diff --git a/docs/source/cpic/data_model.md b/docs/source/cpic/data_model.md index 1aafe577b90bb4cf1483fc5119d1b5aeba6ae5af..ce54a868efd5af4d772cab61848b74ebdcb6ca34 100644 --- a/docs/source/cpic/data_model.md +++ b/docs/source/cpic/data_model.md @@ -1,5 +1,7 @@ # L1-CPI-C Data model +- `---`表示在模块算法失败的情况下按照实际情况填写,比如无论模块是否成功,时间戳都应该填写实际值 + ## File: *_VIS_SCI_*.*fits ### File contents @@ -8,7 +10,7 @@ |------|-------------------------|------------| | HDU0 | None | PrimaryHDU | | HDU1 | reduced image (1k x 1k) | ImageHDU | -| HDU2 | mask image (9k x 9k) | ImageHDU | +| HDU2 | mask image (1k x 1k) | ImageHDU | ### HDU0 @@ -18,8 +20,6 @@ ### HDU1 -#### Header of `csst_ms_mbi_instrument` - | keyword | value | comment | fill value | type | module | |-----------|:----------------------|-------------------------------------------------|--------------|------|--------------------------| | VER_PIPE | '0.01' | version of CPI-C pipeline | '0.01' | str | csst_cpic | @@ -53,3 +53,14 @@ | CR_MOD | 'lacosmic' | mode of CR clean. 'lacosmic' or 'deepCR' | -1 | str | csst_cpic | | CR_NUM | 10 | number of cosmic ray | -1 | i16 | csst_cpic | +### HDU2 + +| keyword | value | comment | fill value | type | module | +|-----------|:----------------------|-------------------------------------------------|--------------|------|--------------------------| +| FLAG | 0 | normal pixels | 0 | i8 | csst_cpic | +| FLAG | 1 | bad pixels | 0 | i8 | csst_cpic | +| FLAG | 2 | hot pixels | 0 | i8 | csst_cpic | +| FLAG | 4 | warm pixels | 0 | i8 | csst_cpic | +| FLAG | 8 | saturated pixels | 0 | i8 | csst_cpic | +| FLAG | 16 | pixels contaminated by cosmic ray | 0 | i8 | csst_cpic | +| FLAG | 32 | pixels contaminated by sputnik | 0 | i8 | csst_cpic | \ No newline at end of file