Full release note for ppsprod-16.34 =================================== Pipeline Version: 16.34_20170131_1230 Pipeline name: ppsprod Release Date: 2017-01-31 SAS Manifest: xmmsas_20170125_1110 Summary ======= This new version of the pipeline is based on SAS16.0 public release and includes two important changes for legacy products: -) Source detection algorithms are applied to slew data. -) Observations of the solar system objects can be processed such that X-rays images and spectra are correctly referred to the moving target. Changes have been introduced for the handling of background extraction: The method established in the previous pipeline version to define the background region for source products from pn data has now been extended to MOS. Note that this method is not applied to sources detected in CCD#1 of MOS cameras operated in "Small Window" readout mode, because the area exposed in that CCD is very small compared to the Point-Spread Function (PSF). Instead, background is estimated from an annulus centred on the source and extending inside the peripheral CCDs. Some new products are delivered to ease quick inspection of the data: -) A single file per souce which includes the plots of the light curves in all EPIC and RGS exposures of the observation. -) For every EPIC spectrum there is a new image file (PNG) which shows the source and background extraction regions. -) Time binning for RGS light curves is now adjusted for the brightness of the source. -) RGS spectral plots are produced without any binning in wavelength. The version of SAS being used is a pipeline-specific manifest xmmsas_20170125_1110. This is based on the public SAS release 16.0.0, described at http://www.cosmos.esa.int/web/xmm-newton/sas-release-notes-1600 Documentation ============= Documentation for this pipeline can be found at: http://www.cosmos.esa.int/web/xmm-newton/pipeline and links therein. Pipeline Summary ================ i. Products created. ii. SAS Tasks. iii. Calibration files. iv. Response matrices. v. Energy Bands. vi. Energy Conversion Factors. vii. Source Position Rectification. i. Products Created =================== The following table summarises all possible product files created by this pipeline. Withdrawn products are noted for completeness. Product file names are subdivided into components: Pooooooooooiiseeeccccccbnnn.ttt where: oooooooooo is the Observation Identifier. ii is the instrument. s is the scheduled flag. eee is the exposure number. cccccc is the file identifier given in the table below. b is the instrument specific field (ISF): Energy band for EPIC instruments. OM science window or OM filter code for OM products. Spectral order for RGS products. nnn is the hexidecimal source number or 000. ttt is the file type. |=============|==========================================|===================|=========|==============|========|==============| | Status/notes| Product Index Description | File Identifier | Class | File Types | ISF | Per Source | |=============|==========================================|===================|=========|==============|========|==============| | | EPIC