LSSTApplications
18.0.0+106,18.0.0+50,19.0.0,19.0.0+1,19.0.0+10,19.0.0+11,19.0.0+13,19.0.0+17,19.0.0+2,19.0.0-1-g20d9b18+6,19.0.0-1-g425ff20,19.0.0-1-g5549ca4,19.0.0-1-g580fafe+6,19.0.0-1-g6fe20d0+1,19.0.0-1-g7011481+9,19.0.0-1-g8c57eb9+6,19.0.0-1-gb5175dc+11,19.0.0-1-gdc0e4a7+9,19.0.0-1-ge272bc4+6,19.0.0-1-ge3aa853,19.0.0-10-g448f008b,19.0.0-12-g6990b2c,19.0.0-2-g0d9f9cd+11,19.0.0-2-g3d9e4fb2+11,19.0.0-2-g5037de4,19.0.0-2-gb96a1c4+3,19.0.0-2-gd955cfd+15,19.0.0-3-g2d13df8,19.0.0-3-g6f3c7dc,19.0.0-4-g725f80e+11,19.0.0-4-ga671dab3b+1,19.0.0-4-gad373c5+3,19.0.0-5-ga2acb9c+2,19.0.0-5-gfe96e6c+2,w.2020.01
LSSTDataManagementBasePackage
|
Classes | |
class | BiasConfig |
class | BiasTask |
class | CalibArgumentParser |
class | CalibCombineConfig |
class | CalibCombineTask |
class | CalibConfig |
class | CalibIdAction |
class | CalibStatsConfig |
class | CalibStatsTask |
class | CalibTask |
Base class for constructing calibs. More... | |
class | CalibTaskRunner |
class | DarkConfig |
class | DarkTask |
class | FlatConfig |
class | FlatTask |
class | FringeConfig |
class | FringeTask |
class | SkyConfig |
class | SkyTask |
Functions | |
def | getSize (dimList) |
def | dictToTuple (dict_, keys) |
Return a tuple of specific values from a dict. More... | |
def | getCcdIdListFromExposures (expRefList, level="sensor", ccdKeys=["ccd"]) |
Determine a list of CCDs from exposure references. More... | |
def | mapToMatrix (pool, func, ccdIdLists, args, kwargs) |
def lsst.pipe.drivers.constructCalibs.dictToTuple | ( | dict_, | |
keys | |||
) |
Return a tuple of specific values from a dict.
This provides a hashable representation of the dict from certain keywords. This can be useful for creating e.g., a tuple of the values in the DataId that identify the CCD.
dict_ | dict to parse |
keys | keys to extract (order is important) |
Definition at line 185 of file constructCalibs.py.
def lsst.pipe.drivers.constructCalibs.getCcdIdListFromExposures | ( | expRefList, | |
level = "sensor" , |
|||
ccdKeys = ["ccd"] |
|||
) |
Determine a list of CCDs from exposure references.
This essentially inverts the exposure-level references (which provides a list of CCDs for each exposure), by providing a dataId list for each CCD. Consider an input list of exposures [e1, e2, e3], and each exposure has CCDs c1 and c2. Then this function returns:
{(c1,): [e1c1, e2c1, e3c1], (c2,): [e1c2, e2c2, e3c2]}
This is a dict whose keys are tuples of the identifying values of a CCD (usually just the CCD number) and the values are lists of dataIds for that CCD in each exposure. A missing dataId is given the value None.
expRefList | List of data references for exposures |
level | Level for the butler to generate CCDs |
ccdKeys | DataId keywords that identify a CCD |
Definition at line 199 of file constructCalibs.py.
def lsst.pipe.drivers.constructCalibs.getSize | ( | dimList | ) |
Determine a consistent size, given a list of image sizes
Definition at line 176 of file constructCalibs.py.
def lsst.pipe.drivers.constructCalibs.mapToMatrix | ( | pool, | |
func, | |||
ccdIdLists, | |||
args, | |||
kwargs | |||
) |
Generate a matrix of results using pool.map The function should have the call signature: func(cache, dataId, *args, **kwargs) We return a dict mapping 'ccd name' to a list of values for each exposure. @param pool Process pool @param func Function to call for each dataId @param ccdIdLists Dict of data identifier lists for each CCD name @return matrix of results
Definition at line 250 of file constructCalibs.py.