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Philippe Gris
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| # sn_tools | ||
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| . | ||
| * \_\_init\_\_.py | ||
| * sn_analyze_simu.py | ||
| * sn_cadence_tools.py | ||
| * sn_clusters.py | ||
| * sn_io.py | ||
| ## sn_cadence_tools.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |ReferenceData | class | handling SN LC templates | | ||
| |GenerateFakeObservations | class | generating fake observations| | ||
| |TemplateData | class | loading template LC| | ||
| |AnaOS | class | observing strategy analysis| | ||
| |Match_DD | function | matching data to DD fields| | ||
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| ## sn_clusters.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |ClusterObs | class | identifying clusters (RA,Dec) of data points| | ||
| |getVisitsBand | function | estimating the number of visits per band| | ||
| |getName | function | getting the field name corresponding to RA| | ||
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| ## sn_io.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |Read_Sqlite | class| reading a sqlite file (from scheduler) and convert to numpy array| | ||
| | append|function |numpy array concatenation| | ||
| |getMetricValues|function |reading and analyzing files from metrics| | ||
| |geth5Data|function |loading the content of hdf5 files| | ||
| |getLC|function |accessing a table in hdf5 file from key| | ||
| |getFile|function |pointing to hdf5 file| | ||
| |selectIndiv|function |applying a selection on an array of data| | ||
| |select|function |applying few selections on an array of data| | ||
| |loadFile|function |loading file according to the type of data it contains| | ||
| |loopStack|function |load files and stack results according to the type of data it contains| | ||
| |convert_to_npy|function |stacking pandas df and converting to numpy array| | ||
| |convert_save|function |convert and save output to hdf5 file| | ||
| |remove_galactic_area|function |excluding galactic plane from data| | ||
| |getObservations|function |extracting observations (db scheduler->numpy array)| | ||
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| * sn_lcana.py | ||
| * sn_obs.py | ||
| * sn_rate.py | ||
| * sn_telescope.py | ||
| * sn_throughputs.py | ||
| * sn_utils.py | ||
| * sn_visu.py | ||
| * sn_calcFast.py | ||
| ## sn_obs.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |PavingSky| class | paving the sky with rectangles| | ||
| |DataInside | class | select data points (RA,Dec) inside a area| | ||
| |DataToPixels | class | match observations to pixels| | ||
| |ProcessPixels | class | processing (metrics) on a set of pixelized data| | ||
| |ProcessArea | class | processing (metrics) on a given part of the sky| | ||
| |DDFields | function | defining DD fields| | ||
| |patchObs | function |getting informations and patches on the sky| | ||
| |getPix| function |grabbing pixels information| | ||
| |area| function |making a dict of coordinates| | ||
| |areap| function |making polygon out of coordinates| | ||
| |areap_diamond| function |defining diamonds| | ||
| |proj_gnomonic_plane| function |performing a gnomonic projection on a plane| | ||
| |proj_gnomonic_sphere| function |performing a gnomonic projection on a sphere| | ||
| |renameFields| function |renaming fields of a numpy array| | ||
| |fillCorresp| function |filling a dict used in renameFields| | ||
| |pixelate| function |pixelating the sky with data| | ||
| |season| function |estimating seasons | | ||
| |LSSTPointing| function |LSST focal plane| | ||
| |LSSTPointing_circular| function |LSST focal plane made circular| | ||
| |getFields_fromId| function |getting fields using fieldIds column| | ||
| |getFields| function |get a type of fields (DD or WFD) from a set of observations| | ||
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| ## sn_rate.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |SN_Rate | class |Estimating production rate of typeIa SNe| | ||
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| ## sn_telescope.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |Telescope | class |generating a telescope | | ||
| |get_val_decor|function|decorator to access class params| | ||
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| ## sn_throughputs.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |Throughputs | class | handling instrument throughputs| | ||
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| ## sn_utils.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |MultiProc|class|performing multiprocessing| | ||
| |GenerateSample|class|generating a sample of parameters for simulation| | ||
| |Make_Files_for_Cadence_Metric|class|producing files requested as input for the Cadence Metric| | ||
| |X0_norm|class|estimating X0s| | ||
| |DiffFlux|class|estimating flux derivatives wrt SN parameters| | ||
| |MbCov|class|estimating covariance matrix with mb| | ||
| |GetReference|class|loading reference data| | ||
| |Gamma|class|estimating gamma parameters vs mag and exposure time| | ||
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| ## sn_visu.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |SnapNight | class | getting a snapshot of the (RA, Dec) pointings observed per night' | ||
| |CadenceMovie| class |displaying obs footprint vs time| | ||
| |fieldType | function|estimating the type of field (DD or WFD) according to the number of exposures| | ||
| |area | function|estimating area of a set of polygons (without overlap)| | ||
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| ## sn_calcFast.py ## | ||
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| |name | type | task| | ||
| |----|----|----| | ||
| |LCfast | class | simulating supernovae light curves in a fast way| | ||
| |CalcSN|class|estimating SN parameters from light curve| | ||
| |CalcSN_df|class|estimate SN parameters from light curve| | ||
| |CovColor | class | estimating CovColor from lc using Fisher matrix element| | ||
| |sigmaSNparams|function| estimating SN parameter errors from Fisher elements| | ||
| |faster_inverse | function | inverting a matrix in a fast way| |