SIMBAD references

2022MNRAS.511.4590A - Mon. Not. R. Astron. Soc., 511, 4590-4618 (2022/April-2)

Data Release 2 of S-PLUS: Accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters.

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. and MENDES DE OLIVEIRA C.

Abstract (from CDS):

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.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): techniques: photometric - astronomical data bases: miscellaneous - catalogues - surveys - stars: general - galaxies: general

Simbad objects: 4

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