JusflPyRoot
a library to ease the life with powerfull python numpy and powerfull ROOT classes.
in progress, very early stage
Installation
Use uv{.verbatim} from astral to handle the environment.
uv tool install jusflpyroot
# OR classically
pip install jusflpyroot
Use examples
Basic histo creation, save, load
Self-explanatory, create TH1F, induce NumpyTH1, save, destoy, repeat, etc...
if __name__ == "__main__":
NumpyTH1.list_file("bobes.root") # list the file content if exists
# create one ROOT histogram
h = ROOT.TH1F("namea", "histogram that goes to file", 100, 0, 100)
print("i... filling-in with a binary pattern to distinguish under/ovrflow and the content")
h.Fill(- 1 ) # underflow
h.Fill(0, 2) # 2x inside
h.Fill(100 - 0.0001, 4) # 4x inside
h.Fill(100 , 8) # 8x overflow
# create THE OBJECT
nh = NumpyTH1.from_th1(h)
nh.save("bobes.root", save_format="root")
nh.force_del() # brutally remove the object from instances
# once more, but empty, I dont care about 'h'
h = ROOT.TH1F("nameb", "histogram that also goes to file", 100, 0, 100)
nh = NumpyTH1.from_th1(h)
nh.save("bobes.root", save_format="root")
nh.force_del()
# last time, but dont delete this time
h = ROOT.TH1F("namec", "histogram just here", 100, 0, 100)
nh = NumpyTH1.from_th1(h)
nh2 = NumpyTH1.load("bobes.root", "namea", load_format="root")
print(" ... _______ I expect to see 'namec' (still in memory) and 'namea' from disk")
NumpyTH1.list()
print(" ... _______ on disk:")
NumpyTH1.list_file("bobes.root")
# get three vectors for the model Fit
x, y, dy = nh.get_xy()
The output should look like this:
i... filling-in with a binary pattern to distinguish under/ovrflow and the content
i... saving histo 'namea' into 'bobes.root'
D... deleting histo 'namea' #instances 1 => 0
i... saving histo 'nameb' into 'bobes.root'
D... deleting histo 'nameb' #instances 1 => 0
i... loading 'namea' from bobes.root
i... there is 2 histograms total in the file
... _______ I expect to see 'namec' (still in memory) and 'namea' from disk
0. namec 'histogram just here ' 2025-07-09 14:21:17.876 100 <0.0 - 100.0) [ 0.0 / 0.0 / 0.0 ]
1. namea 'histogram that goes to file ' 2025-07-09 14:21:17.876 100 <0.0 - 100.0) [ 1.0 / 6.0 / 8.0 ]
... _______ on disk:
f... ... namea (TH1 in bobes.root)
f... ... nameb (TH1 in bobes.root)
Minuit fit
h = ROOT.TH1F("namec", "histogram just here", 10, 0, 10)
for i in range(10): # for range(11) .... 10 will already go to overflows
h.Fill(i, i)
for i in range(10): # make some mess
h.Fill(2)
h.Fill(3)
h.Fill(4)
h.Fill(5)
NumpyTH1.by_name("namec").Draw("numpy") # Draw using matplotlib
print("... ========================= fitting ==========================")
x, y, dy = nh.get_xy() # Get data for fit (from histogram)
print(x)
print(y)
print(dy)
Fitter = PrepareLSQFit(x, y, dy ) # provide data to FITTER
Fitter.set_model("p2") # select mode name and function
Fitter.FIT( a= -0.1, b=1, c=1) # initial values + constant names; par names must match
Fitter.conclude() # prints and plots using matplotlib
# NumpyTH1.wait_loop() # not needed with matplotlib plt
Delete all
Delete all instances, reset colors. Can be useful in emacs codeblocks.
print("i... LIST")
NumpyTH1.list()
print("X... DELETING ALL")
NumpyTH1.reset_all()
print("X... DELETED")
print("i... LIST EMPTY - START")
NumpyTH1.list()
print("i... LIST EMPTY - END")
Thoughts on development
[TODO]{.todo .TODO} External models {#external-models}
- model
name... whatever name is ok - and MODEL ... now it is like
def P0(self, a):
model_points = np.zeros_like(self.cx) + a
if self.switch_xi2_output:
return self.XI2(model_points)
return model_points
- But an external model needs more than just
switch_xi2_output{.verbatim} (to be able to conclude - and the summary is very important). - My ODE needed:
- constants defined for the actual situation
- parameter
xs1that is varied but had to be global for different steps - parameter
normthat was simply just byXi2*norm - X0 field that keeps per partes calculation data
-
Class for an external model
It seems that a dedicated class would be a solution for an external mode.
- init and/or reset all steps
- set the array of
x{.verbatim} points where the model is evaluatedset_x_points(x){.verbatim} - evaluate Xi2 given the parameters:
evaluate_Xi2(a=1,b=2){.verbatim} - provide the calculated points:
calculate_points(a=1,b=2){.verbatim}
class MyModel: "The most basic model we can have" cx=np.array([]) params={} # container for parameters model_name="mymodel" def __init__(self): # initial parameters self.params['a'] = 1 self.params['b'] = 1 return def set_x_points(self,x): "Set X pointes, where the model calculates y values" self.cx=np.array(x) return def MODEL(self,xx): "Model here... whatever calculation, parameters are set globaly-in-the-class" y=xx*self.params['a'] + self.params['b'] return y def calculate_points(self,a=1,b=1): "MAIN CALLed FUNCTION... set the parameters and call MODEL on xx" if len(cx)==0:return None self.params['a']=a self.params['b']=b # Save The parameters to the instance y=self.MODEL(self.cx) return y # ---------- other ideas ---------------- def guess_init_parameters_from_y(self,y): if len(cx)==0:return None self.params['a']=1 self.params['a']=1 return par_dict
How to call it?
A=MyModel() A.set_x_points(x) # Fitter = PrepareLSQFit(x, y, dy ) # provide data to FITTER Fitter.set_model_name("mm", set_model=False) Fitter.set_ext_model( A.calculate_points ) # but I need only the function y=f(x) Fitter.FIT( a= -0.1, b=1 ) # paramater names must match Fitter.conclude()
Metadata
Release files for jusflpyroot 0.1.12
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| File | Size | Uploaded | Provenance | Actions |
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Built distribution (wheel)
| File | Interpreter | ABI | Platform | Actions Reset |
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| jusflpyroot-0.1.12-py3-none-any.whl | Python 3 | none | any | Details for jusflpyroot-0.1.12-py3-none-any.whl |
Total release size: 66.5 kB
Release files / jusflpyroot-0.1.12.tar.gz
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