Changeset 39377
- Timestamp:
- Feb 23, 2016, 4:53:15 PM (10 years ago)
- Location:
- trunk/Ohana/src
- Files:
-
- 10 edited
-
addstar/src/find_matches_ICRF.c (modified) (1 diff)
-
libdvo/include/dvo.h (modified) (1 diff)
-
relphot/src/ImageOps.c (modified) (1 diff)
-
relphot/src/MosaicOps.c (modified) (2 diffs)
-
relphot/src/StarOps.c (modified) (4 diffs)
-
relphot/src/initialize.c (modified) (1 diff)
-
relphot/src/relphot_images.c (modified) (1 diff)
-
relphot/src/relphot_objects.c (modified) (1 diff)
-
relphot/src/setMrelCatalog.c (modified) (1 diff)
-
relphot/src/setMrelFinal.c (modified) (1 diff)
Legend:
- Unmodified
- Added
- Removed
-
trunk/Ohana/src/addstar/src/find_matches_ICRF.c
r38441 r39377 140 140 catalog[0].measure[Nmeas].catID = catID; 141 141 142 catalog[0].average[n].flags |= ID_ ICRF_QSO;142 catalog[0].average[n].flags |= ID_OBJ_ICRF_QSO; 143 143 144 144 stars[N].found = TRUE; -
trunk/Ohana/src/libdvo/include/dvo.h
r39359 r39377 172 172 /* Average.flags values -- these values are 32 bit (as of PS1_V1) */ 173 173 typedef enum { 174 ID_STAR_FEW = 0x00000001, // used within relphot: skip star 175 ID_STAR_POOR = 0x00000002, // used within relphot: skip star 176 ID_ICRF_QSO = 0x00000004, // object IDed with known ICRF quasar (may have ICRF position measurement) 177 ID_OTHEF_QSO = 0x00000008, // object IDed with known or suspected quasar, without ICRF reference data 178 ID_PROPER = 0x00000010, // star with large proper motion 179 ID_TRANSIENT = 0x00000020, // identified as a non-periodic (stationary) transient 180 ID_VARIABLE = 0x00000040, // identified as a periodic variable 181 ID_ASTEROID = 0x00000080, // identified with a known solar-system object (asteroid or other) 182 ID_STACK_ASTROM = 0x00000100, // stack position used for astrometry 183 184 // bits 0x00000200 - 0x00008000 are currently unused 185 ID_OBJ_BEST_STACK = 0x00008000, // the primary stack measurement are the best measurements 186 ID_STAR_FIT_AVE = 0x00010000, // average position fitted 187 ID_STAR_FIT_PM = 0x00020000, // proper motion fitted 188 ID_STAR_FIT_PAR = 0x00040000, // parallax fitted 189 ID_STAR_USE_AVE = 0x00080000, // average position used (not PM or PAR) 190 ID_STAR_USE_PM = 0x00100000, // proper motion used (not AVE or PAR) 191 ID_STAR_USE_PAR = 0x00200000, // parallax used (not AVE or PM) 192 ID_STAR_NO_ASTROM = 0x00400000, // mean astrometry could not be measured 193 ID_STAR_BAD_PM = 0x00800000, // mean astrometry could not be measured 194 ID_OBJ_EXT = 0x01000000, // extended in our data (eg, PS) 195 ID_OBJ_EXT_ALT = 0x02000000, // extended in external data (eg, 2MASS) 196 ID_OBJ_GOOD = 0x04000000, // good-quality measurement in our data (eg,PS) 197 ID_OBJ_GOOD_ALT = 0x08000000, // good-quality measurement in external data (eg, 2MASS) 198 ID_OBJ_GOOD_STACK = 0x10000000, // good-quality object in the stack (> 1 good stack) 199 ID_OBJ_SUSPECT_STACK = 0x20000000, // suspect object in the stack (> 