Precision of the J-PLUS photometric calibration from giant branch stars.
|Passband||σSLR||σISL||σISL + P|
|[mmag] (a)||[mmag] (b)||[mmag] (c)|
Stellar locus regression (SLR) was used as calibration method. Uncertainty from duplicated GB stars in overlapping pointings.
Instrumental stellar locus (ISL) or PS1 was used to homogenize the photometry. Uncertainty from duplicated GB stars in overlapping pointings.
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