CalDB 9 (20240815) ================== Listed below are the changes in XRISM CalDB 9 compared to CalDB 8. 1. The Resolve line-spread-functions file ("rmfparam") was replaced with a version that has updated FWHM calibration data based on inflight measurements. 2. Errors in the optical axis keywords in the Xtend instrument map file appeared in the CalDB 8 version of the file and have been corrected in CalDB 9. The optical axis position is still based on ground measurements and will be updated again based on inflight calibration results. 3. The values in the column TRAIL_PHCUT were changed by the Xtend instrument team from 0 to 1. CalDB 8 (20240315) ================== All the changes that have been made to CalDB files for this release of CalDB 8, compared to CalDB 7, are summarized below. 1. The Resolve pixel gain calibration has been updated by the Resolve instrument team, based on ground calibration. 2. The Xtend "FOC" coordinate offsets have been updated by Xtend team, based on inflight data. The updates are in the headers of the telescope definition file and instrument map files. The new FOC coordinate offsets provide improved alignment between Resolve and Xtend images and change the position of the "aim point" on the Xtend detector. Note that this change also affects the outcome of running the tool xaarfgen (which calculates the net effective area), because a celestial source with a given set of coordinates that are input to xaarfgen appears at a different position on the detector when the FOC offsets are changed. 3. The SAA boundaries were updated in the SAA CalDB file. The SAA definitions are different for Resolve and Xtend. 4. In the Resolve timing coefficients CalDB file, some of the entries suffered from numerical rounding errors, and these have been corrected. 5. The Resolve pulse templates configuration file was updated to reflect the gate valve closed status. 6. The Xtend rmfparam file was updated with a line spread function that better describes inflight data. CalDB 7 (20230815) ================== The XRISM CalDB 7 release contains some important changes compared to the previous CalDB release. The individual updates are summarized below. Note that as of this CalDB 7 release, older versions of very large files are not retained, in order to prevent large increases in the size of the CalDB with each release. In particular, the Resolve RMF parameters file, and some of the XMA files have older versions removed, and these files are also gzipped in the CalDB. They do not need to be uncompressed because the software will work whether they are compressed or not. 1. Revised quartz frequency versus temperature data have been used to revise the corresponding CalDB files for both SMU (Satellite Management Units) A & B. 2. The CalDB file holding selection expressions for data screening etc., has been updated. 3. The CalDB file that holds vignetting coefficients for the Resolve and Xtend telescopes has contents that are based on ground measurements of the XRISM telescopes. The CalDB 7 version of this file corrects some errors in the CalDB 6 version, so the latter is now obsolete and should not be used. The vignetting coefficients for each telescope are a set of numbers that are associated with empirical analytic functions that have been fitted to ground calibration results. These functions describe the changes in effective area as a function of energy and off-axis angle for a point source. 4. In addition to the vignetting coefficients CalDB file, six of the other eight XMA-related CalDB files (three for each XMA), have updates compared to their CalDB 6 counterparts. The updates correspond to (1) the inclusion of a bevel on the thermal shield mesh (based on ground measurements), and (2) refinement of the model for the support structures in the telescopes. The changes are identical for both telescopes. There is a net increase in the overall XMA effective area of ~0.5% up to ~8 keV, increasing to ~0.8% up to 30 keV. 5. The treatment of Resolve mid-res secondary pulses has been improved and the associated CalDB file has been updated. 6. An error in some of the Resolve "time coefficients" CalDB file was corrected, as well as an error in the pulse shape template identifier. Previous versions of this file in previous CalDB releases are now obsolete and should not be used. 7. A new extension was added to the MXS parameters CalDB file that allows the software to calculate afterglow properties analytically instead of using look-up tables. The CalDB file also has some keyword updates. Note that the Build 7 software will not work with earlier versions of the MXS parameters CalDB file. 8. The Resolve RMF parameters CalDB file was updated with refinements to the Gaussian core component FWHM of the line-spread functions. CalDB 6 (20230515) ================== XRISM CalDB 6 contains some significant changes and is launch-ready for XRISM. The individual updates are summarized below. Note that there are three possible Resolve gain CalDB files that can be selected, based on the date/time of the data being processed. Further details are given below, but here we note that no automated gain file CalDB selection is now appropriate for Hitomi-converted XRISM data. The current scheme