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draft nuv dark monitor. help. #156

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64 changes: 61 additions & 3 deletions cosmo/monitors/data_models.py
Original file line number Diff line number Diff line change
Expand Up @@ -217,12 +217,13 @@ def get_new_data(self):
'YCORR'
],
3: [
'TIME',
'LATITUDE',
'LONGITUDE'
'LONGITUDE',
'DARKRATE'
]

}
# TODO: add gross counts, don't need PHA, lat or long right now

# any special data requests
# TODO: add spt support for temp, sun_lat, sun_long
Expand All @@ -235,7 +236,6 @@ def get_new_data(self):
for program in program_ids:
new_files_source = os.path.join(FILES_SOURCE, program)
subfiles = glob(os.path.join(new_files_source, "*corrtag*"))
# TODO: figure out why this wasn't working with find_files()
files += subfiles

if not files: # No new files
Expand All @@ -247,3 +247,61 @@ def get_new_data(self):
table_request=table_request)

return data_results


class CorrtagDataModel(BaseDataModel):
"""Datamodel for all NUV Dark files."""
files_source = FILES_SOURCE
subdir_pattern = '?????'

def get_new_data(self):
header_request = {
0: ['ROOTNAME'],
1: [
'EXPSTART',
'EXPTIME',
'EXPTYPE',
'DETECTOR'
]
}

table_request = {
1: [
'TIME',
'XCORR',
'YCORR'
],
3: [
'LATITUDE',
'LONGITUDE'
]

}
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# TODO: add gross counts, don't need PHA, lat or long right now

# any special data requests
# TODO: add spt support for temp, sun_lat, sun_long
# TODO: is this a good place to add solar data scraping in the future?

# this is temporary to find the files from the dark programs until
# we can add the dark files to the monitor_data database
# files = []
# program_ids = ['15776/']
# for program in program_ids:
# new_files_source = os.path.join(FILES_SOURCE, program)
# subfiles = glob(os.path.join(new_files_source, "*corrtag*"))
# # TODO: figure out why this wasn't working with find_files()
# files += subfiles

files = find_files('*corrtag*', data_dir=self.files_source,
subdir_pattern=self.subdir_pattern)

if not files: # No new files
return pd.DataFrame()

# need to add any other keywords that need to be set
data_results = data_from_exposures(files,
header_request=header_request,
table_request=table_request)

return data_results
37 changes: 28 additions & 9 deletions cosmo/monitors/nuv_dark_monitor.py
Original file line number Diff line number Diff line change
Expand Up @@ -28,24 +28,29 @@ def get_data(self):
# access data, perform any filtering required for analysis
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Suggested change
# access data, perform any filtering required for analysis
"""access data, perform any filtering required for analysis"""

data = self.model.new_data
dark_rate_column = []
dec_year_column = []

xlim = [0, 1024]
ylim = [0, 1024]

# parallelize, this is going to get bad when looking at a lot of data
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for index, row in data.iterrows():
subdf = pd.DataFrame({
"TIME": row["TIME"], "XCORR": row["XCORR"],
"YCORR": row["YCORR"]
"EXPSTART": row["EXPSTART"], "TIME": row["TIME"],
"XCORR": row["XCORR"], "YCORR": row["YCORR"],
"TIME_3": row["TIME_3"]
})
filtered = subdf.where(
(subdf["XCORR"] > xlim[0]) & (subdf["XCORR"] < xlim[1]) & (
subdf["YCORR"] > ylim[0]) & (
subdf["YCORR"] < ylim[1]))
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dark_rate = self.calculate_dark_rate(filtered, xlim, ylim)
dark_rate_column.append(dark_rate)
dark_rate_array, dec_year_array = self.calculate_dark_rate(
filtered, xlim, ylim)
dark_rate_column.append(dark_rate_array)
dec_year_column.append(dec_year_array)

data["DARK_RATE"] = dark_rate_column
data["DECIMAL_YEAR"] = dec_year_column

return data

Expand All @@ -59,19 +64,33 @@ def calculate_dark_rate(self, dataframe, xlim, ylim):

counts = np.histogram(dataframe["TIME"], bins=time_bins)[0]
npix = float((xlim[1] - xlim[0]) * (ylim[1] - ylim[0]))
dark_rate = np.median(counts / npix / timestep)
# what is going on with the whole histogram, ok to use median?

return dark_rate
dark_rate_array = counts / npix / timestep
# save the whole histogram in time bins, and then plot each of them

# make a decimal year array corresponding to the time bins of the
# dark rates
# do this with the expstart (mjd) and time array from the timeline
# extension
mjd_conversion_factor = 1.15741e-5
# taking the expstart, binning the time array by the timestep,
# removing the last element in the array (bin by front edge),
# and then multiplying by the conversion factor
mjd_array = dataframe["EXPSTART"] + dataframe["TIME_3"][::timestep][
:-1] * mjd_conversion_factor
mjd_array = Time(mjd_array, format='mjd')
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dec_year_array = mjd_array.decimalyear

return dark_rate_array, dec_year_array

def track(self):
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The track method should return some sort of quantity (scalar, dataframe, etc), not execute plotting

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yep that is the end goal, don't worry. once the histogram is working correctly it will get the rates from the histogram and return those

# track something. perhaps current dark rate?
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pass

def plot(self):
# do some plots

pass

def store_results(self):
# need to store results if not going in the database
pass
pass