Changeset 31022
- Timestamp:
- Mar 23, 2011, 10:08:25 AM (15 years ago)
- File:
-
- 1 edited
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branches/eam_branches/ipp-20110213/ippconfig/gpc1/psastro.config
r30982 r31022 15 15 PSASTRO.GRID.OFFSET F32 1000. 16 16 PSASTRO.GRID.SCALE F32 50 17 PSASTRO.GRID.NSTAR.MAX S32 800 # max stars accepted for fitting 17 PSASTRO.GRID.NSTAR.MAX S32 800 # deprecated 18 PSASTRO.GRID.NREF.MAX S32 800 # max stars accepted for fitting from ref catalog 19 PSASTRO.GRID.NRAW.MAX S32 1200 # max stars accepted for fitting from raw image 18 20 19 21 PSASTRO.MAX.NRAW S32 1000 # max stars accepted for fitting (0 for all) … … 44 46 PSASTRO.MATCH.RADIUS.N5 F32 10 45 47 PSASTRO.MATCH.RADIUS.N6 F32 10 46 PSASTRO.MATCH.RADIUS.N7 F32 547 PSASTRO.MATCH.FIT.NITER S32 848 PSASTRO.MATCH.RADIUS.N7 F32 5 49 PSASTRO.MATCH.FIT.NITER S32 8 48 50 49 51 # for iterations >= N, require a single match per reference … … 295 297 PSASTRO.CATDIR STR SAS.REF.V1 296 298 END 299 300 # these values worked to get solutions for the STS observations from 2009 & 2010 301 # these field has damage from excessive persistence and the impact of burntool 302 STS_DATASET METADATA 303 304 # need to boost the total number of stars available for the fit: 305 # allow more stars per chip and boost the density to which we query 306 # from the reference database. 307 PSASTRO.MAX.NRAW S32 2000 # 308 PSASTRO.MAX.NREF S32 8000 # max stars accepted for fitting (0 for all) 309 DVO.GETSTAR.MAX.RHO F32 60000.0 310 311 # the crowding is high, so unless we restrict somewhat tightly early 312 # on, we get very noisy (and wrong) fits. These values are probably 313 # too restrictive for the general observation: we would risk missing 314 # matches. 315 316 # single-chip radius match in pixels 317 PSASTRO.MATCH.RADIUS.N0 F32 10 318 PSASTRO.MATCH.RADIUS.N1 F32 5 319 PSASTRO.MATCH.RADIUS.N2 F32 5 320 PSASTRO.MATCH.RADIUS.N3 F32 5 321 PSASTRO.MATCH.RADIUS.N4 F32 3 322 PSASTRO.MATCH.RADIUS.N5 F32 3 323 PSASTRO.MATCH.RADIUS.N6 F32 5 324 PSASTRO.MATCH.RADIUS.N7 F32 5 325 PSASTRO.MATCH.FIT.NITER S32 5 326 END
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