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Studying the ISM at ∼10 pc scale in NGC 7793 with MUSEII : Constraints on the oxygen abundance and ionising radiation escape (Corrigendum)

Della Bruna, Lorenza (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Adamo, Angela, 1981- (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Lee, Janice C. (author)
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Smith, Linda J. (author)
Krumholz, Mark (author)
Bik, Arjan (author)
Calzetti, Daniela (author)
Fox, Anne (author)
Fumagalli, Michele (author)
Grasha, Kathryne (author)
Messa, Matteo, 1988- (author)
Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Université de Genève, Switzerland
Östlin, Göran (author)
Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Walterbos, Rene (author)
Wofford, Aida (author)
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 (creator_code:org_t)
2022-07-04
2022
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 663
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Table 3 in the original paper reports inaccurate values of Q0exp;YSC and Q0obs(and hence of the related quantities Qexp;tot, Qexptot=Qobs, and fesc). The error in Q0exp;YSC results from a mistake in the sampling of the cluster probability distribution functions (PDFs), whereas Q0obswas mistakenly computed from non-dereddened values of L(Hα). In Table 1 we provide a revised version of the original Table 3, and in Figs. 1 and 2 we show revised versions of the original Figs. 10 and 11. The revised values do not change any of the conclusions stated in the original paper. In the following we provide revised text for the affected sections. (Figure Presented). 

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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