1. The NOEMA observations of GN-z11: constraining the neutral interstellar medium and dust formation in the heart of cosmic reionization at z = 10.6.
- Author
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Fudamoto, Y, Oesch, P A, Walter, F, Decarli, R, Carilli, C L, Ferrara, A, Barrufet, L, Bouwens, R, Dessauges-Zavadsky, M, Nelson, E J, Dannerbauer, H, Illingworth, G, Inoue, A K, Marques-Chaves, R, Pérez-Fournon, I, Riechers, D A, Schaerer, D, Smit, R, Sugahara, Y, and van der Werf, P
- Subjects
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INTERSTELLAR medium , *INTERPLANETARY dust , *GALACTIC redshift , *RADIATIVE transfer , *MOLECULAR weights , *SIGMA receptors , *GALAXY formation , *SUBMILLIMETER astronomy - Abstract
We present results of dust continuum and [C ii ] |$\, 158\, {\rm \mu m}$| emission line observations of a remarkably UV luminous (M UV = −21.6) galaxy at z = 10.603: GN-z11. Using the Northern Extended Millimeter Array (NOEMA), observations have been carried out over multiple observing cycles. We achieved a high sensitivity resulting in a |$\lambda _{\rm rest}=160\, {\rm \mu m}$| continuum |$1\, \sigma$| sensitivity of |$13.0\, \rm {\mu Jy \, beam}^{ -1}$| and a [C ii ] emission line |$1\, \sigma$| sensitivity of |$31\, \rm {mJy\, beam^{ -1}\, km \, s}^{ -1}$| using |$50\, \rm {km \, s}^{ -1}$| binning with a |$\sim 2\, {\rm arcsec}$| synthesized beam. Neither dust continuum nor [C ii ] |$\, 158\, {\rm \mu m}$| line emission are detected at the expected frequency of ν[C ii ] |$= 163.791\, \rm {GHz}$| and the sky location of GN-z11. The upper limits show that GN-z11 is neither luminous in L IR nor L [C ii ], with a dust mass |$3\, \sigma$| limit of |${\rm log}\, (M_{\rm dust}/{\rm {\rm M}_{\odot }}) \, \lt\, 6.5-6.9$| and with a [C ii ] based molecular gas mass |$3\, \sigma$| limit of log (M mol, [C ii ] |$/{\rm {\rm M}_{\odot }}) \, \lt \, 9.3$|. Together with radiative transfer calculations, we also investigated the possible cause of the dust poor nature of the GN-z11 showed by the blue colour in the UV continuum of GN-z11 (βUV = −2.4), and found that ≳3 × deeper observations are crucial to study dust production at very high-redshift. Nevertheless, our observations show the crucial role of deep mm/submm observations of very high-redshift galaxies to constrain multiple phases in the interstellar medium. [ABSTRACT FROM AUTHOR]
- Published
- 2024
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