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Cosmetics.
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docs/source/berenice.rst

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*From Βερενíκη, Ancient Macedonian form of the Attic Greek, Φερενíκη: she, who brings victory.*
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This city produces the spectrum of dark noise of the SiPMs. This is achieved by binning either the :math:`pe` or ``ADC`` content of each raw WF sample. Some slices will have only electronic noise while others will contain one or more dark counts. The resulting spectra give a representation of the SiPM charge in the absence of external light above detector ambient conditions.
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This city produces the spectrum of dark noise of the SiPMs. This is achieved by binning either the :math:`pe` or :math:`ADC` content of each raw WF sample. Some slices will have only electronic noise while others will contain one or more dark counts. The resulting spectra give a representation of the SiPM charge in the absence of external light above detector ambient conditions.
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.. _Berenice input:
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* ``/Run/events``:list of the ``evt_number`` and the correspondent ``timestamp``.
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* ``/Run/runInfo``: stores the ``run_number``.
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* ``/RD/sipmrwf``: stores the raw waveform itself. It indicates the number of ``ADCs`` per time bin for each event and SiPM.
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* ``/RD/sipmrwf``: stores the raw waveform itself. It indicates the number of :math:`ADCs` per time bin for each event and SiPM.
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.. _Berenice output:
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Output
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------
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* ``HIST/median``: histogram values of the dark spectrum when the baseline substraction has been performed with the median of the waveform along with the ``ADCs`` to ``pes`` conversion (calibration).
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* ``HIST/median``: histogram values of the dark spectrum when the baseline substraction has been performed with the median of the waveform along with the :math:`ADCs` to :math:`pes` conversion (calibration).
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* ``HIST/median_bins``: bin values of the dark spectrum ``HIST/median``.
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* ``HIST/mode``: histogram values of the dark spectrum when the baseline substraction has been performed with the mode of the waveform along with the ``ADCs`` to ``pes`` conversion (calibration).
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* ``HIST/mode``: histogram values of the dark spectrum when the baseline substraction has been performed with the mode of the waveform along with the :math:`ADCs` to :math:`pes` conversion (calibration).
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* ``HIST/mode_bins``: bin values of the dark spectrum ``HIST/mode``.
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* ``HIST/adc``: histogram values of the dark spectrum when the baseline substraction has been performed with the mode of the waveform and no calibration.
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* ``HIST/adc_bins``: bin values of the dark spectrum ``HIST/adc_bins``.
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* - ``min|max_bin``
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- ``float``
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- Lower/upper limit of the number of ``ADCs`` of the waveform to be considered for the spectrum.
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- Lower/upper limit of the number of :math:`ADCs`` of the waveform to be considered for the spectrum.
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* - ``bin_width``
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- ``int``
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Waveform calibration
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In this step, the waveform in ``ADCs`` in converted to photoelectrons (``pes``). For this, the gains are loaded from the NEXT database.
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In this step, the waveform in :math:`ADCs`` in converted to photoelectrons (:math:`pes`). For this, the gains are loaded from the NEXT database.
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This step is optional when subtracting the baseline the using the mode of the waveform.
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Histogram the result
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For each slice performed on the waveform in the previous section, it sums all the ``ADCs`` in each slice and adds an entry to the histogram. It repeats this for each waveform of the same sensor.
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For each slice performed on the waveform in the previous section, it sums all the :math:`ADCs`` in each slice and adds an entry to the histogram. It repeats this for each waveform of the same sensor.

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