EW0 (Hα) plane and above the main relation defined from intermediate- and high-redshift (z = 3 − 7) galaxies detected with JWST. Finally, clump S and N show very different Hα kinematics, with velocity dispersions of 56 ± 4 km s−1 and 113 ± 33 km s−1, likely indicating the presence of outflows or increased turbulence in clump N. The dynamical mass Mdyn = (2.4 ± 0.5) × 109 M⊙, obtained from the size of the integrated Hα ionized nebulae and its velocity dispersion, is within the range previously measured with the spatially resolved [OIII]88 μm line. 
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700 1 |a Gómez, A. Crespo  |e VerfasserIn  |4 aut 
700 1 |a Rinaldi, P.  |e VerfasserIn  |4 aut 
700 1 |a Melinder, J.  |e VerfasserIn  |4 aut 
700 1 |a Östlin, G.  |e VerfasserIn  |4 aut 
700 1 |a Annunziatella, M.  |e VerfasserIn  |4 aut 
700 1 |a Labiano, A.  |e VerfasserIn  |4 aut 
700 1 |a Bik, A.  |e VerfasserIn  |4 aut 
700 1 |a Bosman, Sarah  |e VerfasserIn  |0 (DE-588)1297436172  |0 (DE-627)185378124X  |4 aut 
700 1 |a Greve, T. R.  |e VerfasserIn  |4 aut 
700 1 |a Wright, G.  |e VerfasserIn  |4 aut 
700 1 |a Alonso-Herrero, A.  |e VerfasserIn  |4 aut 
700 1 |a Boogaard, Leindert A.  |e VerfasserIn  |0 (DE-588)1224829727  |0 (DE-627)1744304718  |4 aut 
700 1 |a Azollini, R.  |e VerfasserIn  |4 aut 
700 1 |a Caputi, K. I.  |e VerfasserIn  |4 aut 
700 1 |a Costantin, L.  |e VerfasserIn  |4 aut 
700 1 |a Eckart, A.  |e VerfasserIn  |4 aut 
700 1 |a García-Marín, M.  |e VerfasserIn  |4 aut 
700 1 |a Gillman, S.  |e VerfasserIn  |4 aut 
700 1 |a Hjorth, J.  |e VerfasserIn  |4 aut 
700 1 |a Iani, E.  |e VerfasserIn  |4 aut 
700 1 |a Ilbert, O.  |e VerfasserIn  |4 aut 
700 1 |a Jermann, I.  |e VerfasserIn  |4 aut 
700 1 |a Langeroodi, D.  |e VerfasserIn  |4 aut 
700 1 |a Meyer, R.  |e VerfasserIn  |4 aut 
700 1 |a Peißker, F.  |e VerfasserIn  |4 aut 
700 1 |a Pérez-González, P.  |e VerfasserIn  |4 aut 
700 1 |a Pye, J. P.  |e VerfasserIn  |4 aut 
700 1 |a Tikkanen, T.  |e VerfasserIn  |4 aut 
700 1 |a Topinka, M.  |e VerfasserIn  |4 aut 
700 1 |a Werf, P. van der  |e VerfasserIn  |4 aut 
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700 1 |a Ray, T.  |e VerfasserIn  |4 aut 
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