gives priority to handling XRISM ground calibration data, and to actual XRISM flight data. However, the user is reminded that the software always allows any file that is retrieved by a CalDB call, to be specified, instead, as a direct input, as opposed to automated retrieval from CalDB. The older Resolve gain file that was the main Resolve gain file in the CalDB 1 release, and is suitable for processing Hitomi-converted data, is still present in CalDB 6. However, since fully-converted Hitomi data will have event dates and times that run into XRISM ground calibration time intervals, the CalDB file appropriate for Hitomi-converted data will not be selected automatically by the software. After installing and initializing XRISM CalDB 6, the user can copy the Resolve gain file suitable for Hitomi-converted data over to the current directory by: cp $CALDB/data/xrism/resolve/bcf/gain/xa_rsl_gainpix_20140101vh003.fits . This file is then specified directly as input to the software, instead of "CALDB". All the changes that have been made to CalDB files, compared to the previous CalDB 5a release, are summarized below. 1. Revised quartz frequency versus temperature data have been used to revise the corresponding CalDB files for both SMU (Satellite Management Units) A & B. 2. The CalDB file holding selection expressions for data screening etc., has been updated. 3. The CalDB file that holds vignetting coefficients for the Resolve and Xtend telescopes now has contents that are based on ground measurements of the XRISM telescopes. The vignetting coefficients for each telescope are a set of numbers that are associated with empirical analytic functions that have been fitted to ground calibration results. These functions describe the changes in effective area as a function of energy and off-axis angle. 4. In addition to the vignetting coefficients CalDB file, the other eight XMA-related CalDB files (four for each XMA), have significant updates that are based on ground calibration and fine-tuning of the raytracing models for each telescope. Together, these new CalDB files constitute the first self-consistent XMA calibration in the CalDB. Previous versions of the CalDB had XMA CalDB files whose contents were identical to the contents of the corresponding Hitomi files. 5. The Resolve pixel gain file was updated, based on further work on ground calibration data. 6. Some header keyword updates were made to the Resolve secondary pulses CalDB file. 7. Header keywords for the optical axes and FOC coordinate offsets were updated in the "teldef" and instrument map CalDB files for both Resolve and Xtend. The updates are based on ground calibration, and alignment measurements. The FOC offsets place point-source data from both instruments at the same position in FOC coordinates. The aim point for Resolve is at the geometric center of the 6x6 pixel array, and the corresponding aim point on Xtend is implicitly encoded in the Xtend FOC offsets. After the launch of XRISM, the optical axes and FOC offsets will be refined, based on inflight calibration. 8. The transmission of the Resolve optical blocking filter was updated. 9. The FWHM data for the Gaussian cores of the line-spread-function in the Resolve RMF parameters CalDB file were updated. 10. In the Resolve "time coefficients" CalDB file, the coefficients for converting Resolve raw trigger times to calibrated photon arrival times for the five event grades, and for each pixel, were updated. The relative time shifts that define the window for flagging coincidence with antico events were also updated for both PSP-A and PSP-B in this file. 11. Some updates were made to the MXS parameters CalDB file, including handling of pulse start and stop times, and the treatment of afterglow. There is also a column name change, so the MXS CalDB file will no longer work with earlier versions of the software. 12. The Resolve Filter Wheel CalDB filter file for the Polyimide/Al filter was updated with a new film transmission function, and with a more sophisticated treatment of the mesh, using new raytracing results, and corrections for bevels on the edge of the mesh structures. 13. The Xtend bad pixel CalDB file was updated. CalDB 5a (20221201) =================== The changes that have been made to CalDB files compared to those in the previous release, CalDB 5, are summarized below. 1) In the "mkfconf" CalDB file, some changes were made to the names of HK extensions. This file will be valid for observation dates on or after 2022-08-05:00:01:00. Before that date, a CalDB call will pick up the previous version of the file. 2) The Xtend "gain", and RMF CalDB files were replaced, based on revised or new data provided by provided by the Xtend team. Previous versions of these files are obsolete. 