1 / 5

MR_filter + SExtractor (current placeholder in catalog pipeline).

Sources detection method used at Saclay :. MR_filter + SExtractor (current placeholder in catalog pipeline). Already applied at DC1 (J. Ballet presentation at closeout) http://www-glast.slac.stanford.edu/software/Workshops/Feb04DC1CloseOut/agenda.htm

milek
Télécharger la présentation

MR_filter + SExtractor (current placeholder in catalog pipeline).

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Sources detection method used at Saclay : MR_filter + SExtractor (current placeholder in catalog pipeline). Already applied at DC1 (J. Ballet presentation at closeout) http://www-glast.slac.stanford.edu/software/Workshops/Feb04DC1CloseOut/agenda.htm Optimal filter method. developed by J. Ballet. Already applied at DC1 (same presentation as above) 3D wavelet filtering (space + energy or time). developed by J.L. Starck. Some ideas presented in J.L. Starck's summary talk in May 2005 http://www-glast.slac.stanford.edu/ScienceTools/workshops/May05DiffuseCat/agenda.htm My modest contribution for DC2: use a 2d binned Poisson likelihood

  2. Use the Egret fortran program LIKE(1994) J.R. Mattox, D.J. Macomb, D.L.Bertsch, J.A. Esposito Why ? I already used it on Egret data. Not fancy but it works very well. Fast. Adjust the diffuse emission model (Gmult, Gbias). Characterisation not as good as 3d models. Alternative method for the catalog.

  3. 40 47 46 45 44 43 42 41 48 37 36 35 34 33 32 31 30 38 27 26 25 24 23 22 21 20 28 17 16 15 14 13 12 11 10 18 7 6 5 4 3 2 1 0 8 What have I done so far ? Developped a cpp wrapper for Like: Like *like=new Like(“counts_g12_30_g002.fits”,2,“cfgas.gal.g002b”,20); like->Set_ROI(60,120,-90,90); like->Set_Sources("sources_gal_g004b_17.list"); like->Set_PSFADJ("MA0"); like->Set_PSFADJ("MAR"); like->do_LM(0.05,25,“y","LM_Output"); delete like; Run Like with the 1997 (P14) and 2001 (P19-reprocessed) Egret data Combined it with Sextractor to detect the likelihood map excess Code to merge results from all maps (gal,eq, energies, zones, periodes) into a catalog

  4. Results with Egret data and diffuse emission : All the sources in catalog were found. Found 12 new sources (not in catalog nor in Egret lower sign. source list) 82 (80) catalog sources are not any more significant. 61 (70) new significant sources should appear in the catalog.

  5. To do list for DC2 Adapt Like for resolution other than 0.5 deg. Generate: Like-PSF file from DC2 PSF Counts and Exposure maps (weeks, days, energy bands) Galactic diffuse emission map Run it (1308 cpu at In2p3 cc-Lyon )

More Related