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

Tipo
Artigo
Data de publicação
2022
Periódico
Monthly Notices of the Royal Astronomical Society
Citações (Scopus)
19
Autores
Almeida-Fernandes F.
Sampedro L.
Herpich F.R.
Molino A.
Barbosa C.E.
Buzzo M.L.
Overzier R.A.
De Lima E.V.R.
Nakazono L.M.I.
Oliveira Schwarz G.B.
Perottoni H.D.
Bolutavicius G.F.
Gutierrez-Soto L.A.
Santos-Silva T.
Vitorelli A.Z.
Werle A.
Whitten D.D.
Costa Duarte M.V.
Bom C.R.
Coelho P.
Sodre L.
Placco V.M.
Teixeira G.S.M.
Alonso-Garcia J.
Barbosa C.L.
Beers T.C.
Bonatto C.J.
Chies-Santos A.L.
Hartmann E.A.
Lopes De Oliveira R.
Navarete F.
Kanaan A.
Ribeiro T.
Schoenell W.
Mendes De Oliveira C.
Orientador
Título da Revista
ISSN da Revista
Título de Volume
Membros da banca
Programa
Resumo
© 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.
Descrição
Palavras-chave
Assuntos Scopus
Astronomical data base: miscellaneous , Catalog , Data release , Galaxies general , Photometrics , Stars: general , Stellars , Techniques: photometric , Template fittings , Zero-point
Citação
DOI (Texto completo)