3) The Xtend teldef is updated. The file no longer contains any place holders left over from the adoption of the Hitomi teldef data. Some errors and typos in header comments were corrected. Also, some numerical coordinate conversion data that was hard-wired into header comments have been removed so that if/when the data change, the changes will be made only to data tables, and do not have to be mirrored in header changes. The optical axis in this teldef is set to the initial intended aim point on the observation CCD, 8mm from each edge at the corner nearest to the center of the detector. The FOC coordinate offsets are set so that the a source appearing at the optical axis in both Resolve and Xtend will appear at the origin of the FOC coordinate system. The optical axis and FOC offsets will be refined in the next version of the teldef, based on ground measurements of the instrument and telescope misalignments, and they will be further refined post-launch, based on inflight data. 4) The Xtend "mask" file that describes the locations of the non-active pixels and calibration sources is updated. Previously it was simply adopted from the Hitomi version. The new version is based on measurements provided by the Xtend instrument team. A corresponding new Xtend instrument map file is included, which also includes relevant keyword and header comment updates corresponding to the Xtend teldef revisions. 5) The Xtend quantum efficiency file is updated, based on new data from the Xtend instrument team. 6) An error was discovered in one of the new Resolve "gainpix" files that was included in the CalDB 5 release (for observation times > 2021-12-13:06:54). That file is replaced with a corrected one, and the previous version (xa_rsl_gainpix_20190101v003.fits) is obsolete, and should not be used. For convenience, here is a summary of the CalDB 5a Resolve gain CalDB files, along with their associated observation time intervals. 6a) t < 2018-09-13 -- Use the Hitomi-based gain file xa_rsl_gainpix_20140101vh003.fits 6b) 2018-09-13 = t < 2019-09-03:18:35:00 -- Use xa_rsl_gainpix_20190101v001.fits, which is based on a ground calibration campaign in September 2018. 6c) 2019-09-03:18:35:00 = t < 2021-12-13:06:54 -- Use xa_rsl_gainpix_20190101v002.fits, which is based on a ground calibration campaign in September 2019. 6d) t = 2021-12-13:06:54 -- Use xa_rsl_gainpix_20190101v004.fits, which is based on a ground calibration campaign in December 2021. The software will pick up the file appropriate for the observation time when CALDB is specified for the file name. However, as noted above, Hitomi-converted XRISM data has observation times that are not compatible with the above gain file time intervals, so the user must manually specify the file listed as 6d) above. 7) One of the new Resolve "confthre" (shape template) files in the CalDB 5 release was not indexed correctly because of a keyword error. The erroneous file has been replaced and the indexing has been corrected. The previous file (xa_rsl_confthre_20190101v004.fits) is obsolete and is replaced by xa_rsl_confthre_20190101v005.fits. 8) A new Resolve CalDB file is introduced, which defines a pulse height "clipping threshold" for each pixel. Further details on the clipping thresholds will be provided in updated help files for the relevant software. 9) A new Resolve teldef is included. Some errors and typos in header comments were corrected. The image location of pixel 12 (the calibration pixel) has also been revised. In previous versions of the teldef, in an image made from unfiltered event data, pixel 12 events would appear at the center of the 6x6 Resolve array. However, this location has been changed to a position that is offset from the 6x6 array. The FOC offsets were set so that a source appearing at the optical axis in both Resolve and Xtend will appear at the origin of the FOC coordinate system. The optical axis and FOC offsets will be refined in the next version of the teldef, based on ground measurements of the instrument and telescope misalignments, and they will be further refined post-launch, based on inflight data. The Resolve instrument map CalDB file was also revised to correct header comments, and includes the above FOC offsets. CalDB 5 (20220630) ================== XRISM CalDB 5 still contains many files that are numerically identical to their Hitomi counterparts. These files have the letter 'h' inserted before the version number (e.g. 'v001' becomes 'vh001'). Note that there are now three possible Resolve gain CalDB files that can be selected, based on the date/time of the data being processed. Further details are given below, but here we note that no automated gain file CalDB selection is now appropriate for Hitomi-converted XRISM data. The current scheme gives priority to handling XRISM ground calibration data, and to pave the way for further modifications to the gain file in the future, which will eventually be appropriate for processing actual XRISM flight data. However, the user is reminded that the software always allows any file that is retrieved by a CalDB call, to be specified, instead, as a direct input, as opposed to automated retrieval from CalDB. The older Resolve gain file that was the main Resolve gain file in the CalDB 1 release, and is suitable for processing Hitomi-converted data, is still present in CalDB 5. However, since fully-converted Hitomi data will have event dates and times that run into XRISM ground calibration time intervals, the CalDB file appropriate for Hitomi-converted data will not be selected automatically by the software. After installing and initializing XRISM CalDB 5, the user can copy the Resolve gain file suitable for Hitomi-converted data over to the current directory by: cp $CALDB/data/xrism/resolve/bcf/gain/xa_rsl_gainpix_20140101vh003.fits . This file is then specified directly as input to the software, instead of "CALDB". All the changes that have been made to CalDB files, compared to CalDB 4, are summarized below. 