1 good or suspect stack, < 2 good) 200 ID_OBJ_BAD_STACK = 0x40000000, // good-quality object in the stack (> 1 good stack) 174 ID_OBJ_FEW = 0x00000001, // used within relphot: skip star 175 ID_OBJ_POOR = 0x00000002, // used within relphot: skip star 176 // NOTE: bits used for object classification: 177 ID_OBJ_ICRF_QSO = 0x00000004, // object IDed with known ICRF quasar (may have ICRF position measurement) 178 ID_OBJ_OTHEF_QSO = 0x00000008, // identified as likely QSO (Hernitschek et al 2015), without ICRF reference data 179 ID_OBJ_TRANSIENT = 0x00000010, // identified as a non-periodic (stationary) transient 180 ID_OBJ_VARIABLE = 0x00000020, // identified as a periodic variable 181 ID_OBJ_RRLYRA = 0x00000040, // identified as likely RR Lyra (Hernitschek et al 2015) 182 ID_OBJ_HAS_SOLSYS_DET = 0x00000080, // identified with a known solar-system object (asteroid or other) 183 ID_OBJ_ALL_SOLSYS_DET = 0x00000100, // identified with a known solar-system object (asteroid or other) 184 // bits 0x00000200 - 0x00000400 are currently unused 185 // NOTE: bits used for astrometry analysis 186 ID_OBJ_LARGE_PM = 0x00000800, // star with large proper motion 187 ID_OBJ_RAW_AVE = 0x00001000, // simple weighted average position was used (no IRLS fitting) 188 ID_OBJ_FIT_AVE = 0x00002000, // average position was fitted 189 ID_OBJ_FIT_PM = 0x00004000, // proper motion model was fitted 190 ID_OBJ_FIT_PAR = 0x00008000, // parallax model was fitted 191 ID_OBJ_USE_AVE = 0x00010000, // average position used (not PM or PAR) 192 ID_OBJ_USE_PM = 0x00020000, // proper motion used (not AVE or PAR) 193 ID_OBJ_USE_PAR = 0x00040000, // parallax used (not AVE or PM) 194 ID_OBJ_NO_MEAN_ASTROM = 0x00080000, // mean astrometry could not be measured 195 ID_OBJ_STACK_FOR_MEAN = 0x00100000, // stack position used for mean astrometry 196 ID_OBJ_MEAN_FOR_STACK = 0x00200000, // mean astrometry could not be measured 197 ID_OBJ_BAD_PM = 0x00400000, // failure to measure proper-motion model 198 // NOTE: bits used for photometry analysis 199 ID_OBJ_EXT = 0x00800000, // extended in our data (eg, PS) 200 ID_OBJ_EXT_ALT = 0x01000000, // extended in external data (eg, 2MASS) 201 ID_OBJ_GOOD = 0x02000000, // good-quality measurement in our data (eg,PS) 202 ID_OBJ_GOOD_ALT = 0x04000000, // good-quality measurement in external data (eg, 2MASS) 203 ID_OBJ_GOOD_STACK = 0x08000000, // good-quality object in the stack (> 1 good stack) 204 ID_OBJ_BEST_STACK = 0x10000000, // the primary stack measurement are the best measurements 205 ID_OBJ_SUSPECT_STACK = 0x20000000, // suspect object in the stack (> 1 good or suspect stack, < 2 good) 206 ID_OBJ_BAD_STACK = 0x40000000, // good-quality object in the stack (> 1 good stack) 201 207 } DVOAverageFlags; 202 208 -
trunk/Ohana/src/relphot/src/ImageOps.c