OBSERVATION BOX-LOCAL SOURCE LIST | OBLSLI | EPICOBS | FIT | | | | | EPIC OBSERVATION BOX-MAP SOURCE LIST | OBMSLI | EPICOBS | FIT | | | | | EPIC OBSERVATION SENSITIVITY MAP | OSNSMP | EPICOBS | FIT | BAND | | | | EPIC SOURCE DS9 REGIONS | REGION | EPICOBS | ASC | | | | | EPIC OBSERVATION ML SOURCE LIST | OMSRLI | EPICOBS | FIT | | | | | EPIC SUMMARY SOURCE LIST | OBSMLI | EPICOBS | FIT,HTM | | | | | EPIC DETECTION MASK | DETMSK | EPICOBS | FIT | BAND | | | | EPIC MERGED BACKGROUND MAP | BKGMAP | EPICOBS | FIT | BAND | | | | EPIC MERGED EXPOSURE MAP | MEXPMP | EPICOBS | FIT | BAND | | | | EPIC OBSERVATION BACKGROUND MAP | OBKGMP | EPICOBS | FIT,PNG | BAND | | | | EPIC OBSERVATION EXPOSURE MAP | OEXPMP | EPICOBS | FIT,PNG | BAND | | | | EPIC OBSERVATION IMAGE | OIMAGE | EPICOBS | FIT,PNG | BAND | | | | EPIC THREE-COLOUR IMAGE | 3COLIM | EPICOBS | FIT,PNG | BAND | | | | EPIC OBSERVATION SUMMARY | SUMMAR | EPICOBS | HTM | | | | | EPIC MOS IMAGING MODE EVENT LIST | MIEVLI | EPICEXP | FIT | | | | | EPIC PN IMAGING MODE EVENT LIST | PIEVLI | EPICEXP | FIT | | | | | EPIC TIMING MODE EVENT LIST | TIEVLI | EPICEXP | FIT | | | | | EPIC FLARE BACKGROUND TIMESERIES | FBKTSR | EPICEXP | FIT,PDF | | | | | EPIC EXPOSURE MAP | EXPMAP | EPICEXP | FIT,PNG | BAND | | | | EPIC IMAGE | IMAGE_ | EPICEXP | FIT,PNG | BAND | | | | EPIC SOURCE DS9 REGION | SRCREG | EPICSRC | ASC | | Y | | | EPIC ANCILLARY RESPONSE FUNCTION | SRCARF | EPICSRC | FIT | | Y | | | EPIC SOURCE BACKGROUND SPECTRUM | BGSPEC | EPICSRC | FIT | | Y | | | EPIC SOURCE SPECTRUM | SRSPEC | EPICSRC | FIT | | Y | | NEW | EPIC SOURCE SPECTRUM | SRSPEC | EPICSRC | PNG | | Y | | | EPIC SOURCE TIMESERIES | SRCTSR | EPICSRC | FIT | BAND | Y | | | EPIC SOURCE SPECTRUM PLOT | SPCPLT | EPICSRC | PDF | | Y | | | EPIC SOURCE TIMESERIES PLOT | STSPLT | EPICSRC | PDF | BAND | Y | | | OM FULL-FRAME IMAGE | FIMAG_ | OMEXP | FIT | | | | | OM TRACKING STAR TIMESERIES | TSTRTS | OMEXP | FIT | | | | | OM FULL-FRAME SKY IMAGE | FSIMAG | OMEXP | FIT,PNG | | | | | OM TRACKING HISTORY PLOT | TSHPLT | OMEXP | PDF | | | | | OM OBSERVATION SOURCE LIST | OBSMLI | OMOBS | FIT | | | | | OM OBSERVATION SOURCE LIST MOSAIC | OBSMOS | OMOBS | FIT | | | | | OM RUDI-5 SOURCE LIST MOSAIC | RSISWS | OMOBS | FIT | | | | | OM FULL-FRAME HIRES SOURCE LIST MOSAIC | HSISWS | OMOBS | FIT | | | | | OM FULL-FRAME LORES SOURCE LIST MOSAIC | LSISWS | OMOBS | FIT | | | | | OM USER WINDOWS SOURCE LIST MOSAIC | USISWS | OMOBS | FIT | | | | | OM OBSERVATION SOURCE REGION | OBSMLI | OMOBS | ASC | | | | | OM RUDI-5 SOURCE REGION MOSAIC | RSISWS | OMOBS | ASC | | | | | OM FULL-FRAME HIRES SOURCE REGION MOSAIC | HSISWS | OMOBS | ASC | | | | | OM FULL-FRAME LORES SOURCE REGION MOSAIC | LSISWS | OMOBS | ASC | | | | | OM USER WINDOWS SOURCE REGION MOSAIC | USISWS | OMOBS | ASC | | | | | OM FULL-FRAME HIRES SKY IMAGE MOSAIC | HSIMAG | OMOBS | FIT,PNG | FILTER | | | | OM FULL-FRAME LORES SKY IMAGE MOSAIC | LSIMAG | OMOBS | FIT,PNG | FILTER | | | | OM RUDI-5 SKY IMAGE MOSAIC | RSIMAG | OMOBS | FIT,PNG | FILTER | | | | OM USER WINDOWS SKY IMAGE MOSAIC | USIMAG | OMOBS | FIT,PNG | FILTER | | | | OM OBSERVATION SUMMARY | SUMMAR | OMOBS | HTM | | | | | OM OSW SOURCE TIMESERIES | TIMESR | OMSRC | FIT,PDF | OSW | Y | | | OM GRISM DS9 REGIONS | SGSREG | OMSW | ASC | OSW | | | | OM GRISM DS9 SPECTRUM REGIONS | SPCREG | OMSW | ASC | OSW | | | | OM OSW FAST REGION FILE | SFSREG | OMSW | ASC | OSW | | | | OM OSW REGION FILE | SWSREG | OMSW | ASC | OSW | | | | OM FAST MODE OSW IMAGE | IMAGEF | OMSW | FIT | OSW | | | | OM FAST MODE OSW SKY IMAGE | SIMAGF | OMSW | FIT | OSW | | | | OM FAST MODE OSW SKY IMAGE | SIMAGF | OMSW | PNG | OSW | | | | OM GRISM SPECTRA LIST | SPECLI | OMSW | FIT | OSW | | | | OM OSW FAST SOURCE LIST | SFSRLI | OMSW | FIT | OSW | | | | OM OSW GRISM SOURCE LIST | SGSRLI | OMSW | FIT | OSW | | | | OM OSW IMAGE | IMAGE_ | OMSW | FIT | | | | | OM OSW SOURCE LIST | SWSRLI | OMSW | FIT | | | | | OM GRISM SOURCE SPECTRUM | SPECTR | OMSW | FIT,PDF | OSW | Y | | | OM GRISM-ALIGNED IMAGE | GIMAGE | OMSW | FIT | OSW | | | | OM OSW SKY IMAGE | SIMAGE | OMSW | FIT,PNG | | | | | RGS BACKGROUND MODEL | BGMODL | RGSEXP | FIT | ORDER | | | | RGS EVENT LIST | EVENLI | RGSEXP | FIT | | | | | RGS EXPOSURE MAP | EXPMAP | RGSEXP | FIT | | | | | RGS SOURCE LIST | SRCLI_ | RGSEXP | FIT | | | | | RGS WHOLE FIELD RESPONSE MATRIX | WREMAT | RGSEXP | FIT | ORDER | Y | | | RGS ENERGY-DISPERSION IMAGE | ORDIMG | RGSEXP | FIT,PNG | | | | | RGS FLARE BACKGROUND TIMESERIES | FBKTSR | RGSEXP | FIT | | | | | RGS IMAGE | IMAGE_ | RGSEXP | FIT,PNG | | | | | RGS WHOLEFIELD SPECTRUM | WFSPEC | RGSEXP | FIT,PDF | ORDER | | | | RGS FLUXED SPECTRUM | FLUXED | RGSOBS | FIT,PDF | ORDER | Y | | | RGS OBSERVATION SUMMARY | SUMMAR | RGSOBS | HTM | | | | | RGS CROSS-DISPERSION HISTOGRAM | DSPHIS | RGSSRC | FIT | ORDER | Y | | | RGS RESPONSE MATRIX | RSPMAT | RGSSRC | FIT | ORDER | Y | | | RGS SOURCE BACKGROUND SPECTRUM | BGSPEC | RGSSRC | FIT | ORDER | Y | | | RGS SOURCE SPECTRUM | SRSPEC | RGSSRC | FIT,PDF | ORDER | Y | | | RGS BACKGROUND SPECTRUM | SBSPEC | RGSSRC | FIT | ORDER | Y | | | RGS SOURCE BACKGROUND TIMESERIES | SRBTSR | RGSSRC | FIT | | Y | | | RGS SOURCE TIMESERIES | SRCTSR | RGSSRC | FIT | | Y | | | RGS SOURCE TIMESERIES PLOT | STSPLT | RGSSRC | PDF | | | | | MAIN CROSS CORRELATION PAGE | XCORRE | CATOBS | HTM | | | | | CATALOGUE DESCRIPTIONS | Dxxxxa | CATCAT | HTM | | | | | EPIC FOV CROSS-CORRELATION RESULTS | FOVRES | CATCAT | HTM | | | | | EPIC FOV CROSS-CORRELATION RESULTS | Fxxxxa | CATCAT | FIT | | | | | EPIC SOURCE CROSS-CORRELATION RESULTS | Sxxxxa | CATOBS | FIT | | | | | EPIC SOURCE CROSS-CORRELATION RESULTS | SRCRES | CATOBS | HTM | | | | | EPIC SOURCE CROSS-CORRELATION SUMMARY | SRCSUM | CATOBS | HTM | | | | | EPIC SOURCE CROSS-CORRELATION SUMMARY | SRCSUM | CATOBS | FIT | | | | | EPIC FOV CROSS-CORRELATION SUMMARY | FOVSUM | CATOBS | FIT | | | | | EPIC FOV CROSS-CORRELATION SUMMARY | FOVSUM | CATOBS | HTM | | | | | EPIC CATALOGUE PLOT | CATPLT | CATOBS | PDF | | | | | SEARCHED CATALOGUES | SRCHD_ | CATOBS | HTM | | | | | SEARCHED CATALOGUES | SRCHD_ | CATOBS | FIT | | | | | XMM-ROSAT IMAGE | ROSIMG | CATOBS | PDF | | | | | FINDING CHART | FCHART | CATSRC | PDF | | Y | | | PPS RUN MESSAGE | PPSMSG | PPSOBS | ASC | | | | | PPS SCRIPT LOG | SCRLOG | PPSOBS | ASC | | | | | ATTITUDE TIME SERIES | ATTTSR | PPSOBS | FIT | | | | | REFERENCE CATALOGUE | REFCAT | PPSOBS | FIT | | | | | CALIBRATION INDEX FILE | CALIND | PPSOBS | FIT | | | | | PPS PRODUCT INDEX | PINDEX | PPSOBS | FIT | | | | | PPS OBSERVATION SUMMARY | SUMMAR | PPSOBS | HTM | | | | | PPS RUN SUMMARY | PPSSUM | PPSOBS | HTM | | | | | SSC LOGO 1 | SSCLG1 | PPSOBS | PNG | | | | | SSC LOGO 2 | SSCLG2 | PPSOBS | PNG | | | | | CDS LOGO 1 | CDSLG1 | PPSOBS | PNG | | | | | CDS LOGO 2 | CDSLG2 | PPSOBS | PNG | | | | | CDS LOGO 3 | CDSLG3 | PPSOBS | PNG | | | |=============|==========================================|===================|=========|==============|========|==============| The files from the CAT* classes, are products generated by the Archival Catalogue and Database Subsystem (ACDS) at the Observatoire Astronomique de Strasbourg (OAS) - they are the result of cross-correlations of XMM sources with archival catalogues by the ACDS. They have been made previously but are outlined here for the first time. Those files with xxxxa tags are generated for each external catalogue that the XMM sources are correlated with. ii. SAS Tasks ============= The current pipeline uses a pipeline-specific SAS manifest xmmsas_20170125_1110. This manifest is built upon the version 16.0.0 release of the SAS (manifest xmmsas_20170112_1337 - see http://www.cosmos.esa.int/web/xmm-newton/sas-release-notes-1600. for details of the SAS task versions and changes relative to the previous SAS releases) but includes a number of specific task patches. SAS tasks used in the current pipeline are shown in the table below, along with their respective versions in SAS 16.0.0. The second column indicates whether the task has a newer (>) or the same (=) version number in the pipeline version. |================|===|=================|============| | TASK | | SAS 16.0.0 | 16.33 | |================|===|=================|============| |addattribute | = | 2.2.7 | 2.2.7 | |arfgen | = | 1.93.1 | 1.93.1 | |attcalc | = | 4.37 | 4.37 | |attfilter | = | 4.37 | 4.37 | |attbin | = | 1.3.3 | 1.3.3 | |atthkgen | = | 1.21 | 1.21 | |attmove | = | 1.5 | 1.5 | |backscale | = | 1.4.2 | 1.4.2 | |badpix | = | 2.32.3 | 2.32.3 | |badpixfind | = | 1.40 | 1.40 | |bkgoptrate | = | 1.7 | 1.7 | |catcorr | = | 0.9.1 | 0.9.1 | |catprep | = | 0.4.2 | 0.4.2 | |cifbuild | = | 4.8 | 4.8 | |dpssflag | = | 11.3.1 | 11.3.1 | |dpsssrc | = | 1.1 | 1.1 | |dscopyblock | = | 1.10 | 1.10 | |dscp | = | 1.10 | 1.10 | |dsrm | = | 1.10 | 1.10 | |eboxdetect | = | 4.27.3 | 4.27.3 | |ebkgreg | = | 0.7.2 | 0.7.2 | |echeckregion | = | 1.44.2 | 1.44.2 | |ecoordconv | = | 1.44.2 | 1.44.2 | |eexpmap | = | 4.11.1 | 4.11.1 | |efftplot | = | 2.20 | 2.20 | |ekstest | = | 2.7 | 2.7 | |elcplot | = | 2.5.3 | 2.5.3 | |emask | = | 2.14 | 2.14 | |embadpixfind | = | 2.5 | 2.5 | |emenergy | = | 8.8 | 8.8 | |emevents | = | 8.7 | 8.7 | |emeventsproj | = | 1.5.2 | 1.5.2 | |emframes | = | 5.10 | 5.10 | |emldetect | = | 7.0.3 | 7.0.3 | |emosaic | = | 1.17 | 1.17 | |emtaglenoise | = | 1.1 | 1.1 | |eootepileupmask | = | 2.9 | 2.9 | |epevents | = | 6.50.1 | 6.50.1 | |epexposure | = | 0.14 | 0.14 | |epfast | = | 0.6 | 0.6 | |epframes | = | 8.109.1 | 8.109.1 | |epiclccorr | = | 1.21.1 | 1.21.1 | |epproc | = | 2.21 | 2.21 | |eposcorr | = | 3.12.2 | 3.12.2 | |epreject | = | 5.17 | 5.17 | |epnoise | = | 0.7.3 | 0.7.3 | |esensmap | = | 3.12.2 | 3.12.2 | |eslewchain | = | 1.11 | 1.11 | |eslewsearch | = | 1.11 | 1.11 | |esources | = | 1.4.1 | 1.4.1 | |especget | = | 1.44.2 | 1.44.2 | |esplinemap | = | 5.0 | 5.0 | |etimeget | = | 1.44.2 | 1.44.2 | |etruecolor | = | 1.29 | 1.29 | |evalcorr | = | 0.7.1 | 0.7.1 | |evlistcomb | = | 4.19.2 | 4.19.2 | |evselect | = | 3.62 | 3.62 | |gtialign | = | 2.10 | 2.10 | |gtimerge | = | 1.7.2 | 1.7.2 | |hkgtigen | = | 1.14.2 | 1.14.2 | |implot | = | 2.19 | 2.19 | |implotregions | = | 0.4 | 0.4 | |implotrgb | = | 2.19 | 2.19 | |imweightadd | = | 1.67 | 1.67 | |lccorr_pcms | = | 1.6.1 | 1.6.1 | |lcplot | = | 1.21 | 1.21 | |merge | = | 0.14 | 0.14 | |odfingest | = | 3.30 | 3.30 | |omatt | = | 2.56.1 | 2.56.1 | |omcomb | = | 2.4.5 | 2.4.5 | |omcosflag | = | 1.33 | 1.33 | |omdetect | = | 5.36.1 | 5.36.1 | |omdrifthist | = | 1.29 | 1.29 | |omfastflat | = | 1.21 | 1.21 | |omfastshift | = | 1.25.1 | 1.25.1 | |omflatfield | = | 2.6.5 | 2.6.5 | |omflatgen | = | 1.12.2 | 1.12.2 | |omlcbuild | = | 1.40 | 1.40 | |ommag | = | 3.11.1 | 3.11.1 | |ommodmap | = | 2.24 | 2.24 | |ommosaic | = | 2.8.1 | 2.8.1 | |omgprep | = | 1.10 | 1.10 | |omgrism | = | 1.25.1 | 1.25.1 | |omgrismplot | = | 1.5.3 | 1.5.3 | |omprep | = | 2.47 | 2.47 | |omqualitymap | = | 1.4 | 1.4 | |omregion | = | 2.14.1 | 2.14.1 | |omsrclistcomb | = | 2.22.2 | 2.22.2 | |ommergelists | = | 1.0.5 | 1.0.5 | |omthconv | = | 1.34.1 | 1.34.1 | |ppsslewsumm | = | 1.1 | 1.1 | |ppssumm | = | 3.5 | 3.5 | |preqgti | = | 0.9 | 0.9 | |region | = | 7.13 | 7.13 | |regionmask | = | 1.67 | 1.67 | |rgsangles | = | 4.8 | 4.8 | |rgsbadpix | = | 2.19.1 | 2.19.1 | |rgsbkgmodel | = | 1.4.1 | 1.4.1 | |rgsbkgmodelTest | = | 1.4.1 | 1.4.1 | |rgsenergy | = | 2.1 | 2.1 | |rgsevents | = | 3.12.3 | 3.12.3 | |rgsfilter | = | 1.18.3 | 1.18.3 | |rgsfluxer | = | 1.9.2 | 1.9.2 | |rgsframes | = | 3.18 | 3.18 | |rgsimplot | = | 1.17.3 | 1.17.3 | |rgslccorr | = | 0.55 | 0.55 | |rgsoffsetcalc | = | 1.18.2 | 1.18.2 | |rgsregions | = | 1.22 | 1.22 | |rgsrmfgen | = | 1.15.6 | 1.15.6 | |rgssources | = | 6.2.2 | 6.2.2 | |rgsspecplot | = | 2.21 | 2.21 | |rgsspectrum | = | 2.8.2 | 2.8.2 | |rmfgen | = | 2.5.1 | 2.5.1 | |slconv | = | 2.5 | 2.5 | |specgroup | = | 1.6 | 1.6 | |srcmatch | = | 3.20 | 3.20 | |tabcalc | = | 2.8 | 2.8 | |tabgtigen | = | 2.12.3 | 2.12.3 | |================|===|=================|============| iii. Calibration Files ====================== Pipeline processing generally accesses an evolving set of CCFs (current calibration files). For each observation, a subset of the full set of CCFs is used in processing that pertains to the epoch of the observation; the CCF components/versions used are identified in the calibration index file (PooooooooooOBX000CALIND0000.FIT) that is included in