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Simulations of sources with flux f_X(0.5-2)=2e-12cgs in grid. Pointed observations and survey fields have been simulated. The latter use the [[https://wiki.mpe.mpg.de/eRosita/ScienceRelatedStuff/ExpoMaps?action=AttachFile&do=view&target=oneyearsurvey_att.fits|attitude file: oneyearsurvey_att.fits]]. Sixte and Simput versions 2.2.0 have been used. The EROSIM task with the [[attachment:erositaXML.tar|XML files]] and the [[attachment:erosita_psf_v2.1.fits|Panter PSF (256M!)]] was run followed by the ERO_CALEVENTS task. | Simulations of sources with flux f_X(0.5-2)=2e-12cgs in grid. Pointed observations and survey fields have been simulated. The latter use the [[https://wiki.mpe.mpg.de/eRosita/ScienceRelatedStuff/ExpoMaps?action=AttachFile&do=view&target=oneyearsurvey_att.fits|attitude file: oneyearsurvey_att.fits]]. Sixte and Simput versions 2.2.0 have been used. The EROSIM task with the [[attachment:erositaXML.tar|XML files]] and the [[attachment:erosita_psf_v2.1.fits|Panter PSF (256M!)]] was run followed by the ERO_CALEVENTS task. |
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The event files produced by this simulation for each telescope separately and merged into a single file (via evtool call) can be found here Issues with simulations: |
The table below lists links to the input simput file, the event files for each telescope separately and the merged one (via call to evtool): |
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Issues with simulations (to be addressed in the future): * the event files produced by ERO_CALEVENTS have columns RA and DEC of type 'J' (integer) in the 'EVENTS' extension. Should be 'E' or 'D' * the event files produced by EROSIM include events with negative energies. |
Description of performance tests and simulations relevant to the APETOOL and SHAPELIB libraries.
Simulations are underway to test the following aspects relevant to apetool and shapelib:
- How well/accurate can the shapelet-PSF model determine the flux of point-sources: simulate fields (both survey-mode and pointed) with a grid of point sources of fixed flux and spectral. Run ermldetect to detect the sources and measure their flux and compare with the input one.
- How well can APETOOL reconstruct the selection function of eROSITA observations: simulate fields (both survey-mode and pointed) with a point-sources with fluxes drawn from a logN-logS distribution and fixed spectral shape. Run ERLDETECT and ptoduce a source list, APETOOL to threshold at a given false detection probability and estimate field sensitivities. Reconstruct input logN-logS and compare.
The relevant simulations are based on modified versions of Nicolas Clerc's python scripts described here. The main modifications are: (i) functions to generate attitude files for both survey and pointed observations (ii) place sources in a grid of fixed spacing within the survey field, (iii) use of simple power-law X-ray spectra with a choice of Gammas for the point sources, (iv) functionality to produce sources of fixed flux. A tarball with the relevant python scripts can be found [[|here(to be added soon)]].
Progress so far
Simulations of sources with flux f_X(0.5-2)=2e-12cgs in grid. Pointed observations and survey fields have been simulated. The latter use the attitude file: oneyearsurvey_att.fits. Sixte and Simput versions 2.2.0 have been used. The EROSIM task with the XML files and the Panter PSF (256M!) was run followed by the ERO_CALEVENTS task.
The table below lists links to the input simput file, the event files for each telescope separately and the merged one (via call to evtool):
simput file |
|
Event file for CCD1 |
|
Event file for CCD2 |
|
Event file for CCD3 |
|
Event file for CCD4 |
|
Event file for CCD5 |
|
Event file for CCD6 |
|
Event file for CCD7 |
|
Merged Event file |
Issues with simulations (to be addressed in the future):
- the event files produced by ERO_CALEVENTS have columns RA and DEC of type 'J' (integer) in the 'EVENTS' extension. Should be 'E' or 'D'
- the event files produced by EROSIM include events with negative energies.