| Start Date | Context | Status | Description |
|---|---|---|---|
| 2026-07-16 | hst_1345.pmap | latest | Update to COS FUV TDSTAB and FLUXTAB reference files for all modes, obtained using python analysis scripts cos_tds_analysis.py, make_tds_reference.py. No new breakpoint introduced, instead the TDS corrections were updated up to Jan 2026 data. The file was tested by comparing all TDS observations to a reference model. The TDSTAB file needs to be used with the new FLUXTABs for LP1, LP2, LP3, LP4, LP5, LP6, LP7, and LP10 which have sensitivities backed out using the updated TDS parameters, and which were delivered on the same date. These reference files have a USEAFTER date of 2009 May 11. |
| 2026-07-13 | hst_1344.pmap | archived | Delivery of new STIS CCD bias and dark reference files for CCD data taken between June 11 2026 through July 09 2026. The files were generated from data taken in the same time frame under STIS calibration programs 18158, and 18155. |
| 2026-07-06 | hst_1343.pmap | archived | The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on June 30, 2026, and should be used to calibrate ACS WFC observations taken between June 5, 2026 and June 30, 2026. |
| 2026-06-29 | hst_1342.pmap | archived | New hot spots have appeared on both COS FUV segments since the last update. This new SPOTTAB corrects science and calibration data affected by these new hot spots. |