Overview of PFS Data Products
This section describes the main PFS data products produced by the 2D DRP pipeline. They are all stored as FITS files and follow a strict naming convention based on observation identifiers.
We will show how PFS data products are stored, can be accessed and analyzed using Butler. Data on the PFS Science Platform will be used as reference, specifically data products from proposal ID S25A-000QF, which is part of the Observatory Filler Program and available to everyone who signs up to the Science Platform. The method of accessing and analyzing PFS data products using Butler is universally applicable to all 2D DRP pipeline reduced data.
As a reference, the following are all the pipeline data products:
apCorr cosmicray_config fitFluxCal_log fluxCal lam1d_modified_updated packages pfsCoadd pfsMergedLsf
calibs cosmicray_log fitFluxCal_metadata isr_config mergeArms_config pfsArm pfsCoaddLsf reduceExposure_config
coaddSpectra_config cosmicray_metadata fitFluxReference_config isr_log mergeArms_log pfsArmLsf pfsConfig reduceExposure_log
coaddSpectra_log detectorMap fitFluxReference_log isr_metadata mergeArms_metadata pfsCalibrated pfsFluxReference reduceExposure_metadata
coaddSpectra_metadata fitFluxCal_config fitFluxReference_metadata lam1d_modified objectGroupMap pfsCalibratedLsf pfsMerged sky1d
Most of these files are not of much significance to the user as they are intermediate pipeline and QA products. The relevant PFS data products and their properties for the science user will be highlighted going forward, but for a detailed description please refer to the PFS Data Model documentation.
In this section we will provide explanations and code for quick analysis of PFS data products out of the box, but the user is also encouraged to follow the PFS Science Platform Getting-Started Notebook — a Jupyter Notebook that provides a step-by-step guide and a granular understanding of each data product.