Start Date | Context | Status | Description |
---|---|---|---|
2025-05-09 | hst_1237.pmap | latest | New STIS NUVMAMA and FUVMAMA throughputs are being delivered for ETC version 33.2. Throughputs are updated due to changes in the TDSTABs. There are no changes to the CCD throughputs. |
2025-05-07 | hst_1236.pmap | archived | These WFC3 UVIS superbias and postflash files will affect all full-frame and subarray 1x1 binned UVIS data. The 2023 superbiases will affect data taken from January 1 - December 31 2023. The 2024 superbiases will affect all data taken after January 1, 2024. Currently, the automated calibration pipeline and Calibration Reference Data System only have WFC3 UVIS full-frame and subarray bias reference files up to a USEAFTER date of January 1, 2022. The automated pipeline should now use these reference files to perform bias subtraction on any 1x1 binned UVIS datasets obtained between the dates above because they represent the most accurate estimate of the residual bias level at the time of the science observation. The 2023 WFC3 UVIS superbias files were generated using bias exposures from the HST Cycle 30 and 31 monitoring programs 16967 and 17345. The 2024 WFC3 UVIS superbias files were generated using bias exposures from the HST Cycle 31 and 32 monitoring programs 17345 and 17665. More information regarding the method used to create UVIS bias calibration reference files can be found in WFC3 ISR 2023 03. Additionally, the header of each reference file has a history section listing the datasets used to create each file. This update also includes redelivery of two 2023 postflash files, which had been corrupted during a safing event, and the first-time delivery of four 2024 postflash files created from calibration data. Yearly postflash files for use in the pipeline to correct for postflashing of UVIS data was first begun in 2022. |
2025-05-02 | hst_1234.pmap | archived | A new ACS SBC IMPHTTAB is being delivered with updated data after newly acquired observations were taken on 25 Mar 2025 as part of CAL/ACS program 17658. |
2025-05-01 | hst_1233.pmap | archived | Updated STIS PHOTTABs to recalibrate M-mode sensitivities using the CALSPECv11 models. These files include recalibrations to the sensitivities of all primary cenwaves of G140M, G230M, G230MB, G430M, and G750M, as well as G230MB secondary cenwave 2794, G430M secondary cenwaves 3305, 3843, 5093, and G750M secondary cenwaves 6094, 6581, 9286. |