the delivered observation data product set. The complete list of CCFs used in the processing is given here: Table of valid CCFs at 2017-01-19T02:00:08 |================================|=============|=======| | Calibration File | Issue range | Count | |================================|=============|=======| | EMOS1_ADUCONV | 0070-0086 | 17 | | EMOS1_BACKGROUND | 0001 | 1 | | EMOS1_BADPIX | 0025-0039(*)| 13 | | EMOS1_CALSOURCEDATA | 0001 | 1 | | EMOS1_CONTAMINATION | 0001 | 1 | | EMOS1_CTI | 0058-0074 | 17 | | EMOS1_DARKFRAME | 0011-0036 | 26 | | EMOS1_EFFICIENCY | 0001 | 1 | | EMOS1_FILTERTRANSX | 0015 | 1 | | EMOS1_FWC | 0001 | 1 | | EMOS1_HKPARMINT | 0008-0011 | 4 | | EMOS1_LINCOORD | 0018 | 1 | | EMOS1_MODEPARAM | 0006 | 1 | | EMOS1_PATTERNLIB | 0005 | 1 | | EMOS1_QUANTUMEF | 0020-0021 | 2 | | EMOS1_REDIST | 0106-0119 | 14 | | EMOS1_SCREENTHRESH | 0001 | 1 | | EMOS1_TIMECORR | 0003 | 1 | | EMOS2_ADUCONV | 0071-0087 | 17 | | EMOS2_BACKGROUND | 0001 | 1 | | EMOS2_BADPIX | 0017-0026(*)| 9 | | EMOS2_CALSOURCEDATA | 0001 | 1 | | EMOS2_CONTAMINATION | 0001 | 1 | | EMOS2_CTI | 0059-0075 | 17 | | EMOS2_DARKFRAME | 0011-0032 | 22 | | EMOS2_EFFICIENCY | 0001 | 1 | | EMOS2_FILTERTRANSX | 0015 | 1 | | EMOS2_FWC | 0001 | 1 | | EMOS2_HKPARMINT | 0008-0010 | 3 | | EMOS2_LINCOORD | 0018 | 1 | | EMOS2_MODEPARAM | 0006 | 1 | | EMOS2_PATTERNLIB | 0005 | 1 | | EMOS2_QUANTUMEF | 0020-0021 | 2 | | EMOS2_REDIST | 0106-0119 | 14 | | EMOS2_SCREENTHRESH | 0001 | 1 | | EMOS2_TIMECORR | 0003 | 1 | | EPN_ADUCONV | 0077-0142(*)| 36 | | EPN_BACKGROUND | 0001 | 1 | | EPN_BADPIX | 0093-0145 | 53 | | EPN_BUCLOSEDODI | 0001-0005 | 5 | | EPN_CALSOURCEDATA | 0001 | 1 | | EPN_CTI | 0047 | 1 | | EPN_DARKFRAME | 0001 | 1 | | EPN_EFFICIENCY | 0001 | 1 | | EPN_FILTERTRANSX | 0019 | 1 | | EPN_FWC | 0001 | 1 | | EPN_HKPARMINT | 0005 | 1 | | EPN_LINCOORD | 0009 | 1 | | EPN_MODEPARAM | 0003 | 1 | | EPN_PATTERNLIB | 0001 | 1 | | EPN_QUANTUMEF | 0018 | 1 | | EPN_REDIST | 0012 | 1 | | EPN_REJECT | 0006-0008(*)| 2 | | EPN_TICLOSEDODI | 0001-0013 | 13 | | EPN_TIMECORR | 0011-0015(*)| 4 | | EPN_TIMEJUMPTOL | 0001 | 1 | | OM_ASTROMET | 0012 | 1 | | OM_BADPIX | 0005 | 1 | | OM_COLORTRANS | 0010 | 1 | | OM_DARKFRAME | 0003 | 1 | | OM_DIFFUSEGALA | 0001 | 1 | | OM_GRISMCAL | 0004 | 1 | | OM_HKPARMINT | 0004 | 1 | | OM_LARGESCALESENS | 0002 | 1 | | OM_LINCOORD | 0001 | 1 | | OM_PHOTTONAT | 0005 | 1 | | OM_PIXTOPIXSENS | 0003 | 1 | | OM_PSF1DRB | 0010 | 1 | | OM_QUICKMAG | 0002 | 1 | | OM_ZODIACAL | 0001 | 1 | | RGS1_ADUCONV | 0006-0027(*)| 15 | | RGS1_BACKGROUND | 0001 | 1 | | RGS1_BADPIX | 0012-0034(*)| 9 | | RGS1_CALSOURCEDATA | 0001 | 1 | | RGS1_CLOCKPATTERNS | 0001 | 1 | | RGS1_COOLPIX | 0001 | 1 | | RGS1_CROSSPSF | 0004 | 1 | | RGS1_CTI | 0001-0014(*)| 9 | | RGS1_DARKFRAME | 0005 | 1 | | RGS1_EFFAREACORR | 0011 | 1 | | RGS1_EXAFS | 0005 | 1 | | RGS1_HKPARMINT | 0009-0015(*)| 5 | | RGS1_LINCOORD | 0008 | 1 | | RGS1_LINESPREADFUNC | 0005 | 1 | | RGS1_MODEPARAM | 0004-0005 | 2 | | RGS1_QUANTUMEF | 0015 | 1 | | RGS1_REDIST | 0004 | 1 | | RGS1_SAACORR | 0001 | 1 | | RGS1_TEMPLATEBCKGND | 0006 | 1 | | RGS2_ADUCONV | 