1) In the "mkfconf" CalDB file, a column name was updated. 2) In the "select" CalDB file, Resolve PI threshold for selection criteria involving SLOPE_DIFFER was changed from 20,000 to 25,0000. 3) The Xtend "gain", "cti", "chtrail", "vtevnodd", and RMF CalDB files were replaced, based on revised values provided by the Xtend team. Note that these files have a CalDB "validity date" of 2021-04-01, and previous versions of these files are obsolete. Consquently, CalDB calls for these files will not work for any observational data that has a date earlier than this validity date. In such cases, the user must specify the files manually, as opposed to setting an input file parameter value to "CALDB". Similarly, the CalDB validity date for the latest Xtend "rmfparam" file is 2020-04-01, and previous versions of this file are obsolete. Therefore, CalDB calls for observational data that has a date earlier than this validity date will not work, so the "rmfparam" file must be specified manually for input to software tasks that use it. 4) Two new Resolve "gainpix" files were added, giving a total of three gain files that are active in CalDB 5. The software and CalDB selection protocols retrieve a gain file from CalDB that is appropriate for the dates and times associated with the event data being processed. The three time intervals are as follows: 4a) t < 2018-09-13 -- Use the Hitomi-based gain file xa_rsl_gainpix_20140101vh003.fits 4b) 2018-09-13 = t < 2019-09-03:18:35:00 -- Use xa_rsl_gainpix_20190101v001.fits, which is based on a ground calibration campaign in September 2018. 4c) 2019-09-03:18:35:00 = t < 2021-12-13:06:54 -- Use xa_rsl_gainpix_20190101v002.fits, which is based on a ground calibration campaign in September 2019. 4d) t = 2021-12-13:06:54 -- Use xa_rsl_gainpix_20190101v003.fits, which is based on a ground calibration campaign in December 2021. 5) Two new "confthre" files were added, each file being associated with one of the new pixel gain files mentioned above. The "confthre" files document the Resolve shape templates. 6) A new Resolve antico gain file ("gainant") was added. The new file is appropriate for event times later than or equal to 2019-09-17:00:00:00, and the previous version of the file is appropriate for earlier event times. The CalDB mechanism and software automatically pick up the correct file based on dates and times of the event data being processed. 7) Both Resolve and Xtend have their own "auxtran" CalDB file, and each file holds a dimensionless function of energy that is an effective area modifier that can be optionally applied by the ARF generator software. The effective area ground calibration of each instrument has not yet been completed, and the "auxtran" files in CalDB 4 and earlier, simply carried the Hitomi functions. For the CalDB 5 release, we reset both functions to unity, and in a future CalDB release, they may be updated to reflect ground and/or inflight knowledge of the effective area functions. CalDB 4 (20210927) ================= XRISM CalDB 4 still contains many files that are numerically identical to their Hitomi counterparts. These files have the letter 'h' inserted before the version number (e.g. 'v001' becomes 'vh001'). Note that the Resolve gain file (which was the "new gain" file that was in CalDB 3), is based on ground measurements for Resolve, which means that this gain file no longer works with XRISM data that is simulated by adapting Hitomi data. The CalDB released with the Build 3 software allowed the user to switch between the XRISM Resolve and Hitomi SXS-based gain files. However, that capability has been retired, in order to give priority to handling new, forthcoming XRISM calibration data, and to pave the way for further modifications to the gain file in the future. However, the software always allows any file that is retrieved by a CalDB call, to be specified, instead, as a direct input, as opposed to automated retrieval from CalDB. The other changes that have been made to CalDB files, compared to XRISM CalDB 3, are summarized below. 1) The "mirror" files for both XMA were replaced, utilizing a new, more complex file format that supports two new features. One of these is the accommodation of additional foils (compared to the Hitomi telescopes) at the innermost radii of each XMA. These foils do not have a thin-film coating, but improve stray light blocking. The second new feature is a more complex treatment of "external objects", that allows for more accurate modeling of the XMA thermal shields. However, the content of the mirror CalDB files in this release reflects the Hitomi parameters for the thermal shield - a more accurate model will populate the CalDB files in the future. Aside from the new innermost foil structure, the content of the mirror CalDB files remains the same as that in the corresponding CalDB 3 files. The updated version of xrtraytrace that is included in the Build 4 software release is back-compatible, and thus capable of handling both the old and new format mirror CalDB files. 