Details
-
Type:
Story
-
Status: Done
-
Resolution: Done
-
Fix Version/s: None
-
Component/s: pipe_drivers
-
Labels:None
-
Story Points:4
-
Epic Link:
-
Sprint:Arch 2019-02-11, Arch 2019-02-18, Arch 2019-02-25, Arch 2019-03-04, Arch 2019-03-11, Arch 2019-03-18
-
Team:Architecture
Description
I was testing the new metadata translator on FITS file I had lying around in testdata repositories and I see that our calibration products do not seem to have a reasonable set of headers. The only indication this is a HSC calibration file rather than an LSST one is the path name to the root directory.
SIMPLE = T / file does conform to FITS standard
|
BITPIX = -32 / number of bits per data pixel
|
NAXIS = 2 / number of data axes
|
NAXIS1 = 2048 / length of data axis 1
|
NAXIS2 = 4176 / length of data axis 2
|
EXTEND = T / FITS dataset may contain extensions
|
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
|
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
|
OBSTYPE = 'bias '
|
HIERARCH CALIB_CREATION_DATE = '2016-03-28'
|
HIERARCH CALIB_CREATION_TIME = '16:16:33 EDT'
|
HIERARCH CALIB_CREATION_ROOT = '/tigress/HSC/HSC/rerun/dm-5124/calib'
|
HIERARCH CALIB_INPUT_0 = '(904542,)'
|
HIERARCH CALIB_INPUT_1 = '(904544,)'
|
HIERARCH CALIB_INPUT_2 = '(904546,)'
|
HIERARCH CALIB_INPUT_3 = '(904548,)'
|
HIERARCH CALIB_INPUT_4 = '(904550,)'
|
HIERARCH CALIB_INPUT_5 = '(904552,)'
|
HIERARCH CALIB_INPUT_6 = '(904554,)'
|
HIERARCH CALIB_INPUT_7 = '(904556,)'
|
HIERARCH CALIB_INPUT_8 = '(904558,)'
|
HIERARCH CALIB_INPUT_9 = '(904560,)'
|
HIERARCH CALIB_INPUT_10 = '(904562,)'
|
HIERARCH CALIB_INPUT_11 = '(904564,)'
|
HIERARCH CALIB_INPUT_12 = '(904566,)'
|
CALIB_ID= 'filter=NONE calibDate=2013-11-03 ccd=50'
|
HIERARCH MD5_IMAGE = '6185bb72f20de7e81c45e6e6591eb6ad'
|
CRVAL1A = 0 / Column pixel of Reference Pixel
|
CRVAL2A = 0 / Row pixel of Reference Pixel
|
CRPIX1A = 1 / Column Pixel Coordinate of Reference
|
CRPIX2A = 1 / Row Pixel Coordinate of Reference
|
CTYPE1A = 'LINEAR ' / Type of projection
|
CTYPE2A = 'LINEAR ' / Type of projection
|
CUNIT1A = 'PIXEL ' / Column unit
|
CUNIT2A = 'PIXEL ' / Row unit
|
At minimum there should be INSTRUME/TELESCOP headers but ideally we should be able to construct a full header based on all the input headers (propagating headers that are identical and indicating which headers define bounds). The latter is what I implemented at the JCMT Science Archive for all data products. It might be that another approach is to at least be able to generate a standard set of headers from the information the Butler (Gen 3) knows about each dataset.
pipe_drivers changes look good. Please be sure to test them, as they do not currently get exercised by unit tests, the demo or ci_hsc. I think ci_ctio0m9 might do.