0006-0033(*)| 17 | | RGS2_BACKGROUND | 0001 | 1 | | RGS2_BADPIX | 0012-0033(*)| 8 | | RGS2_CALSOURCEDATA | 0001 | 1 | | RGS2_CLOCKPATTERNS | 0001 | 1 | | RGS2_COOLPIX | 0001 | 1 | | RGS2_CROSSPSF | 0004 | 1 | | RGS2_CTI | 0001-0015(*)| 10 | | RGS2_DARKFRAME | 0006 | 1 | | RGS2_EFFAREACORR | 0011 | 1 | | RGS2_EXAFS | 0005 | 1 | | RGS2_HKPARMINT | 0008-0014(*)| 5 | | RGS2_LINCOORD | 0008 | 1 | | RGS2_LINESPREADFUNC | 0005 | 1 | | RGS2_MODEPARAM | 0004-0005 | 2 | | RGS2_QUANTUMEF | 0016 | 1 | | RGS2_REDIST | 0004 | 1 | | RGS2_SAACORR | 0001 | 1 | | RGS2_TEMPLATEBCKGND | 0007-0008 | 2 | | XMM_ABSCOEFS | 0004 | 1 | | XMM_BORESIGHT | 0027 | 1 | | XMM_MISCDATA | 0022 | 1 | | XMM_SPECQUAL | 0002 | 1 | | XRT1_XAREAEF | 0009 | 1 | | XRT1_XENCIREN | 0003 | 1 | | XRT1_XPSF | 0014 | 1 | | XRT2_XAREAEF | 0010 | 1 | | XRT2_XENCIREN | 0003 | 1 | | XRT2_XPSF | 0014 | 1 | | XRT3_XAREAEF | 0012 | 1 | | XRT3_XENCIREN | 0003 | 1 | | XRT3_XPSF | 0017 | 1 | |================================|=============|=======| (*): Incomplete range. Total number of valid CCFs required : 464 iv. Response Matrices ===================== The pipeline accesses a set of canned response matrices (RMFs) which correspond to those issued with the SAS public release used as base for it, here 16.0.0. RMFs used in this pipeline were released Apr 8, 2016. EPIC MOS RMFs are defined via a set of epoch-dependent files (14 epochs to date). They are further divided by instrument mode and by detector position - in particular, MOS RMFs are available to reflect the impacts of changes occurring in the core (c) and wings (w) of a small patch known to have suffered degradation, as well as off-patch (o) locations (i.e. everywhere else on the detector). PN RMFs are divided by instrument mode and position along the Y-direction of the CCDs. The canned EPIC response matrices used in the bulk reprocessing are shown below. |====================================| | Canned RMFs | |====================================| | m_e_im_p0_c.rmf | | m_e_im_p0_w.rmf | | m_e_im_p0_o.rmf | | m_e_im_pall_o.rmf | | m_e_im_pall_c.rmf | | m_e_im_pall_w.rmf | | m_e_tu_p0_c.rmf | | m_e_tu_p0_w.rmf | | m_e_tu_p0_o.rmf | | m_e_tu_pall_o.rmf | | m_e_tu_pall_c.rmf | | m_e_tu_pall_w.rmf | | | | epn_e_bu23_dY9_v16.0.rmf | | epn_e_bu23_sdY9_v16.0.rmf | | epn_e_bu23_sY9_v16.0.rmf | | epn_e_ef20_dY_v16.0.rmf | | epn_e_ef20_sdY_v16.0.rmf | | epn_e_ef20_sY_v16.0.rmf | | epn_e_ff20_dY_v16.0.rmf | | epn_e_ff20_sdY_v16.0.rmf | | epn_e_ff20_sY_v16.0.rmf | | epn_e_lw20_dY_v16.0.rmf | | epn_e_lw20_sdY_v16.0.rmf | | epn_e_lw20_sY_v16.0.rmf | | epn_e_sw20_dY_v16.0.rmf | | epn_e_sw20_sdY_v16.0.rmf | | epn_e_sw20_sY_v16.0.rmf | | epn_e_sw20_sdY6_v16.0.rmf | | epn_e_sw20_sY6_v16.0.rmf | | epn_e_ti40_sdY9_v16.0.rmf | |====================================| where = 1 (MOS1) or 2 (MOS2), , i=1-14 (MOS epochs), i=1-3 (PN epochs) and , j=0-9 (Y-positions); , m=5-9 (Y-positions); , n=7-9 (Y-positions); The latest available canned response files are described at, and available from, http://www.cosmos.esa.int/web/xmm-newton/epic-response-files. See also http://www.cosmos.esa.int/web/xmm-newton/epic-files-updates