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  • gtobssim:
    • The event type partition has been added as an option for gtobssim.  Examples for P8R2_SOURCE_V6:

      Code Block
      gtobssim irfs=P8R2_SOURCE_V6 evtype=none
      gtobssim irfs=P8R2_SOURCE_V6 evtype=PSF
      gtobssim irfs=P8R2_SOURCE_V6 evtype=EDISP

      evtype=none is the default, in which case the application will use the front/back partition, consistent with pre-Pass 8 behavior.

    • For evtype=[PSF,EDISP], DSS keywords specifying the event_type partition that was used will be written to the FT1 files that are produced.  These keywords will show the bit pattern that would be used to mask to obtain the corresponding partition, e.g., for evtype=PSF:

      Code Block
      DSTYP2: BIT_MASK(EVENT_CLASS,128,P8R2)
      DSUNI2: DIMENSIONLESS
      DSVAL2: 1:1
      
      DSTYP3: BIT_MASK(EVENT_TYPE,60,P8R2)
      DSUNI3: DIMENSIONLESS
      DSVAL3: 1:1

      Here 60 = 0b111100, the binary representation of the mask with bits 2-5 set.  Note that the event_type DSS keywords will be omitted for the front/back partition.

    • Since there is no information in the IRFs on cross-membership between event_type partitions, only bits for the selected partition will be set in the FT1 file.  This means that choosing event_types in gtselect for a different partition will result in no events passing the cut.
  • gtselect
    • The evtype option has been added, and DSS keywords indicating this selection will be written.
    • For both evclass and evtype, the user must specify the integer corresponding to bit-mask that selects the desired events within a single partition:

      Code Block
      gtselect evclass=128 evtype=3     # P8R2_SOURCE_V6, front and back (i.e., all) events
      gtselect evclass=128 evtype=1     # P8R2_SOURCE_V6, front-only events
      gtselect evclass=128 evtype=60    # P8R2_SOURCE_V6, PSF[0-3] (all) events
      gtselect evclass=256 evtype=960   # P8R2_CLEAN_V6, EDISP[0-3] (all) events

      The evtype=[3,60,960] selections all return all of the events, but they also specify the irfs corresponding to the event_type partition selected.  This information is written to the DSS keywords and read by downstream tools.

    • One can also do

      Code Block
      gtselect evclass=none evtype=none

      in which case, no event_class or event_type cuts are applied and the DSS keywords associated with those cuts would not be added.  This will allow one to use an FT1 file from the astroserver as the common input file for different evclass and evtype selections.

    • evtype selections that cross partitions can be specified, but the behavior of the downstream tools (i.e., which irfs are used) is undefined.  At some point, we will add code to guard against invalid selections.
  • gtdiffrsp
    • evtype has been added as a hidden parameter.
    • If DSS keywords are in the input FT1 file (e.g., from gtselect or gtobssim), then gtdiffrsp will read those keywords to determine which event_type partition to use for computing the diffuse responses.   If no DSS keywords are present, then the evtype option will used to determine the partition.  If it is omitted, then front/back will be used. 
    • The value of evtype must be the integer representation of the full bit-mask corresponding to the desired partition, i.e., evtype=[3,60,960] for F/B, PSF, and EDISP, respectively.
    • The DSS keywords will be updated with the evtype selection and this will indicate the event_type partition used in computing the diffuse response columns.
  • gtexpcube2
    • If the cmap argument is missing, the DSS keywords from that input file will provide the information to determine the event_class and event_type selections.
    • The user can override the geometry of the cmap file.  This will allow exposure maps larger than the cmap to be specified.  The energy planes will be read from the cmap file, so these would no longer need to be specified by hand, but they could still be over-ridden.
  • gtirfs
    • The output will be expanded to indicate event_type partitions:

      Code Block
      $ gtirfs
      
      <...output for P7* irfs...>
      
      P8R2_CLEAN_V6 ( = P8R2_CLEAN_V6::BACK + P8R2_CLEAN_V6::FRONT )
      P8R2_CLEAN_V6 (EDISP) ( = P8R2_CLEAN_V6::EDISP0 + P8R2_CLEAN_V6::EDISP1 + P8R2_CLEAN_V6::EDISP2 + P8R2_CLEAN_V6::EDISP3 )
      P8R2_CLEAN_V6 (PSF) ( = P8R2_CLEAN_V6::PSF0 + P8R2_CLEAN_V6::PSF1 + P8R2_CLEAN_V6::PSF2 + P8R2_CLEAN_V6::PSF3 )
      P8R2_CLEAN_V6::BACK
      P8R2_CLEAN_V6::EDISP0
      P8R2_CLEAN_V6::EDISP1
      P8R2_CLEAN_V6::EDISP2
      P8R2_CLEAN_V6::EDISP3
      P8R2_CLEAN_V6::FRONT
      P8R2_CLEAN_V6::PSF0
      P8R2_CLEAN_V6::PSF1
      P8R2_CLEAN_V6::PSF2
      P8R2_CLEAN_V6::PSF3
      P8R2_SOURCE_V6 ( = P8R2_SOURCE_V6::BACK + P8R2_SOURCE_V6::FRONT )
      P8R2_SOURCE_V6 (EDISP) ( = P8R2_SOURCE_V6::EDISP0 + P8R2_SOURCE_V6::EDISP1 + P8R2_SOURCE_V6::EDISP2 + P8R2_SOURCE_V6::EDISP3 )
      P8R2_SOURCE_V6 (PSF) ( = P8R2_SOURCE_V6::PSF0 + P8R2_SOURCE_V6::PSF1 + P8R2_SOURCE_V6::PSF2 + P8R2_SOURCE_V6::PSF3 )
      P8R2_SOURCE_V6::BACK
      P8R2_SOURCE_V6::EDISP0
      P8R2_SOURCE_V6::EDISP1
      P8R2_SOURCE_V6::EDISP2
      P8R2_SOURCE_V6::EDISP3
      P8R2_SOURCE_V6::FRONT
      P8R2_SOURCE_V6::PSF0
      P8R2_SOURCE_V6::PSF1
      P8R2_SOURCE_V6::PSF2
      P8R2_SOURCE_V6::PSF3
      
      <...output for remainder of P8R2 irfs...>

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