SDFITS Loaders
Motivation
Although the initial design will be for GBT data, a goal is for dysh to be easily modifiable for any single-dish radio telescope. Thus came the idea of an SDFITS loader which would standardize inputs.
ScanBlock
Here’s the class diagram for an ScanBlock and its derived classes.
classDiagram
class ScanBlock{
metadata
spectra
summary()
calibrate()
baseline()
timeaverage()
polaverage()
finalspectrum()
undo()
}
class PSScan{
metadata
spectra
}
class FSScan{
metadata
spectra
fold()
}
class SubBeamNodScan{
metadata
spectra
}
class OTFScan{
metadata
spectra
}
ScanBlock <|-- PSScan
ScanBlock <|-- FSScan
ScanBlock <|-- NodScan
ScanBlock <|-- OTFScan
That’s probably not super accurate. I just copied the diagram in the stakeholder presentation from last May.
SDFITSLoad
classDiagram
class SDFITSLoad{
_filename
_bintable
_index
_binheader
_data
_hdu
_header
__len__()
__repr__()
_bintable_from_rows()
_loadlists()
_summary()
info()
bintable()
binheader()
filename()
index()
reset()
create_index()
load()
fix_meta()
velocity_convention()
udata()
ushow()
naxis()
nintegrations()
rawspectra()
rawspectrum()
getrow()
getspec()
nrows()
nchan()
npol()
sources()
scans()
summary()
write()
}
GBTFITSLoad
classDiagram
class SDFITSLoad{
method()
}
class GBTFITSLoad{
method()
}
SDFITSLoad <|-- GBTFITSLoad