Erratum: The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5

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dc.contributor.authorOld, Lyndsay J.en
dc.contributor.authorBalogh, Michael L.en
dc.contributor.authorvan der Burg, Remco F.J.en
dc.contributor.authorBiviano, Andreaen
dc.contributor.authorYee, Howard K.C.en
dc.contributor.authorPintos-Castro, Ireneen
dc.contributor.authorWebb, Kristien
dc.contributor.authorMuzzin, Adamen
dc.contributor.authorRudnick, Gregoryen
dc.contributor.authorVulcani, Benedettaen
dc.contributor.authorPoggianti, Biancaen
dc.contributor.authorCooper, Michaelen
dc.contributor.authorZaritsky, Dennisen
dc.contributor.authorCerulo, Pierluigien
dc.contributor.authorWilson, Gillianen
dc.contributor.authorChan, Jeffrey C.C.en
dc.contributor.authorLidman, Chrisen
dc.contributor.authorMcGee, Seanen
dc.contributor.authorDemarco, Ricardoen
dc.contributor.authorForrest, Benen
dc.contributor.authorde Lucia, Gabriellaen
dc.contributor.authorGilbank, Daviden
dc.contributor.authorKukstas, Egidijusen
dc.contributor.authorMcCarthy, Ian G.en
dc.contributor.authorJablonka, Pascaleen
dc.contributor.authorNantais, Julieen
dc.contributor.authorNoble, Allisonen
dc.contributor.authorReeves, Andrew M.M.en
dc.contributor.authorShipley, Heathen
dc.date.accessioned2025-06-11T13:34:59Z
dc.date.available2025-06-11T13:34:59Z
dc.date.issued2021-01-01en
dc.description.abstractThis is a correction to: Monthly Notices of the Royal Astronomical Society, Volume 493, Issue 4, April 2020, Pages 5987–6000, https://doi.org/10.1093/mnras/staa579 This is an erratum to the paper ‘The GOGREEN survey: the environmental dependence of the star-forming galaxymain sequence at 1.0 < z < 1.5’ that was published in MNRAS, 493, 5987– 6000 (2020). The [O II] fluxes and derived star-formation rates we derive from our spectra require an absolute flux calibration, which is obtained by comparing with the i-band photometry. In the data presented in the original publication, this calibration was applied incorrectly, as its inverse. The error has little effect on the mean properties of the sample, because the scaling factor is below unity for about half the sample, and above unity for the other half. However, it had the effect of greatly increasing the scatter in these derived quantities. This has a modest impact on our quantitative conclusions and interpretation.en
dc.description.statusPeer-revieweden
dc.format.extent3en
dc.identifier.issn0035-8711en
dc.identifier.scopus85097460804en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=85097460804&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733758662
dc.language.isoenen
dc.rightsPublisher Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.en
dc.sourceMonthly Notices of the Royal Astronomical Societyen
dc.subjectAddendaen
dc.subjectErrataen
dc.subjectgalaxies: clusters: generalen
dc.subjectgalaxies: evolutionen
dc.titleErratum: The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at 1.0 &lt; z &lt; 1.5en
dc.typeCommentaryen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage357en
local.bibliographicCitation.startpage355en
local.contributor.affiliationOld, Lyndsay J.; European Space Astronomy Centreen
local.contributor.affiliationBalogh, Michael L.; University of Waterlooen
local.contributor.affiliationvan der Burg, Remco F.J.; European Southern Observatoryen
local.contributor.affiliationBiviano, Andrea; Osservatorio Astronomico di Triesteen
local.contributor.affiliationYee, Howard K.C.; University of Torontoen
local.contributor.affiliationPintos-Castro, Irene; University of Torontoen
local.contributor.affiliationWebb, Kristi; University of Waterlooen
local.contributor.affiliationMuzzin, Adam; York University Torontoen
local.contributor.affiliationRudnick, Gregory; University of Kansasen
local.contributor.affiliationVulcani, Benedetta; Astronomical Observatory of Paduaen
local.contributor.affiliationPoggianti, Bianca; Astronomical Observatory of Paduaen
local.contributor.affiliationCooper, Michael; University of California at Irvineen
local.contributor.affiliationZaritsky, Dennis; University of Arizonaen
local.contributor.affiliationCerulo, Pierluigi; Universidad de Concepciónen
local.contributor.affiliationWilson, Gillian; University of California at Riversideen
local.contributor.affiliationChan, Jeffrey C.C.; University of California at Riversideen
local.contributor.affiliationLidman, Chris; Australian Astronomical Observatoryen
local.contributor.affiliationMcGee, Sean; University of Birminghamen
local.contributor.affiliationDemarco, Ricardo; Universidad de Concepciónen
local.contributor.affiliationForrest, Ben; University of California at Riversideen
local.contributor.affiliationde Lucia, Gabriella; Osservatorio Astronomico di Triesteen
local.contributor.affiliationGilbank, David; South African Astronomical Observatoryen
local.contributor.affiliationKukstas, Egidijus; Liverpool John Moores Universityen
local.contributor.affiliationMcCarthy, Ian G.; Liverpool John Moores Universityen
local.contributor.affiliationJablonka, Pascale; Swiss Federal Institute of Technology Lausanneen
local.contributor.affiliationNantais, Julie; Universidad Andrés Belloen
local.contributor.affiliationNoble, Allison; Arizona State Universityen
local.contributor.affiliationReeves, Andrew M.M.; University of Waterlooen
local.contributor.affiliationShipley, Heath; McGill Universityen
local.identifier.citationvolume500en
local.identifier.doi10.1093/mnras/staa2890en
local.identifier.pure14786e55-4933-4383-ad49-482be5bd5da1en
local.identifier.urlhttps://www.scopus.com/pages/publications/85097460804en
local.type.statusPublisheden

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