- Timestamp:
- Aug 7, 2014, 6:21:58 AM (12 years ago)
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branches/eam_branches/ipp-20140717/ippToPsps/jython/stackbatch.py
r37191 r37200 428 428 sqlLine.group("a."+filter+"ApRadius", "b.AP_MAG_RADIUS") 429 429 sqlLine.group("a."+filter+"KronRad", "b.MOMENTS_R1 * 2.5") 430 sqlLine.group("a."+filter+"PlateScale", "b.PLTSCALE") 430 431 431 432 sql = sqlLine.makeEquals("WHERE a." + filter + "ippDetectID = b.IPP_IDET") … … 519 520 520 521 sqlLine.group("a." + filter + model + "Radius", "b.EXT_WIDTH_MAJ") 521 sqlLine.group("a." + filter + model + "Ab", "b.EXT_WIDTH_M AJ/b.EXT_WIDTH_MIN")522 sqlLine.group("a." + filter + model + "Phi", " b.EXT_THETA")522 sqlLine.group("a." + filter + model + "Ab", "b.EXT_WIDTH_MIN/b.EXT_WIDTH_MAJ") 523 sqlLine.group("a." + filter + model + "Phi", "DEGREES(b.EXT_THETA)") 523 524 524 525 sqlLine.group("a." + filter + model + "RadiusErr", "b.EXT_WIDTH_MAJ_ERR") # these are not correctly defined. … … 526 527 sqlLine.group("a." + filter + model + "PhiErr", "b.EXT_THETA_ERR") # these are not correctly defined. 527 528 529 sqlLine.group("a." + filter + model + "Chisq", "b.EXT_CHISQ / b.EXT_NDOF") 530 531 # I have raExp = X_EXT 532 528 533 # XXX this is tricky: RA_EXT is not defined, but X_EXT is... 529 # sqlLine.group("a." + filter + model + "RaOff","b.X_EXT")530 # sqlLine.group("a." + filter + model + "DecOff","b.Y_EXT")531 # sqlLine.group("a." + filter + model + "RaErr", "b.X_EXT_SIG * b.PLTSCALE")532 # sqlLine.group("a." + filter + model + "DecErr", "b.Y_EXT_SIG * b.PLTSCALE")534 sqlLine.group("a." + filter + model + "Ra", "b.X_EXT") 535 sqlLine.group("a." + filter + model + "Dec", "b.Y_EXT") 536 sqlLine.group("a." + filter + model + "RaErr", "b.X_EXT_SIG") # need to modify by platescale 537 sqlLine.group("a." + filter + model + "DecErr", "b.Y_EXT_SIG") 533 538 534 539 # sersic fit has an extra parameter … … 547 552 548 553 # insert detection information for each filter based on the DVO contents 554 # XXX since I already have extracted StackObjectRaw, this is probably faster using that table: 549 555 sqlLine = sqlUtility("UPDATE " + tablename + " AS a, " + self.scratchDb.dvoDetectionTable + " as b SET") 550 556 sqlLine.group("a." + filter + model + "Mag", "a." + filter + model + "Mag + b.zp") 551 557 sql = sqlLine.makeEquals("WHERE a.objID = b.objID AND a." + filter + "ippDetectID = b.ippDetectID") 558 559 self.logger.infoPair('sql', sql) 560 try: 561 self.scratchDb.execute(sql) 562 except: 563 self.logger.errorPair('failed sql',sql) 564 return 565 566 # we have (modulo signs): 567 # gRaExp = gra + (X_EXT - gxPos)*gPlateScale / cos(gdec) 568 # gDecExp = gdec + (Y_EXT - gyPos)*gPlateScale 569 570 rawS = "c." + filter + "PlateScale" 571 572 extR = "a." + filter + model + "Ra" 573 rawR = "b." + filter + "ra" 574 rawX = "c." + filter + "xPos" 575 576 extD = "a." + filter + model + "Dec" 577 rawD = "b." + filter + "dec" 578 rawY = "c." + filter + "yPos" 579 580 # dRA / dX = -PlateScale 581 # b.