give resolution time in minutes for the given user story, only provide the number of minutes in the output without any other text

User story: {code}  processCcd.py /lsst3/HSC/data/ --output /raid/price/test --id visit=904400 ccd=50  [...]  processCcd.calibrate.astrometry.solver.loadAN: Loading reference objects using center (1023.5, 2091) pix = Fk5Coord(319.8934727, -0.0006943, 2000.00) sky and radius 0.111920792477 deg  processCcd FATAL: Failed on dataId={'taiObs': '2013-11-03', 'pointing': 672, 'visit': 904400, 'dateObs': '2013-11-03', 'filter': 'HSC-Y', 'field': 'STRIPE82L', 'ccd': 50, 'expTime': 30.0}: Could not find flux field(s) y_camFlux, y_flux  Traceback (most recent call last):    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/cmdLineTask.py", line 320, in __call__      result = task.run(dataRef, **kwargs)    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/pipe_tasks/10.1-28-gf9582e4+2/python/lsst/pipe/tasks/processCcd.py", line 85, in run      result = self.process(sensorRef, postIsrExposure)    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/pipe_tasks/10.1-28-gf9582e4+2/python/lsst/pipe/tasks/processImage.py", line 160, in process      calib = self.calibrate.run(inputExposure, idFactory=idFactory)    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/pipe_tasks/10.1-28-gf9582e4+2/python/lsst/pipe/tasks/calibrate.py", line 457, in run      astromRet = self.astrometry.run(exposure, sources1)    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/meas_astrom/10.1-19-g6e01b25+5/python/lsst/meas/astrom/anetAstrometry.py", line 177, in run      results = self.astrometry(sourceCat=sourceCat, exposure=exposure, bbox=bbox)    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/meas_astrom/10.1-19-g6e01b25+5/python/lsst/meas/astrom/anetAstrometry.py", line 292, in astrometry      astrom = self.solver.determineWcs(sourceCat=sourceCat, exposure=exposure, bbox=bbox)    File "/home/lsstsw/stack/Linux64/meas_astrom/10.1-19-g6e01b25+5/python/lsst/meas/astrom/anetBasicAstrometry.py", line 409, in determineWcs      return self.determineWcs2(sourceCat=sourceCat, **margs)    File "/home/lsstsw/stack/Linux64/meas_astrom/10.1-19-g6e01b25+5/python/lsst/meas/astrom/anetBasicAstrometry.py", line 437, in determineWcs2      astrom = self.useKnownWcs(sourceCat, wcs=wcs, **kw)    File "/home/lsstsw/stack/Linux64/meas_astrom/10.1-19-g6e01b25+5/python/lsst/meas/astrom/anetBasicAstrometry.py", line 308, in useKnownWcs      calib = None,    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/meas_algorithms/10.1-15-g0d3ecf6/python/lsst/meas/algorithms/loadReferenceObjects.py", line 173, in loadPixelBox      loadRes = self.loadSkyCircle(ctrCoord, maxRadius, filterName)    File "/home/lsstsw/stack/Linux64/pipe_base/10.1-4-g6ba0cc7+15/python/lsst/pipe/base/timer.py", line 118, in wrapper      res = func(self, *args, **keyArgs)    File "/home/lsstsw/stack/Linux64/meas_astrom/10.1-19-g6e01b25+5/python/lsst/meas/astrom/loadAstrometryNetObjects.py", line 141, in loadSkyCircle      fluxField = getRefFluxField(schema=refCat.schema, filterName=filterName)    File "/home/lsstsw/stack/Linux64/meas_algorithms/10.1-15-g0d3ecf6/python/lsst/meas/algorithms/loadReferenceObjects.py", line 40, in getRefFluxField      raise RuntimeError("Could not find flux field(s) %s" % (", ".join(fluxFieldList)))  RuntimeError: Could not find flux field(s) y_camFlux, y_flux  {code}    We should be able to fix this by setting config parameters (e.g., {{calibrate.astrometry.solver.defaultFilter}} or {{calibrate.astrometry.solver.filterMap}}), but how do we keep that synched with the choice of reference catalog?  And once we get past astrometry, we also have the same problem in photocal.
Answer: 9726.0