2) The four Resolve filter wheel CalDB files, and the gate valve CalDB file, were replaced by files with a new, more complex file format that is designed to enable on-the-fly raytracing for the full range of input source type, and for arbitrary off-axis angles. The current older file format CalDB files only support pre-calculated raytracing functions, and were strictly valid only for on-axis point sources. The new files are back-compatible in the sense that they carry both the pre-calculated data as well as the geometric parameters to perform on-the-fly raytracing. However, software that utilizes the new features in the CalDB files is not yet available (it will consist of an updated ARF generator, and a new raytracing driver tool, xmasim). The older software (i.e., Build 3, and earlier), is able to use the appropriate portions of the content in the new-format files in a manner that is equivalent to using the old-format files. The pre-calculated raytracing content in the gate valve file, and in three of the filter-wheel files, are unchanged relative to the contents in the corresponding previous versions of the file. The exception is the Fe 55 filter file, in which an error in previous versions was corrected. Note that the models in the new portions of the file are not necessarily consistent with the pre-calculated raytracing results in the old portion of the files. New calculations will be performed for later CalDB releases, and consistency obtained, after the relevant software development is completed. 3) A new CalDB file was added that models the Resolve filter-wheel OPEN positions. The file will be utilized only after some future modifications and additions to the software tasks. Currently, the information in the CalDB file is hard-wired in the software. 4) Updates were made to two CalDB files that are used in calculations to calibrate time. Specifically, the quartz clock frequency-versus-temperature relations for SMU (Satellite Management Unit) A and B ("qclocka" and "qclockb" files respectively) are updated, based on ground measurements. 5) In the "coldef" (HK column definitions) and "delay" (time delay factors) CalDB files, data pertaining to the Hitomi HXI and SGD instruments were removed. 6) In the "mkfconf" CalDB file, some column names were updated from Hitomi to XRISM values. 7) In the "select" CalDB file, Xtend selection criteria relating to the STATUS bit were modified, and Xtend selection criteria related to the light leak parameters (e.g. MZDYE and MZNTE) were retired. 8) In the "mxsparam" CalDB file, two new pulse offset time keywords were added (SCDLTNOM and SCDLTRED), and these are accompanied by appropriate changes in the MXS-related software (see above). 9) The leap-second CalDB file is identical to the latest version in the HEASoft CalDB. The file included in the previous XRISM CalDB release had columns that were in a different order, although the contents of the file were already identical to the contents of the latest HEASoft CalDB file. The software tasks read the contents by column name, and not by column number, so in practice, there are no differences resulting from usage of the two different files. 10) The Xtend quantum efficiency (QE) CalDB file was replaced by the Xtend instrument team, with a version in which the QE functions are theoretical. Future versions of the file will have functions based on new ground measurements. 11) The Xtend "gain", "cti", "chtrail", "vtevnodd", and RMF CalDB files were replaced, based on revised values provided by the Xtend team. 12) The Xtend "config" CalDB file was retired, as it is no longer used. 13) Other, more minor, changes were made to some of the CalDB files,. e.g. epoch updates. 14) All three CalDB files relating to the Non X-ray Background (NXB) were retired because there will be new XRSIM tools and calibration data for treating the NXB in future software and CalDB releases. The XRSIM NXB data in previous versions of the CalDB were simply copies of the corresponding Hitomi data, and the Hitomi data and associated software tasks are still available. CalDB 3 (20200319) ================= The XRISM CalDB 3 still contains many files that are numerically identical to their Hitomi counterparts. These files have the letter 'h' inserted before the version number (e.g. 'v001' becomes 'hv001'). Note that the new Resolve gain file is based on new ground measurements for Resolve, which means that the new gain file will no longer work with XRISM data that is simulated by adapting Hitomi data. However, the CalDB released with the Build 3 software allows the user to switch between the XRISM Resolve and Hitomi SXS gain files (the default is the new XRISM file). In order to switch gain files, go to $CALDB/data/xrism/ and execute one of the following unix scripts: switch_to_oldgain.txt (to switch from new gain to old gain) switch_to_newgain.txt (to switch from old gain to new gain) The other changes that have been made to CalDB files compared to CalDB 2 are summarized below. - There is a new Resolve RMF parameter file with a new format that supports pixel-dependent response functions. Whilst the previous RMF parameter file supported