Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/341
Title: J-PLUS: photometric calibration of large-area multi-filter surveys with stellar and white dwarf loci
Authors: López Sanjuan, C.
Varela, J.
Cristóbal Hornillos, D.
Vazquez Ramió, H.
Carrasco, J. M.
Tremblay, P. E.
Whitten, D. D.
Placco, V. M.
Marín Franch, A.
Cenarro, A. J.
Ederoclite, A.
Alfaro, Emilio J.
Coelho, P. R. T.
Civera, T.
Hernández Fuertes, J.
Jiménez Esteban, F. M.
Jiménez Teja, Y.
Maíz Apellániz, J.
Sobral, D.
Vílchez, J. M.
Alcaniz, J. S.
Angulo, R. E.
Dupke, R. A.
Hernández Monteagudo, C.
Mendes de Oliveira, C. L.
Moles, M.
Sodré, L.
Keywords: Methods: statistical;Techniques: photometric
Issue Date: 5-Nov-2019
Publisher: EDP Sciences
DOI: 10.1051/0004-6361/201936405
Published version: https://www.aanda.org/articles/aa/abs/2019/11/aa36405-19/aa36405-19.html
Citation: Astronomy and Astrophysics 631: A119(2019)
Abstract: Aims. We present the photometric calibration of the 12 optical passbands observed by the Javalambre Photometric Local Universe Survey (J-PLUS). Methods. The proposed calibration method has four steps: (i) definition of a high-quality set of calibration stars using Gaia information and available 3D dust maps; (ii) anchoring of the J-PLUS gri passbands to the Pan-STARRS photometric solution, accounting for the variation in the calibration with the position of the sources on the CCD; (iii) homogenization of the photometry in the other nine J-PLUS filters using the dust de-reddened instrumental stellar locus in (𝒳 − r) versus (g − i) colours, where 𝒳 is the filter to calibrate. The zero point variation along the CCD in these filters was estimated with the distance to the stellar locus. Finally, (iv) the absolute colour calibration was obtained with the white dwarf locus. We performed a joint Bayesian modelling of 11 J-PLUS colour–colour diagrams using the theoretical white dwarf locus as reference. This provides the needed offsets to transform instrumental magnitudes to calibrated magnitudes outside the atmosphere. Results. The uncertainty of the J-PLUS photometric calibration, estimated from duplicated objects observed in adjacent pointings and accounting for the absolute colour and flux calibration errors, are ∼19 mmag in u, J0378, and J0395; ∼11 mmag in J0410 and J0430; and ∼8 mmag in g, J0515, r, J0660, i, J0861, and z. Conclusions. We present an optimized calibration method for the large-area multi-filter J-PLUS project, reaching 1–2% accuracy within an area of 1022 square degrees without the need for long observing calibration campaigns or constant atmospheric monitoring. The proposed method will be adapted for the photometric calibration of J-PAS, that will observe several thousand square degrees with 56 narrow optical filters.
URI: http://hdl.handle.net/20.500.12666/341
E-ISSN: 1432-0746
ISSN: 0004-6361
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