r39357 r39377 772 772 if (PoorImages) { 773 773 IMAGE_BAD = ID_IMAGE_PHOTOM_POOR | ID_IMAGE_PHOTOM_FEW | ID_IMAGE_PHOTOM_SKIP; 774 STAR_BAD = ID_ STAR_POOR | ID_STAR_FEW;774 STAR_BAD = ID_OBJ_POOR | ID_OBJ_FEW; 775 775 MEAS_BAD = ID_MEAS_NOCAL | ID_MEAS_POOR_PHOTOM | ID_MEAS_SKIP_PHOTOM | ID_MEAS_AREA; 776 776 } -
trunk/Ohana/src/relphot/src/MosaicOps.c
r39290 r39377 1036 1036 if (PoorImages) { 1037 1037 IMAGE_BAD = ID_IMAGE_PHOTOM_POOR | ID_IMAGE_PHOTOM_FEW | ID_IMAGE_PHOTOM_SKIP; 1038 STAR_BAD = ID_ STAR_POOR | ID_STAR_FEW;1038 STAR_BAD = ID_OBJ_POOR | ID_OBJ_FEW; 1039 1039 MEAS_BAD = ID_MEAS_NOCAL | ID_MEAS_POOR_PHOTOM | ID_MEAS_SKIP_PHOTOM | ID_MEAS_AREA; 1040 1040 } … … 1351 1351 if (PoorImages) { 1352 1352 IMAGE_BAD = ID_IMAGE_PHOTOM_POOR | ID_IMAGE_PHOTOM_FEW | ID_IMAGE_PHOTOM_SKIP; 1353 STAR_BAD = ID_ STAR_POOR | ID_STAR_FEW;1353 STAR_BAD = ID_OBJ_POOR | ID_OBJ_FEW; 1354 1354 MEAS_BAD = ID_MEAS_NOCAL | ID_MEAS_POOR_PHOTOM | ID_MEAS_SKIP_PHOTOM | ID_MEAS_AREA; 1355 1355 } -
trunk/Ohana/src/relphot/src/StarOps.c
r38466 r39377 756 756 if (N < Nminmeas) { /* too few measurements */ 757 757 // fprintf (f, "%10.6f %10.6f %d %d %d\n", catalog[Nc].averageT[j].R, catalog[Nc].averageT[j].D, catalog[Nc].measureT[catalog[Nc].averageT[j].measureOffset].imageID, N, STAR_TOOFEW); 758 catalog[Nc].secfilt[Nsecfilt*j+Nsec].flags |= ID_ STAR_FEW;758 catalog[Nc].secfilt[Nsecfilt*j+Nsec].flags |= ID_OBJ_FEW; 759 759 if (Ncode == 0) { 760 760 results->Ncode ++; … … 764 764 continue; 765 765 } else { 766 catalog[Nc].secfilt[Nsecfilt*j+Nsec].flags &= ~ID_ STAR_FEW;766 catalog[Nc].secfilt[Nsecfilt*j+Nsec].flags &= ~ID_OBJ_FEW; 767 767 } 768 768 … … 1108 1108 mark = (dM > MaxScatter) || (isnan(Mchisq)) || (Mchisq > MaxChisq); 1109 1109 if (mark) { 1110 catalog[i].secfilt[Nsecfilt*j+Nsec].flags |= ID_ STAR_POOR;1110 catalog[i].secfilt[Nsecfilt*j+Nsec].flags |= ID_OBJ_POOR; 1111 1111 Ndel ++; 1112 1112 if (dM > MaxScatter) { Nscat ++; } … … 1114 1114 if (Mchisq > MaxChisq) { Nchi ++; } 1115 1115 } else { 1116 catalog[i].secfilt[Nsecfilt*j+Nsec].flags &= ~ID_ STAR_POOR;1116 catalog[i].secfilt[Nsecfilt*j+Nsec].flags &= ~ID_OBJ_POOR; 1117 1117 } 1118 1118 Nave ++; -
trunk/Ohana/src/relphot/src/initialize.c
r38062 r39377 32 32 33 33 IMAGE_BAD = ID_IMAGE_PHOTOM_POOR | ID_IMAGE_PHOTOM_FEW | ID_IMAGE_PHOTOM_SKIP; 34 STAR_BAD = ID_ STAR_POOR | ID_STAR_FEW;34 STAR_BAD = ID_OBJ_POOR | ID_OBJ_FEW; 35 35 MEAS_BAD = ID_MEAS_NOCAL | ID_MEAS_POOR_PHOTOM | ID_MEAS_SKIP_PHOTOM | ID_MEAS_AREA; 36 36 -
trunk/Ohana/src/relphot/src/relphot_images.c
r39344 r39377 90 90 int star_toofew; 91 91 92 // until we finish the grid analysis, do not reject stars out-of-hand based on ID_ STAR_FEW92 // until we finish the grid analysis, do not reject stars out-of-hand based on ID_OBJ_FEW 93 93 // XXX this is kind of poor: need to have a better distinctions about STAR_BAD in setMrel vs getMrel 94 94 star_toofew = STAR_TOOFEW; 95 95 STAR_TOOFEW = 0; 96 96 for (i = 0; i < NGRID; i++) { 97 STAR_BAD = ID_ STAR_POOR;97 STAR_BAD = ID_OBJ_POOR; 98 98 setMrel (catalog, Ncatalog, flatcorr); 99 STAR_BAD = ID_ STAR_POOR | ID_STAR_FEW;99 STAR_BAD = ID_OBJ_POOR | ID_OBJ_FEW; 100 100 setMgrid (catalog, flatcorr); 101 101 } 102 STAR_BAD = ID_ STAR_POOR | ID_STAR_FEW;102 STAR_BAD = ID_OBJ_POOR | ID_OBJ_FEW; 103 103 STAR_TOOFEW = star_toofew; 104 104 } -