pixel-dependence of the core Gaussian component of the line spread function, the new format supports pixel dependence of the exponential tail, the escape peaks, and the electron loss continuum (ELC). Also, the ELC is now a matrix such that the shape of the ELC depends on the input energy, instead of the ELC being a single function. In addition, the new RMF parameter file now supports fluorescent line emission components (which also pixel dependent). - There are updates to the Resolve time coefficients file, with small changes to some of the critical time values that affect Primary and Secondary event processing. - The Resolve optical blocking filter transmission function is revised. - The Xtend RMF parameter file is replaced with a revised version that has an updated format to support the changes to xtdrmf. This version contains a new column PRIMARY_CENTER that describes the effective PI value of the main Gaussian peak as a function of energy. Other columns remain the same from the previous version. CalDB 2 (20190915) ================== The XRISM CalDB 2 still contains many files that are numerically identical to their Hitomi counterparts. These files have the letter 'h' inserted before the version number (e.g. 'v001' becomes 'hv001'). Note that the new Resolve gain file is based on new ground measurements for Resolve, which means that the new gain file will no longer work with XRISM data that is simulated by adapting Hitomi data. However, the CalDB released with the Build 2 software allows the user to switch between the XRISM Resolve and Hitomi SXS gain files (the default is the new XRISM file). In order to switch gain files, go to $CALDB/data/xrism/ and execute one of the following unix scripts: switch_to_oldgain.txt (to switch from new gain to old gain) switch_to_newgain.txt (to switch from old gain to new gain) The other changes that have been made to CalDB files compared to CalDB 1 are summarized here: - A new CalDB file ('mxsparam') has been added to support the more complex treatment of Resolve MXS GTI that has been implemented in updated versions of the tasks rslmxstime and rslmxsgti (see help files for these tasks). - The Resolve quantum efficiency file ('quanteff') now supports pixel-dependent QE. - The file containing the log of Resolve detector thresholds and optimal filter templates ('confthre') has been revised. - The file containing pixel gain calibration data ('gainpix') has been revised. There are now data for higher-order polynomial fitting of the gain functions compared to Hitomi. - The file containing anti-co gain parameters has been revised. - In the Resolve 'teldef' and instrument map files, the optical axis position has been reset to the center of the detector. The position is (3.5,3.5) in DET coordinates. - The columns in the time delays file ('delay' file) and the MKF configuration ('mkfconf') file pertaining to the HXI and SGD have been eliminated. - The NXB EHK file ('nxbehk') had the incorrect TELESCOP keyword and this has now been corrected. CalDB 1 (20181203) ================== The first XRISM CalDB is based on the last-released Hitomi CalDB and it contains files that are numerically identical to their Hitomi counterparts, with the exception of the Resolve gate valve file. Other, non-numerical changes are listed below. The gain scale file (used by sxspha2pi) has been removed. The file names are similar to the corresponding Hitomi files, for XRISM pre-launch CalDB files the date and version portion of file names have been preserved, with addition of the letter 'h' inserted before the version number (e.g. 'v001' becomes 'hv001'), if the data are numerically identical to the corresponding Hitomi file. The changes to the CalDB files compared to the Hitomi CalDB are summarized here: - In the mirror vignetting file (under caldb/data/xrism/gen/), the HXI columns have been removed, and the SXS and SXI column names changed to RESOLVE and XTEND respectively. - In the "select" CalDB file (under caldb/data/xrism/gen/), rows corresponding to HXI have been removed. Also SUBSYS=SXS and SUBSYS=SXI were changed to SUBSYS=RESOLVE and SUBSYS=XTEND respectively. - The 'linefit' file (used by ahgainfit) was moved from caldb/data/hitomi/gen/ to caldb/data/gen/. - In the Resolve instrument map file (xa_rsl_instmap_20140101vh002.fits) some keywords have SXS in some keywords replaced by RSL. - The HXI columns in the SAA vertices file (under caldb/data/xrism/gen/) were removed. - The atomic scattering file under hitomi/gen was missing the TELESCOP and INSTRUME keywords so was not being indexed before. The Hitomi and XRISM versions of the files both now have the required keywords. - The Resolve gate valve will have a different design to that for the Hitomi SXS. Specifically, the new gate valve will not have the opaque "cross" structure that supported the Be window and mesh. The Resolve gate valve CalDB file currently models the gate valve structure as a simple hole (diameter 29 mm) in an opaque, infinite plane parallel to the focal plane, located at a height of 243.9 mm above the focal plane. The Be filter and mesh transmission versus energy function in the Build 1 XRISM CalDB file is identical to that used for Hitomi (but will be replaced later).