0301690601/pps/P0301690601OBX000SUMMAR0000.HTM 100644 0 0 31120 13507660464 14575 0 ustar root 0 0
Observation Data Summary File
0301690601 Observation Data Summary File
Revolution | Target | Scheduled Length | Observer |
1058 | Ursa Minor Dwarf | 4582 | Dr Thomas Maccarone |
Guest Observer Information
Dr Thomas Maccarone |
School of Physics & Astronomy |
University of Southampton |
Southampton |
Hampshire |
UNITED KINGDOM |
SO17 1BJ |
tjm@astro.soton.ac.uk |
Proposal Target Information
Target | : | Ursa Minor Dwarf |
Target RA [hms] | : | 15 09 11.34 |
Taget Dec [dms] | : | 67 12 51.70 |
Proposed Duration [s] | : | 12900 |
Boresight RA [hms] | : | 15 09 11.34 |
Boresight Dec [dms] | : | 67 12 51.70 |
Lower Pos Ang | : | 0 |
Upper Pos Ang | : | 360 |
SC Pos Ang | : | N |
AO | : | 4 |
Science Type | : | E |
Observation Record
Observation ID | : | 0301690601 |
Revolution | : | 1058 |
Odf Version | : | 004 |
Start time | : | 2005-09-19T15:02:35.000 |
Stop time | : | 2005-09-19T16:18:57.000 |
Exposure and Configuration Information
Inst. | Exp Id | Sched. | Mode | Data Mode | Filter | Position | Total Duration | Actual Start | Actual Stop |
---|
EMOS1 | S003 | Y | PrimeFullWindow | Imaging | CalClosed | NOT VALID CS | 4573 | 2005-09-19T15:02:36 | 2005-09-19T16:18:49 |
EMOS2 | S004 | Y | PrimeFullWindow | Imaging | CalClosed | NOT VALID CS | 4582 | 2005-09-19T15:02:35 | 2005-09-19T16:18:57 |
0301690601/pps/P0301690601OBX000PPSSUM0000.HTM 100644 0 0 22267 13507660464 14634 0 ustar root 0 0
PPS Processing Summary
0301690601 PPS Processing Summary
Revolution | Target | Scheduled Length | Observer |
1058 | Ursa Minor Dwarf | 4582 | Dr Thomas Maccarone |
EPIC Exposures processed by PPS
No EPIC exposures processed by the PPS.
OM Exposures processed by PPS
No OM exposures processed by the PPS.
RGS Exposures processed by PPS
No RGS exposures processed by the PPS.
0301690601/pps/PP0301690601PPSMSG000_0.ASC 100644 0 0 103534 13544433026 14270 0 ustar root 0 0
Delivery Note for Observation - 1058/0301690601 (Ursa Minor Dwarf)
===============================================================
XFTS Delivery Date to SOC : Mon Sep 30 19:06:30 2019
1 PCMS Processing
-----------------
Full release note for ppsprod-17.56
===================================
Pipeline Version: 17.56_20190403_1200
Pipeline name: ppsprod
Release Date: 2019-04-03
SAS Manifest: xmmsas_20190401_1820
Summary
=======
This pipeline is being released specifically for the reprocessing
of all XMM-Newton observations available to date with the goal
to generate a major new version of the EPIC Serendipitous Source
Catalogue. It is based on public SAS17.0 but in fact is much closer
to forthcoming SAS18.0.
The major changes outlined below refer to the pipeline used for
previous major version of the SSC catalogue, some of them were
already introduced in previous pipeline versions.
Improvements in calibrations are not
listed here as they can be found in SAS and/or CCFs release notes.
i) Extraction of source-specific products (SSP) (time-series and
spectra) for individual sources has undergone a major revision.
The size of the source extraction region is still optimized according
to the brightness of the source, but the region to estimate the
associated background is now restricted to the same CCD where the
center of the source is found, except for MOS SW modes, where an
annulus over the peripheral CCDs is chosen. PNG files with source
and background extraction regions overlaid on count images are also
new SSP products.
In the case of EPIC-pn Timing mode data the location of the source
in RAWX coordinate is determined as the
location of maximum of the RAWX histogram. The source extraction region
extends 9 RAWX columns on side of the source location and the
background region is fixed to RAWX in [2,6]. If the source and background
extraction regions are found to overlap or there are less than 100 counts
in the histogram, the source products are not created. In the case of
very strong spectra this method may produce a background with significant
contribution of the source at certain energies.
ii) EPIC lightcurves are produced per energy band for all exposures.
