Core package to analyze gravitational-wave data, find signals, and study their parameters. This package was used in the first direct detection of gravitational waves (GW150914), and is used in the ongoing analysis of LIGO/Virgo data.
This is a new feature that propagates slide_id information across some PyGRB's plotting scripts. In particular it implements a new way of displaying triggers from a specific slide_id.
Currently some PyGRB plots are overpopulated with the addition of timeslides in recent runs. For example, the following plot shows the background triggers obtained from zerlolag data + all timeslides (blue crosses), and just zerolag data, i.e. slide_id=0 (black crosses) around GW170817
Standard information about the request
This is a new feature that propagates slide_id information across some PyGRB's plotting scripts. In particular it implements a new way of displaying triggers from a specific slide_id.
Currently some PyGRB plots are overpopulated with the addition of timeslides in recent runs. For example, the following plot shows the background triggers obtained from zerlolag data + all timeslides (blue crosses), and just zerolag data, i.e.
slide_id=0(black crosses) around GW170817This change affects: PyGRB
pycbc/bin/pycbc_pygrb_plot_snr_timeseries
pycbc/bin/pycbc_pygrb_plot_coh_ifo_snr
pycbc/bin/pycbc_pygrb_plot_null_stats
pycbc/bin/pycbc_pygrb_plot_chisq_veto
pycbc/results/pygrb_plotting_utils.py
pycbc/results/pygrb_postprocessing_utils.py