Start Date | Context | Status | Description |
---|---|---|---|
2025-03-18 | hst_1221.pmap | latest | The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on March 11, 2025, and should be used to calibrate ACS WFC observations taken between February 11, 2024 and March 11, 2025. |
2025-03-10 | hst_1220.pmap | archived | This SPOTTAB update includes new hot spot occurrences that have appeared since September 2022. The positions and locations of the hot spots were determined using an automated code that examines summed, weekly dark exposures in each segment. The COS team confirmed that all of the hot spots are real and also that none of the previous manually flagged spots are omitted. For cases where a hot spot is known to be active during a science exposure only, their positions and time frames were input manually. This SPOTTAB delivery is more comprehensive than those in the past. |
2025-03-10 | hst_1219.pmap | archived | These time-dependent WFC3 IR superdark reference files will affect certain IR data taken from HST Cycle 26, beginning on November 5, 2018, to the present. They will replace reference files that contain a small number of pixels that had values of NaN due to an edge case in which all input pixels were rejected for persistence or as bad pixels. A description of the process used to create these files is recorded in the history sections of their headers, as is a list of the individual dark images used to create each file. Additional information on the superdark creation process can be found in WFC3 ISRs by Sunnquist et al., 2019, and Pidgeon and Khandrika, 2024. |
2025-03-06 | hst_1218.pmap | archived | Delivering updated ACS WFC CTE-corrected darks, DKCs, that incorporate the new pixel-based serial CTE correction. This serial CTE correction was implemented in the latest version of CALACS, v10.4.0, in December 2024. In the standard calibration pipeline, the new serial, X-direction, CTE correction and the parallel, Y-direction, correction are both run by default on all full-frame WFC exposures obtained post-SM4, i.e., after May 2009. These new post-SM4, CTE-corrected darks utilize both the serial and parallel corrections for optimal calibration. |