A new FITS file is available under the PPS products per EPIC instrument
and observation which contains lightcurves for all the available
exposures in the energy bands 1, 2, 3, 4, 5 and 8. For TIMING mode
information is given in the energy bands 2, 3, 4 and 9.
The time bin size for PN Light Curves has been fixed to 20 times
the frametime of the corresponding exposure mode. For MOS1/2 the
method to fix the time bin size according the mean count rate has
not been modified. Given the low count number per bin in most EPIC-pn
lightcurves the variability tests are computed on lightcurves rebinned
to an average of 20 counts per bin and the results of the tests are
saved in the header of the small time bin PPS product.
iii) The method to estimate the background in EPIC images has been
changed from splines interpolation to local smoothing of source free
regions. The new method in combination of an extra call to embadpixfind
task yield a reasonable compromise between detection number and spurious
content.
iv) Special flagging has been included for sources detected in OM low
sensitivity patch.
v) Quiescent particle background (estimated from Filter-Wheel-Closed
repository) and EPIC-pn out of time events are subtracted from EPIC
coloured images.
Other minor changes related to general info about observations
environment are
a) new PPS file with spacecraft orbit information as Geocentric Equatorial
J2000 and Geocentric Solar Ecliptic coordinates
b) new PPS file with Radiation Monitor count rates
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 FOOTPRINT | OFTPRT | EPICOBS | ASC | 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 |
| | 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 | | |
| | SPACECRAFT ORBIT | ORBTSR | PPSOBS | FIT | | |
| NEW | RADMON RATE | RADMON | PPSOBS | FIT | | |
| | 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_20190401_1820.
This manifest is built upon the version 17.0.0 release of the SAS
(manifest xmmsas_20180620_1732 - see
http://www.cosmos.esa.int/web/xmm-newton/sas-release-notes-1700.
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 17.0.0. The second column indicates
whether the task has a newer (>) or the same (=) version number in the
pipeline version.
|================|===|=================|============|
| TASK | | SAS 17.0.0 | 17.56 |
|================|===|=================|============|
|addattribute | = | 2.3 | 2.3 |
|arfgen | = | 1.98.3 | 1.98.3 |
|attcalc | = | 4.39 | 4.39 |
|attfilter | = | 4.39 | 4.39 |
|attbin | = | 1.5 | 1.5 |
|atthkgen | = | 1.22.1 | 1.22.1 |
|attmove | = | 1.6 | 1.6 |
|backscale | > | 1.5 | 1.6 |
|badpix | = | 2.33 | 2.33 |
|badpixfind | = | 1.41 | 1.41 |
|bkgoptrate | = | 1.8 | 1.8 |
|catcorr | > | 0.10 | 0.11 |
|catprep | > | 0.5.2 | 0.5.3 |
|cifbuild | = | 4.9 | 4.9 |
|dpssflag | = | 11.6 | 11.6 |
|dpsssrc | = | 1.2.1 | 1.2.1 |
|dscopyblock | = | 1.11.1 | 1.11.1 |
|dscp | = | 1.11.1 | 1.11.1 |
|dsrm | = | 1.11.1 | 1.11.1 |
|eboxdetect | = | 4.28.2 | 4.28.2 |
|ebkgreg | = | 0.8 | 0.8 |
|echeckregion | > | 1.53.1 | 1.54 |
|ecoordconv | > | 1.53.1 | 1.54 |
|eexpmap | = | 4.12 | 4.12 |
|efftplot | = | 2.21 | 2.21 |
|ekstest | = | 2.8 | 2.8 |
|elcplot | = | 2.6 | 2.6 |
