![Compact [C ii] emitters around a C iv absorption complex at redshift 5.7 – Nature](https://media.springernature.com/m685/springer-static/image/art:10.1038/s41586-023-05901-3/MediaObjects/41586_2023_5901_Fig1_HTML.png)
Simcoe, R. A., Sargent, W. L. W., Rauch, M. & Becker, G. Observations of chemically enriched QSO absorbers near z~2.3 galaxies: galaxy formation feedback signatures in the intergalactic medium. Astrophys. J. 637, 648–668 (2006).
Prochaska, J. X. et al. The UCSD/Keck damped Lyα abundance database: a decade of high-resolution spectroscopy. Astrophys. J. Suppl. Ser. 171, 29–60 (2007).
Fox, A. J., Ledoux, C., Petitjean, P. & Srianand, R. C IV absorption in damped and sub-damped Lyman-α systems. Correlations with metallicity and implications for galactic winds at z ≈ 2–3. Astron. Astrophys. 473, 791–803 (2007).
Bordoloi, R. et al. Resolving the H I in damped Lyman α systems that power star formation. Nature 606, 59–63 (2022).
Díaz, C. G. et al. Faint LAEs near z > 4.7 C IV absorbers revealed by MUSE. Mon. Not. R. Astron. Soc. 502, 2645–2663 (2021).
Wu, Y. et al. A [C II] 158 μm emitter associated with an O I absorber at the end of the reionization epoch. Nat. Astron. 5, 1110–1117 (2021).
Becker, G. D., Sargent, W. L. W., Rauch, M. & Simcoe, R. A. Discovery of excess O I absorption toward the z = 6.42 QSO SDSS J1148+5251. Astrophys. J. 640, 69–80 (2006).
Simcoe, R. A. et al. Constraints on the universal C IV mass density at z ~ 6 from early infrared spectra obtained with the Magellan FIRE spectrograph. Astrophys. J. 743, 21 (2011).
Chen, S.-F. S. et al. Mg II absorption at 2 < z < 7 with Magellan/Fire. III. Full statistics of absorption toward 100 high-redshift QSOs. Astrophys. J. 850, 188 (2017).
Codoreanu, A. et al. The CGM and IGM at z ~ 5: metal budget and physical connection. Mon. Not. R. Astron. Soc. 481, 4940–4959 (2018).
Cooper, T. J. et al. Heavy element absorption systems at 5.0 < z < 6.8: metal-poor neutral gas and a diminishing signature of highly ionized circumgalactic matter. Astrophys. J. 882, 77 (2019).
Becker, G. D. et al. The evolution of O I over 3.2 < z < 6.5: reionization of the circumgalactic medium. Astrophys. J. 883, 163 (2019).
Vallini, L., Gallerani, S., Ferrara, A. & Baek, S. Far-infrared line emission from high-redshift galaxies. Mon. Not. R. Astron. Soc. 433, 1567–1572 (2013).
Vallini, L., Gallerani, S., Ferrara, A., Pallottini, A. & Yue, B. On the [CII]-SFR relation in high redshift galaxies. Astrophys. J. 813, 36 (2015).
Dutta, R. et al. Metal-enriched halo gas across galaxy overdensities over the last 10 billion years. Mon. Not. R. Astron. Soc. 508, 4573–4599 (2021).
Toshikawa, J. et al. Discovery of protoclusters at z ~ 3.7 and 4.9: embedded in primordial superclusters. Astrophys. J. 888, 89 (2020).
Venemans, B. P. et al. Kiloparsec-scale ALMA imaging of [C II] and dust continuum emission of 27 quasar host galaxies at z ~ 6. Astrophys. J. 904, 130 (2020).
Zana, T. et al. Enhanced star formation in z ~ 6 quasar companions. Mon. Not. R. Astron. Soc. 513, 2118–2135 (2022).
Aravena, M. et al. The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: search for [C II] line and dust emission in 6 < z < 8 galaxies. Astrophys. J. 833, 71 (2016).
Neeleman, M. et al. [C II] 158-μm emission from the host galaxies of damped Lyman-alpha systems. Science 355, 1285–1288 (2017).
Fujimoto, S. et al. The ALPINE–ALMA [C II] survey: size of individual star-forming galaxies at z = 4–6 and their extended halo structure. Astrophys. J. 900, 1 (2020).
Fudamoto, Y. et al. The ALMA REBELS survey: average [C II] 158 μm sizes of star-forming galaxies from z ~ 7 to z ~ 4. Astrophys. J. 934, 144 (2022).
Olsen, K. P. et al. Simulator of Galaxy Millimeter/Submillimeter Emission (SíGAME): The [C II]-SFR relationship of massive z = 2 main sequence galaxies. Astrophys. J. 814, 76 (2015).
De Looze, I. et al. The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. Astron. Astrophys. 568, A62 (2014).
Schaerer, D. et al. The ALPINE-ALMA [C II] survey. Little to no evolution in the [C II]-SFR relation over the last 13 Gyr. Astron. Astrophys. 643, A3 (2020).
