Correction to: Characterising the contribution of dust-obscured star formation at <i>z</i> ≳ 5 using 18 serendipitously identified [C<scp> ii</scp>] emitters

given as follows: 'Characterising the contribution of dust-obscured star formation at 5 using 18 serendipitously identified [C II ] emitters'.

Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-11-26
DOI
https://doi.org/10.1093/mnras/stae2624
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00
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article

Correction to: Characterising the contribution of dust-obscured star formation at z ≳ 5 using 18 serendipitously identified [C ii] emitters

Monthly Notices of the Royal Astronomical Society
Astro and Planetary Science
article

Correction to: Characterising the contribution of dust-obscured star formation at z ≳ 5 using 18 serendipitously identified [C ii] emitters

article en

Abstract

given as follows: 'Characterising the contribution of dust-obscured star formation at 5 using 18 serendipitously identified [C II ] emitters'.

Monthly Notices of the Royal Astronomical SocietyVol. 535(4)
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Correction to: Characterising the contribution of dust-obscured star formation at <i>z</i> ≳ 5 using 18 serendipitously identified [C<scp> ii</scp>] emitters · Monthly Notices of the Royal Astronomical Society (2024) | TGRS Research Map | TGRS