+filter+ra - (a.+filter+model+Ra - c.+filter+xPos)*c.+filter+PlateScale / cos(+filter+dec) 582 # extR = rawR - (extR - rawX)*rawS / 3600.0 / cos(rawD) 583 584 # dDEC / dY = +PlateScale 585 # b.+filter+dec + (a.+filter+model+Dec - c.+filter+xPos)*c.+filter+PlateScale / cos(+filter+dec) 586 # extD = rawD + (extD - rawY)*rawS / 3600.0 587 588 # insert detection information for each filter based on the DVO contents 589 sqlLine = sqlUtility("UPDATE " + tablename + " AS a, StackObjectThin as b, StackObjectRaw as c SET ") 590 sqlLine.group(extR, rawR + " - (" + extR + " - " + rawX + ")*" + rawS + " / 3600.0 / cos(radians(" + rawD + "))") 591 sqlLine.group(extD, rawD + " + (" + extD + " - " + rawY + ")*" + rawS + " / 3600.0") 592 field = "a." + filter + model + "RaErr" 593 sqlLine.group(field, field + "*" + rawS) 594 field = "a." + filter + model + "DecErr" 595 sqlLine.group(field, field + "*" + rawS) 596 sql = sqlLine.makeEquals("WHERE a.objID = b.objID AND a.objID = c.objID") 552 597 553 598 self.logger.infoPair('sql', sql) … … 760 805 self.scratchDb.execute(sql) 761 806 807 # instrumental flux, AB mags, Jy: 808 # flux_inst = cts / sec 809 # mag_AB = -2.5*log(flux_inst) + ZP [with appropriate definition of zero point] 810 # mag_AB = -2.5*log(flux_cgs) - 48.6 [by construction with ~Vega flux in V-band] 811 # flux_cgs = ten(-0.4*(mag_AB + 48.6)) 812 # flux_cgs = ten(-0.4*((-2.5*log(flux_inst) + ZP) + 48.6)) 813 # flux_cgs = flux_inst * ten(-0.4*(ZP + 48.6)) 814 # flux_Jy = flux_cgs * 10^23 815 # flux_Jy = flux_inst * ten(-0.4*(ZP + 48.6) + 23.0) [23.0 - 0.4*48.6 = 3.56] 816 # flux_Jy = flux_inst * ten(-0.4*ZP + 3.56) 817 # flux_Jy = flux_inst * ten(-0.4*ZP) * 3630.78 818 762 819 # modify flux to apply the zero point 763 # sqlLine = sqlUtility("UPDATE " + tablename + " AS a, " + self.scratchDb.dvoDetectionTable + " as b SET") 764 # field = filter + prefix + "flxR" + number 765 # sqlLine.group(field, field + " * POW(10, 3.56 - 0.4* b.zp)") 766 # sqlLine.group(field + "Err", field + "err" + " * POW(10, 3.56 - 0.4* b.zp)") 767 # sqlLine.group(field + "Std", field + "Std" + " * POW(10, 3.56 - 0.4* b.zp)") 768 # sql = sqlLine.makeEquals("WHERE a.objID = b.objID AND a." + filter + "ippDetectID = b.ippDetectID") 820 sqlLine = sqlUtility("UPDATE " + tablename + " AS a, " + self.scratchDb.dvoDetectionTable + " as b SET") 821 for number in numbers: 822 field = filter + prefix + "flxR" + number 823 sqlLine.group(field, field + " * POW(10, 3.56 - 0.4* b.zp)") 824 sqlLine.group(field + "Err", field + "err" + " * POW(10, 3.56 - 0.4* b.zp)") 825 sqlLine.group(field + "Std", field + "Std" + " * POW(10, 3.56 - 0.4* b.zp)") 826 sql = sqlLine.makeEquals("WHERE a.objID = b.objID AND a." + filter + "ippDetectID = b.ippDetectID") 769 827 770 828 '''
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