Open stscijgbot opened 5 years ago
Comment by David Law: Have now been able to look at some data from program 850 as well; even for cases where MRS is the only instrument taking data (no simultaneous imaging, no FGS) the APERNAME (and associated V2REF, V3REF keywords) are still incorrectly set to MIRIM_FULL. From the files that I looked at, it also seemed like the crossed-dichroic information was not set properly in the headers for this program.
Another comment: It would be super-helpful to be able to see the BAND keyword as a column in the MAST interface! I don't see a way to enable this?
Comment by Rosa Diaz: I assume you already know this. PID 825 Obs 13 is a coordinate parallel with FGS
Comment by David Law: Right; FGS should be taking parallel data, but the science target should always be in the MRS for all 4 dither positions.
Comment by David Law: Adding other comments from my original email here just for completeness:
Comment by Misty Cracraft: Who should be looking into these issues? Alberto just brought up the same header issue of channel being defined as a NIRCam keyword in GSEG3 files. Should we assign this to a specific person since it looks like it hasn't been addressed since it was filed in May?
Issue JP-736 was created by David Law:
Mock data produced for the MIRI MRS in SIR2 and retrieved from MAST exhibits a number of problems with the FITS headers in the uncalibrated frames.
For program 825, observation 13 should have been a 4-point dithered MRS observation using the Channel 2 - optimized point source dither pattern. I downloaded the uncal.fits data for exposures 2-4; the first-extension header of exposures 2+3 use V2REF, V3REF keyword values appropriate for the MIRI imager, not the MRS. The values for exposure 4 look like they correspond to a location in the FGS, not the MRS. This matches with the APERNAME and PPS_APER values in the primary header, which are MIRIM_FULL and FGS2_FULL; both are incorrect, they should be MIRIFU_CHANNEL2A. V2REF, V3REF keywords for the MRS should always be tied to MIRIFU_CHANNEL1A for all MRS exposures, regardless of the actual aperture in use.
Similarly, the target observed was meant to be at (RA,DEC)=(80.47, -69.51), which agrees with the TARG_RA and TARG_DEC keywords from the exposures 2+3 primary headers (but not exp 4). If the RA_REF, DEC_REF keywords in the first extension header are to be believed though then the MIRI Imager is pointing at (RA,DEC)=(79.60, -68.91) and therefore the science target is about 2400 arcsec away; far outside the FOV of any of the JWST instruments...