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Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6


The existence of massive (1011 solar masses) elliptical galaxies by redshift z ≈ 4 (refs 1, 2, 3; when the Universe was 1.5 billion years old) necessitates the presence of galaxies with star-formation rates exceeding 100 solar masses per year at z > 6 (corresponding to an age of the Universe of less than 1 billion years). Surveys have discovered hundreds of galaxies at these early cosmic epochs, but their star-formation rates are more than an order of magnitude lower4. The only known galaxies with very high star-formation rates at z > 6 are, with one exception5, the host galaxies of quasars6,7,8,9, but these galaxies also host accreting supermassive (more than 109 solar masses) black holes, which probably affect the properties of the galaxies. Here we report observations of an emission line of singly ionized carbon ([C ii] at a wavelength of 158 micrometres) in four galaxies at z > 6 that are companions of quasars, with velocity offsets of less than 600 kilometres per second and linear offsets of less than 100 kiloparsecs. The discovery of these four galaxies was serendipitous; they are close to their companion quasars and appear bright in the far-infrared. On the basis of the [C ii] measurements, we estimate star-formation rates in the companions of more than 100 solar masses per year. These sources are similar to the host galaxies of the quasars in [C ii] brightness, linewidth and implied dynamical mass, but do not show evidence for accreting supermassive black holes. Similar systems have previously been found at lower redshift10,11,12. We find such close companions in four out of the twenty-five z > 6 quasars surveyed, a fraction that needs to be accounted for in simulations13,14. If they are representative of the bright end of the [C ii] luminosity function, then they can account for the population of massive elliptical galaxies at z ≈ 4 in terms of the density of cosmic space.

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Figure 1: Images and spectra of the quasars and their companion galaxies discovered in this study.
Figure 2: Velocity structure in the system PJ308−21.
Figure 3: Intensely star-forming galaxies in the earliest galactic overdensities.


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We thank J. Hennawi, Y. Shen, A. Myers and L. Guzzo for comments on the QSO clustering. Support for R.D. was provided by the DFG priority programme 1573 “The physics of the interstellar medium.” F.W., B.V. and E.P.F. acknowledge support through ERC grant COSMIC-DAWN. R.W. acknowledges support from the National Science Foundation of China (NSFC; grant numbers 11473004 and 11533001) and the National Key Program for Science and Technology Research and Development (grant 2016YFA0400703). ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (South Korea), in cooperation with Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. E.B. is a Carnegie-Princeton Fellow.

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Authors and Affiliations



R.D. led the writing and analysis. F.W. was principle investigator of the ALMA programme that led to this discovery. F.W. and B.P.V. played a central part in the project design and implementation. E.P.F. provided the clustering analysis. E.B., B.P.V., E.P.F., C.M., F.W. and H.W.R. contributed to the identification of Pan-STARRS1 quasars. X.F. provided the Hubble observations of J0842+1218. All authors contributed to writing the proposal, and reviewed, discussed and commented on the manuscript.

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Correspondence to R. Decarli.

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The authors declare no competing financial interests.

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Reviewer Information Nature thanks D. Frayer and the other anonymous reviewer(s) for their contribution to the peer review of this work.

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Decarli, R., Walter, F., Venemans, B. et al. Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6. Nature 545, 457–461 (2017).

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