ACS Data Handbook v. 9.0
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ACS Data Handbook > Chapter 3: ACS Calibration Pipeline > 3.1 Mikulski Archive for Space Telescopes (MAST)

3.1
ACS data requests are processed with the Mikulski Archive for Space Telescopes (MAST) pipeline. It provides users with calibrated data that is created using the best available reference files and latest software upgrades.
STScI's calibration pipeline consists of two main software systems: the "Data Management System" (DMS) and the "Data Archive and Distribution System" (DADS).
Raw spacecraft telemetry data from the Goddard Space Flight Center are transmitted to STScI in the form of POD files which are stored in the HST Archive. MAST processing begins with the POD files when DMS runs a step called Generic Conversion to extract and create uncalibrated "raw" data. During this step, the "Calibration Reference Database System" (CRDS), where all calibration reference files are stored, is queried to determine the most current reference files for the observation's configuration and date. DMS then calibrates the raw data using calacs, with the best-available reference images and tables from the CRDS. These calibrated data, along with other requested data products, are sent to the user. (See Chapter 1 of the Introduction to the HST Data Handbooks for more information about retrieving data from the Archive.)
CCD dark, bias, and sink pixel reference files are frequently delivered to CRDS, or occasionally updated. Users who receive their data shortly after an observation was executed are advised to wait a few more weeks for the best-suited reference files (usually the darks) to become available in CRDS. At that point, the data could be re-retrieved from the Archive or manually recalibrated using the new reference files. To find out if reference files have been updated, compare the names of the reference files in the image header with those listed as the recommended reference files for a particular dataset in MAST HST Data Search. For dated ACS products, it is often more convenient to retrieve freshly-calibrated data from the Archive before beginning data analysis. Users who choose to rerun calacs on raw data should consult the ACS Reference Files web page and retrieve reference files from the CRDS web page (See Section 3.5 for information about running calacs).

ACS Data Handbook > Chapter 3: ACS Calibration Pipeline > 3.1 Mikulski Archive for Space Telescopes (MAST)

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