Carniani, S. et al. Kiloparsec-scale gaseous clumps and star formation at z = 5–7. Mon. Not. R. Astron. Soc. 478, 1170–1184 (2018).
Le Fèvre, O. et al. The ALPINE-ALMA [CII] survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6. Astron. Astrophys. 643, A1 (2020).
Fudamoto, Y. et al. The ALPINE-ALMA [CII] survey. Dust attenuation properties and obscured star formation at z ~ 4.4–5.8. Astron. Astrophys. 643, A4 (2020).
Pentericci, L. et al. Tracing the reionization epoch with ALMA: [C II] emission in z ~ 7 galaxies. Astrophys. J. Lett. 829, L11 (2016).
Bradač, M. et al. ALMA [C II] 158 μm detection of a redshift 7 lensed galaxy behind RX J1347.1–1145. Astrophys. J. Lett. 836, L2 (2017).
Behrens, C., Pallottini, A., Ferrara, A., Gallerani, S. & Vallini, L. Dusty galaxies in the Epoch of Reionization: simulations. Mon. Not. R. Astron. Soc. 477, 552–565 (2018).
Planck Collaboration et al. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 641, A6 (2020).
Alam, S. et al. The eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-III. Astrophys. J. Supp. 219, 12 (2015).
McMullin, J. P., Waters, B., Schiebel, D., Young, W. & Golap, K. in Astronomical Data Analysis Software and Systems XVI ASP Conference Series Vol. 376 (eds Shaw, R. A., Hill, F. & Bell, D. J.) 127 (Astronomical Society of the Pacific, 2007).
Walter, F. et al. ALMA spectroscopic survey in the Hubble Ultra Deep Field: survey description. Astrophys. J. 833, 67 (2016).
Boogaard, L., Meyer, R. A. & Novak, M. Interferopy: analysing datacubes from radio-to-submm observations. Zenodo https://zenodo.org/record/5775604 (2021).
Popping, G. et al. Sub-mm emission line deep fields: CO and [C II] luminosity functions out to z = 6. Mon. Not. R. Astron. Soc. 461, 93–110 (2016).
Ferrara, A. et al. The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at z ≈ 7. Mon. Not. R. Astron. Soc. 512, 58–72 (2022).
Béthermin, M. et al. The ALPINE-ALMA [CII] survey: data processing, catalogs, and statistical source properties. Astron. Astrophys. 643, A2 (2020).
Madau, P. & Dickinson, M. Cosmic star-formation history. Annu. Rev. Astron. Astrophys. 52, 415–486 (2014).
Chabrier, G. Galactic stellar and substellar initial mass function. Publ. Astron. Soc. Pac. 115, 763–795 (2003).
Vernet, J. et al. X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope. Astron. Astrophys. 536, A105 (2011).
Simcoe, R. A. et al. FIRE: a facility class near-infrared echelle spectrometer for the Magellan telescopes. Publ. Astron. Soc. Pac. 125, 270 (2013).
Prochaska, J. et al. PypeIt: the Python spectroscopic data reduction pipeline. J. Open Source Softw. 5, 2308 (2020).
Gagné, J., Lambrides, E., Faherty, J. K. & Simcoe, R. FireHose_v2: Firehose v2.0. Zenodo https://zenodo.org/record/18775 (2015).
Vacca, W. D., Cushing, M. C. & Rayner, J. T. A method of correcting near-infrared spectra for telluric absorption. Publ. Astron. Soc. Pac. 115, 389–409 (2003).
Cushing, M. C., Vacca, W. D. & Rayner, J. T. Spextool: a spectral extraction package for SpeX, a 0.8–5.5 micron cross-dispersed spectrograph. Publ. Astron. Soc. Pac. 116, 362–376 (2004).
Foreman-Mackey, D., Hogg, D. W., Lang, D. & Goodman, J. emcee: the MCMC hammer. Publ. Astron. Soc. Pac. 125, 306–312 (2013).
Hoffmann, S. L. et al. The DrizzlePac Handbook, Version 2.0. Space Telescope Science Institute https://hst-docs.stsci.edu/drizzpac (2021).
Weilbacher, P. M. et al. The data processing pipeline for the MUSE instrument. Astron. Astrophys. 641, A28 (2020).
Borisova, E. et al. Ubiquitous giant Lyα nebulae around the brightest quasars at z ~ 3.5 revealed with MUSE. Astrophys. J. 831, 39 (2016).
Cantalupo, S. et al. The large- and small-scale properties of the intergalactic gas in the Slug Ly α nebula revealed by MUSE He II emission observations. Mon. Not. R. Astron. Soc. 483, 5188–5204 (2019).
Bacon, R. et al. The MUSE 3D view of the Hubble Deep Field South. Astron. Astrophys. 575, A75 (2015).
More News
Author Correction: Stepwise activation of a metabotropic glutamate receptor – Nature
Changing rainforest to plantations shifts tropical food webs
Streamlined skull helps foxes take a nosedive