trunk/Ohana/src/relphot/src/relphot_objects.c
r38986 r39377 63 63 Nsecfilt = catalog.Nsecfilt; 64 64 65 DVOAverageFlags astromBits = 66 ID_STAR_FIT_AVE | 67 ID_STAR_FIT_PM | 68 ID_STAR_FIT_PAR | 69 ID_STAR_USE_AVE | 70 ID_STAR_USE_PM | 71 ID_STAR_USE_PAR | 72 ID_STAR_NO_ASTROM ; 65 DVOAverageFlags photomBits = 66 ID_OBJ_EXT | // extended in our data (eg, PS) 67 ID_OBJ_EXT_ALT | // extended in external data (eg, 2MASS) 68 ID_OBJ_GOOD | // good-quality measurement in our data (eg,PS) 69 ID_OBJ_GOOD_ALT | // good-quality measurement in external data (eg, 2MASS) 70 ID_OBJ_GOOD_STACK | // good-quality object in the stack (> 1 good stack) 71 ID_OBJ_BEST_STACK | // the primary stack measurement are the best measurements 72 ID_OBJ_SUSPECT_STACK | // suspect object in the stack (> 1 good or suspect stack, < 2 good) 73 ID_OBJ_BAD_STACK; // good-quality object in the stack (> 1 good stack) 73 74 74 75 for (j = 0; j < catalog.Naverage; j++) { 75 catalog.average[j].flags &= astromBits; // reset all except astrometry bits76 catalog.average[j].flags &= ~photomBits; // reset all except astrometry bits 76 77 catalog.average[j].psfQF = NAN; // reset (will be re-calculated here) 77 78 catalog.average[j].psfQFperf = NAN; // reset (will be re-calculated here) -
trunk/Ohana/src/relphot/src/setMrelCatalog.c
r39362 r39377 351 351 int Nranking = magStatsByRanking (&results->psfData[Nsec], psfstats); 352 352 if (Nranking < Nminmeas) { 353 secfilt[Nsec].flags |= ID_ STAR_FEW;353 secfilt[Nsec].flags |= ID_OBJ_FEW; 354 354 } else { 355 355 secfilt[Nsec].M = psfstats->mean; -
trunk/Ohana/src/relphot/src/setMrelFinal.c
r38474 r39377 104 104 if (!simpleAverage) setMcalOutput (catalog, 1, flatcorr); 105 105 106 /* clear ID_ STAR_POOR, ID_STAR_FEW values before writing ??? */106 /* clear ID_OBJ_POOR, ID_OBJ_FEW values before writing ??? */ 107 107 /* ID_MEAS_NOCAL is an internal bit, so it should be cleared */ 108 108 // XXX eventually: move these internal flags to an internal-only catalog->FOO element (like found) 109 109 for (i = 0; i < catalog[0].Naverage; i++) { 110 catalog[0].average[i].flags &= ~ID_ STAR_FEW;111 catalog[0].average[i].flags &= ~ID_ STAR_POOR;110 catalog[0].average[i].flags &= ~ID_OBJ_FEW; 111 catalog[0].average[i].flags &= ~ID_OBJ_POOR; 112 112 off_t j; 113 113 for (j = 0; j < Nsecfilt; j++) { 114 catalog[0].secfilt[i*Nsecfilt+j].flags &= ~ID_ STAR_FEW;115 catalog[0].secfilt[i*Nsecfilt+j].flags &= ~ID_ STAR_POOR;114 catalog[0].secfilt[i*Nsecfilt+j].flags &= ~ID_OBJ_FEW; 115 catalog[0].secfilt[i*Nsecfilt+j].flags &= ~ID_OBJ_POOR; 116 116 } 117 117 off_t m = catalog[0].average[i].measureOffset;
Note:
See TracChangeset
for help on using the changeset viewer.