for further details on the latest update to EPIC RMFs. v. Energy Bands =============== |======|===================| | Band | Energy Range (eV) | |======|===================| | 1 | 200 - 500 | | 2 | 500 - 1000 | | 3 | 1000 - 2000 | | 4 | 2000 - 4500 | | 5 | 4500 - 12000 | | 8 | 200 - 12000 | | 9 | 500 - 4500 | |======|===================| vi. Energy Conversion Factors ============================= EPIC energy conversion factors (ECFs) are used to derive simple flux estimates from measured count rates. The ECFs are computed using the instrument response files (PN version 15.0) for an assumed absorbed power law model with Gamma=1.7 and an absorbing column density of 3x10^20/cm2. ECFs used in pipeline processing are not computed as functions of position or epoch but are fixed values, computed for each EPIC instrument and filter, for each energy band. They are presented in the table below. For PN they are based on the full-frame, on-axis position from epoch 3. For MOS they are based on the Full-frame (imaging) mode, off-patch RMF from epoch 14. Rather than compute an average ECF over time, a single epoch was chosen so as to relate to a specific epoch RMF. The largest epoch-dependence is in band 1 and amounts to a range of about 15%. The off-patch position was chosen to reflect the majority of sources - RMFs for the core and wings of the MOS 'patch' are only relevant to a very small number of objects in the field. In this pipeline, the following fixed energy conversion factors (ECFs) are used: |============|========|============================================================================| | Instrument | Filter | Band | | | | 1 | 2 | 3 | 4 | 5 | 8 | 9 | |============|========|============================================================================| | epn | open | 16.9773 | 10.0691 | 6.1545 | 1.9843 | 0.5778 | 4.1236 | 5.0977 | | epn | thin | 9.5243 | 8.1205 | 5.8670 | 1.9531 | 0.5765 | 3.3242 | 4.5586 | | epn | medium | 8.3692 | 7.8679 | 5.7674 | 1.9297 | 0.5764 | 3.1925 | 4.4604 | | epn | thick | 5.1061 | 6.0478 | 4.9895 | 1.8286 | 0.5694 | 2.5928 | 3.7636 | | emos1 | open | 3.1888 | 2.1888 | 2.1509 | 0.7674 | 0.1490 | 1.0914 | 1.5191 | | emos1 | thin | 1.7812 | 1.8014 | 2.0517 | 0.7557 | 0.1491 | 0.9292 | 1.3963 | | emos1 | medium | 1.5638 | 1.7499 | 2.0175 | 0.7471 | 0.1484 | 0.9000 | 1.3697 | | emos1 | thick | 1.0183 | 1.4197 | 1.7965 | 0.7161 | 0.1475 | 0.7780 | 1.2129 | | emos2 | open | 3.2054 | 2.2019 | 2.1545 | 0.7758 | 0.1580 | 1.1004 | 1.5271 | | emos2 | thin | 1.7758 | 1.8087 | 2.0556 | 0.7637 | 0.1578 | 0.9358 | 1.4029 | | emos2 | medium | 1.5533 | 1.7570 | 2.0205 | 0.7548 | 0.1569 | 0.9060 | 1.3761 | | emos2 | thick | 1.0038 | 1.4237 | 1.7992 | 0.7236 | 0.1556 | 0.7830 | 1.2181 | |============|========|============================================================================| vii. Source Position Rectification ================================== In the bulk reprocessing, astrometric field rectification (where possible) is performed against extracts from the USNO-B1.0, SDSS-DR9 or 2MASS catalogues as the astrometric reference frame.