|emask | = | 2.15 | 2.15 |
|embadpixfind | > | 2.6 | 2.6.1 |
|emenergy | = | 8.9 | 8.9 |
|emevents | = | 8.8 | 8.8 |
|emeventsproj | = | 1.6 | 1.6 |
|emframes | = | 5.11 | 5.11 |
|emldetect | > | 7.4.1 | 7.5.2 |
|emosaic | = | 1.18 | 1.18 |
|emtaglenoise | = | 1.2 | 1.2 |
|eootepileupmask | = | 2.10 | 2.10 |
|epatplot | > | 1.21 | 1.22 |
|epevents | > | 6.53.1 | 6.55 |
|epexposure | = | 0.16 | 0.16 |
|epfast | = | 0.7 | 0.7 |
|epframes | > | 8.112.2 | 8.116 |
|epiclccorr | = | 1.22.2 | 1.22.2 |
|epproc | > | 2.23.1 | 2.24.1 |
|eposcorr | = | 3.13 | 3.13 |
|epreject | = | 5.18.1 | 5.18.1 |
|epnoise | > | 0.8 | 0.9 |
|esensmap | = | 3.13 | 3.13 |
|eslewchain | = | 1.17.1 | 1.17.1 |
|eslewsearch | = | 1.17.1 | 1.17.1 |
|esources | = | 1.5 | 1.5 |
|especget | > | 1.53.1 | 1.54 |
|esplinemap | = | 5.1.1 | 5.1.1 |
|etimeget | > | 1.53.1 | 1.54 |
|etruecolor | = | 1.30.1 | 1.30.1 |
|evalcorr | = | 0.8 | 0.8 |
|evlistcomb | = | 4.20 | 4.20 |
|evqpb | = | 0.5 | 0.5 |
|evselect | > | 3.64 | 3.68 |
|gtialign | = | 2.11 | 2.11 |
|gtimerge | = | 1.8 | 1.8 |
|hkgtigen | = | 1.15 | 1.15 |
|implot | = | 2.20 | 2.20 |
|implotregions | = | 1.1 | 1.1 |
|implotrgb | = | 2.20 | 2.20 |
|imweightadd | = | 1.68 | 1.68 |
|lccorr_pcms | = | 1.7 | 1.7 |
|lcplot | = | 1.22.1 | 1.22.1 |
|merge | = | 0.15 | 0.15 |
|odfingest | > | 3.31 | 3.32.1 |
|omatt | = | 2.57.1 | 2.57.1 |
|omcomb | = | 2.5 | 2.5 |
|omcosflag | > | 1.34 | 1.35 |
|omdetect | > | 5.37 | 5.41 |
|omdrifthist | = | 1.30.1 | 1.30.1 |
|omfastflat | = | 1.22 | 1.22 |
|omfastshift | = | 1.26 | 1.26 |
|omflatfield | = | 2.7 | 2.7 |
|omflatgen | = | 1.13 | 1.13 |
|omlcbuild | = | 1.41 | 1.41 |
|ommag | = | 3.12 | 3.12 |
|ommodmap | = | 2.26 | 2.26 |
|ommosaic | > | 2.9 | 2.10 |
|omgprep | = | 1.11 | 1.11 |
|omgrism | > | 1.26 | 1.29 |
|omgrismplot | > | 1.6 | 1.7 |
|omprep | = | 2.48 | 2.48 |
|omqualitymap | = | 1.5 | 1.5 |
|omregion | = | 2.15 | 2.15 |
|omsrclistcomb | = | 2.23 | 2.23 |
|ommergelists | = | 1.1 | 1.1 |
|omthconv | = | 1.35 | 1.35 |
|orbit | = | 2.12 | 2.12 |
|ppsslewsumm | = | 1.3 | 1.3 |
|ppssumm | = | 3.7 | 3.7 |
|preqgti | = | 0.10.1 | 0.10.1 |
|radmonfix | > | 0.3 | 0.5 |
|region | = | 7.15 | 7.15 |
|regionmask | = | 1.68 | 1.68 |
|rgsangles | = | 4.9 | 4.9 |
|rgsbadpix | = | 2.20 | 2.20 |
|rgsbkgmodel | = | 1.5.1 | 1.5.1 |
|rgsbkgmodelTest | = | 1.5.1 | 1.5.1 |
|rgsenergy | = | 2.2 | 2.2 |
|rgsevents | = | 3.13 | 3.13 |
|rgsfilter | = | 1.19 | 1.19 |
|rgsfluxer | = | 1.10 | 1.10 |
|rgsframes | = | 3.19 | 3.19 |
|rgsimplot | = | 1.18 | 1.18 |
|rgslccorr | = | 0.57 | 0.57 |
|rgsoffsetcalc | = | 1.19 | 1.19 |
|rgsregions | = | 1.23 | 1.23 |
|rgsrmfgen | = | 1.16 | 1.16 |
|rgssources | = | 6.3 | 6.3 |
|rgsspecplot | = | 2.23 | 2.23 |
|rgsspectrum | = | 2.9 | 2.9 |
|rmfgen | > | 2.6.1 | 2.8 |
|slconv | = | 2.6 | 2.6 |
|specgroup | = | 1.7 | 1.7 |
|srcmatch | > | 3.21 | 3.22 |
|tabcalc | = | 2.9 | 2.9 |
|tabgtigen | = | 2.13 | 2.13 |
|================|===|=================|============|
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:
=====> CCFs_table PENDING <====
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 17.0.0.
RMFs used in this pipeline were released August 16th, 2018.
