Data Release 2 of S-PLUS: Accurate template-fitting based photometry covering ∼1000 deg2in 12 optical filters

dc.contributor.authorAlmeida-Fernandes F.
dc.contributor.authorSampedro L.
dc.contributor.authorHerpich F.R.
dc.contributor.authorMolino A.
dc.contributor.authorBarbosa C.E.
dc.contributor.authorBuzzo M.L.
dc.contributor.authorOverzier R.A.
dc.contributor.authorDe Lima E.V.R.
dc.contributor.authorNakazono L.M.I.
dc.contributor.authorOliveira Schwarz G.B.
dc.contributor.authorPerottoni H.D.
dc.contributor.authorBolutavicius G.F.
dc.contributor.authorGutierrez-Soto L.A.
dc.contributor.authorSantos-Silva T.
dc.contributor.authorVitorelli A.Z.
dc.contributor.authorWerle A.
dc.contributor.authorWhitten D.D.
dc.contributor.authorCosta Duarte M.V.
dc.contributor.authorBom C.R.
dc.contributor.authorCoelho P.
dc.contributor.authorSodre L.
dc.contributor.authorPlacco V.M.
dc.contributor.authorTeixeira G.S.M.
dc.contributor.authorAlonso-Garcia J.
dc.contributor.authorBarbosa C.L.
dc.contributor.authorBeers T.C.
dc.contributor.authorBonatto C.J.
dc.contributor.authorChies-Santos A.L.
dc.contributor.authorHartmann E.A.
dc.contributor.authorLopes De Oliveira R.
dc.contributor.authorNavarete F.
dc.contributor.authorKanaan A.
dc.contributor.authorRibeiro T.
dc.contributor.authorSchoenell W.
dc.contributor.authorMendes De Oliveira C.
dc.date.accessioned2024-03-12T19:15:16Z
dc.date.available2024-03-12T19:15:16Z
dc.date.issued2022
dc.description.abstract© 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing survey of ∼9300 deg2 in the southern sky in a 12-band photometric system. This paper presents the second data release (DR2) of S-PLUS, consisting of 514 tiles covering an area of 950 deg2. The data has been fully calibrated using a new photometric calibration technique suitable for the new generation of wide-field multifilter surveys. This technique consists of a χ2 minimization to fit synthetic stellar templates to already calibrated data from other surveys, eliminating the need for standard stars and reducing the survey duration by ∼15 per cent. We compare the template-predicted and S-PLUS instrumental magnitudes to derive the photometric zero-points (ZPs). We show that these ZPs can be further refined by fitting the stellar templates to the 12 S-PLUS magnitudes, which better constrain the models by adding the narrow-band information. We use the STRIPE82 region to estimate ZP errors, which are 10 mmags for filters J0410, J0430, g, J0515, r, J0660, i, J0861 and z; 15 mmags for filter J0378; and 25 mmags for filters u and J0395. We describe the complete data flow of the S-PLUS/DR2 from observations to the final catalogues and present a brief characterization of the data. We show that, for a minimum signal-to-noise threshold of 5, the photometric depths of the DR2 range from 19.1 to 20.5 mag (measured in Petrosian apertures), depending on the filter. The S-PLUS DR2 can be accessed from the website: https://splus.cloud.
dc.description.firstpage4590
dc.description.issuenumber3
dc.description.lastpage4618
dc.description.volume511
dc.identifier.doi10.1093/mnras/stac284
dc.identifier.issn1365-2966
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/34378
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsAcesso Restrito
dc.subject.otherlanguageastronomical data bases: miscellaneous
dc.subject.otherlanguagecatalogues
dc.subject.otherlanguagegalaxies: general
dc.subject.otherlanguagestars: general
dc.subject.otherlanguagesurveys
dc.subject.otherlanguagetechniques: photometric
dc.titleData Release 2 of S-PLUS: Accurate template-fitting based photometry covering ∼1000 deg2in 12 optical filters
dc.typeArtigo
local.scopus.citations28
local.scopus.eid2-s2.0-85127448552
local.scopus.subjectAstronomical data base: miscellaneous
local.scopus.subjectCatalog
local.scopus.subjectData release
local.scopus.subjectGalaxies general
local.scopus.subjectPhotometrics
local.scopus.subjectStars: general
local.scopus.subjectStellars
local.scopus.subjectTechniques: photometric
local.scopus.subjectTemplate fittings
local.scopus.subjectZero-point
local.scopus.updated2024-12-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85127448552&origin=inward
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