Differences between revisions 3 and 6 (spanning 3 versions)
Revision 3 as of 2018-06-13 13:41:05
Size: 733
Comment:
Revision 6 as of 2019-01-16 12:26:11
Size: 1617
Comment:
Deletions are marked like this. Additions are marked like this.
Line 2: Line 2:

If you need access to the simulations or need more information contact us by email.
Line 10: Line 12:
 * Estimate on the performance of the default source detection
Line 21: Line 24:
AGN options: AGN:
Line 23: Line 26:
 * contacted Antara (Goddard) about a SIMPUT Catalog
 * alternative: use Catalog of N. Clerc for one skyfield and randomize positions and permutate models for all other skyfields
 * used the 4 AGN Catalogs by N. Clerc simulations as a "standard" catalog to get sources parameters
 * applied a 5e-15 erg/s flux threshold to the the catalog
 * rescaled the number of sources to match the 4700 skyfields for eROSITA and rolled new positions on a sphere
 * reduced the nbins in the spectra from 1000 to 100 to improve performance of the simulation
 * "remove" galactic NH from input catalog spectra
 * determined NH for each source and applied it to the spectra
 * more than 20.000.000 AGN
Line 29: Line 37:
 * List of sources and fluxes provided by Axel Schwope, spectrum and/or model information is needed  * Catalog of sources (CVS, IPS, POLARS) provided by Axel Schwope
 * applied a flux threshold 1.0e-15 erg/s
 * used unabsorbed flux / model / NH to create spectra useable by SIXTE
 * few 100.000 sources
Line 34: Line 45:
 * Beta Model?
 * Images?
   * SIMPUT catalog provided by Jeremy Sanders, Sebastian Grandis, John Mohr
 * more than 3.000.000 Galaxy Clusters with images
 * currently up to 1.0e-20 erg/s
 * next simulation will be reduced to match thresholds of other input catalogs
Line 40: Line 54:
 * contact Jan Robrade  * in contact Jan Robrade / Juergen Schmitt - plan to integrate catalog based on parts of the GAIA catalog

AllSkySurvey

If you need access to the simulations or need more information contact us by email.

Goals:

  • Test of Pipeline (eSASS) environment
  • Test of NRTA environment
  • Test of Data Access Tools (datool)
  • Handling the large amount of data
  • Derive computational requirements
  • Estimate on the performance of the default source detection

Objects Types (planned):

  • AGN
  • Galaxy Cluster
  • Stars
  • Cataclysmic Variables


AGN:

  • used the 4 AGN Catalogs by N. Clerc simulations as a "standard" catalog to get sources parameters
  • applied a 5e-15 erg/s flux threshold to the the catalog
  • rescaled the number of sources to match the 4700 skyfields for eROSITA and rolled new positions on a sphere
  • reduced the nbins in the spectra from 1000 to 100 to improve performance of the simulation
  • "remove" galactic NH from input catalog spectra
  • determined NH for each source and applied it to the spectra
  • more than 20.000.000 AGN


CV:

  • Catalog of sources (CVS, IPS, POLARS) provided by Axel Schwope
  • applied a flux threshold 1.0e-15 erg/s
  • used unabsorbed flux / model / NH to create spectra useable by SIXTE
  • few 100.000 sources


Galaxy Cluster:

  • SIMPUT catalog provided by Jeremy Sanders, Sebastian Grandis, John Mohr
  • more than 3.000.000 Galaxy Clusters with images
  • currently up to 1.0e-20 erg/s
  • next simulation will be reduced to match thresholds of other input catalogs


Stars:

  • in contact Jan Robrade / Juergen Schmitt - plan to integrate catalog based on parts of the GAIA catalog

EROSITAwiki: AllSkySurvey (last edited 2019-01-16 12:26:11 by ChristophGrossberger)