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_v17.0.rmf |
| epn_e_bu23_sdY9_v17.0.rmf |
| epn_e_bu23_sY9_v17.0.rmf |
| epn_e_ef20_dY_v17.0.rmf |
| epn_e_ef20_sdY_v17.0.rmf |
| epn_e_ef20_sY_v17.0.rmf |
| epn_e_ff20_dY_v17.0.rmf |
| epn_e_ff20_sdY_v17.0.rmf |
| epn_e_ff20_sY_v17.0.rmf |
| epn_e_lw20_dY_v17.0.rmf |
| epn_e_lw20_sdY_v17.0.rmf |
| epn_e_lw20_sY_v17.0.rmf |
| epn_e_sw20_dY_v17.0.rmf |
| epn_e_sw20_sdY_v17.0.rmf |
| epn_e_sw20_sY_v17.0.rmf |
| epn_e_sw20_sdY6_v17.0.rmf |
| epn_e_sw20_sY6_v17.0.rmf |
| epn_e_ti40_sdY9_v17.0.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 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 | 16.9774 | 10.0691 | 6.1547 | 1.9844 | 0.5777 | 4.1236 | 5.0977 |
| epn | thin | 9.5242 | 8.1207 | 5.8665 | 1.9526 | 0.5771 | 3.3242 | 4.5585 |
| epn | medium | 8.3693 | 7.8679 | 5.7672 | 1.9292 | 0.5765 | 3.1924 | 4.4602 |
| epn | thick | 5.1065 | 6.0476 | 4.9896 | 1.8286 | 0.5699 | 2.5930 | 3.7637 |
| emos1 | open | 3.1885 | 2.1889 | 2.1508 | 0.7674 | 0.1494 | 1.0915 | 1.5192 |
| emos1 | thin | 1.7813 | 1.8011 | 2.0521 | 0.7557 | 0.1489 | 0.9291 | 1.3963 |
| emos1 | medium | 1.5637 | 1.7500 | 2.0174 | 0.7469 | 0.1486 | 0.9000 | 1.3700 |
| emos1 | thick | 1.0185 | 1.4197 | 1.7962 | 0.7164 | 0.1470 | 0.7778 | 1.2128 |
| emos2 | open | 3.2055 | 2.2018 | 2.1546 | 0.7759 | 0.1579 | 1.1004 | 1.5270 |
| emos2 | thin | 1.7753 | 1.8085 | 2.0555 | 0.7640 | 0.1575 | 0.9357 | 1.4028 |
| emos2 | medium | 1.5530 | 1.7568 | 2.0208 | 0.7546 | 0.1581 | 0.9064 | 1.3762 |
| emos2 | thick | 1.0039 | 1.4236 | 1.7995 | 0.7239 | 0.1556 | 0.7832 | 1.2182 |
|============|========|============================================================================|
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.
2 Data Product Screening Report
-------------------------------
XMM SSC data-product screening log
Version: 30-Sep-2019
Revolution 1058
Obs Seq. 0301690601
Target Ursa Minor Dwarf
Seq_id 145012
These data were processed as part of the bulk reprocessing of all
XMM-Newton observations, performed in 2019, which are used
in the 4XMM catalogue. It was not possible to visually screen the data
from this bulk reprocessing (as is done for daily processing), due
to the volume of data and limited human resources available.
Users can find below the previous screening reports, but they should
note that, due to significant changes in some of the processing
algorithms, there may be issues in the the new products that were not
present in the earlier screening reports, and vice versa.
If questions arise, please contact the XMM-Newton Science Operations
Centre at ESAC.
Maximum shift in EPIC attitude:
Pointing difference: 0.0 arcsec = 0 pixels
RA: 0.0 arcsec
Dec: 0.0 arcsec
Percentage of flaring time:
--
EPIC exposures used in the source detection:
--
** GENERAL COMMENTS
No science data at all
EPIC comments refer, in general, to Energy-band 8.
** EPIC MOS1
** EPIC MOS2
** EPIC PN
** epic
** RGS1, RGS2
** OM
** Catalogue cross-correlation products
0301690601/pps/P0301690601OBX000ORBTSR0000.FTZ 100644 0 0 1151515 13507660463 14672 0 ustar root 0 0 3a] P0301690601OBX000ORBTSR0000.FIT ZmF+SxW)߷J.W*;wS)qVIޚʏO *%u`i{]MM!-2trM-|bΣIkgaxĒO9y}$s+/ Kx4ag4cHS]2rj峀!9`oN:Q.E#ntYk㹋\Oh
&QAL)5pbI?_o3
MZLh(4JD+d9dpk,Mgͷ)W%PФ_frgex|\KLD,O@'R/4ÃOgI.$n?b5sx0rX>eɮȕf̶-pʞ\{@1m:\>>\3 <'coh