2020-01-14T02:13:47 LIGO Scientific Collaboration and Virgo Collaboration The Notice Type number is assigned/used within GCN, eg type=150 is an LVC_PRELIMINARY notice Indicates whether this event should be distributed to LSC/Virgo members only A number that increments by 1 each time a new revision is issued for this event Identifier in GraceDB VOEvent alert type Indicates that this event is a hardware injection if 1, no if 0 Indicates that this event is an open alert if 1, no if 0 Web page for evolving status of this GW candidate List of instruments used in analysis to identify this event False alarm rate for GW candidates with this strength or greater Data analysis working group Low-latency data analysis pipeline Specific low-latency search Sky Map FITS Central frequency of GW burst signal Measured duration of GW burst signal Estimated fluence of GW burst signal Source classification: binary neutron star (BNS), neutron star-black hole (NSBH), binary black hole (BBH), MassGap, or terrestrial (noise) Qualitative properties of the source, conditioned on the assumption that the signal is an astrophysical compact binary merger Report of a candidate gravitational wave event Candidate gravitational wave event identified by low-latency analysis V1: Virgo 3 km gravitational wave detector H1: LIGO Hanford 4 km gravitational wave detector L1: LIGO Livingston 4 km gravitational wave detector 2020-01-14T02:18:55 LIGO Scientific Collaboration and Virgo Collaboration The Notice Type number is assigned/used within GCN, eg type=150 is an LVC_PRELIMINARY notice Indicates whether this event should be distributed to LSC/Virgo members only A number that increments by 1 each time a new revision is issued for this event Identifier in GraceDB VOEvent alert type Indicates that this event is a hardware injection if 1, no if 0 Indicates that this event is an open alert if 1, no if 0 Web page for evolving status of this GW candidate List of instruments used in analysis to identify this event False alarm rate for GW candidates with this strength or greater Data analysis working group Low-latency data analysis pipeline Specific low-latency search Sky Map FITS Central frequency of GW burst signal Measured duration of GW burst signal Estimated fluence of GW burst signal Source classification: binary neutron star (BNS), neutron star-black hole (NSBH), binary black hole (BBH), MassGap, or terrestrial (noise) Qualitative properties of the source, conditioned on the assumption that the signal is an astrophysical compact binary merger Report of a candidate gravitational wave event Candidate gravitational wave event identified by low-latency analysis V1: Virgo 3 km gravitational wave detector H1: LIGO Hanford 4 km gravitational wave detector L1: LIGO Livingston 4 km gravitational wave detector ivo://gwnet/LVC#S200114f-1-Preliminary Initial localization is now available (preliminary) 2020-01-14T02:48:21 LIGO Scientific Collaboration and Virgo Collaboration The Notice Type number is assigned/used within GCN, eg type=151 is an LVC_INITIAL notice Indicates whether this event should be distributed to LSC/Virgo members only A number that increments by 1 each time a new revision is issued for this event Identifier in GraceDB VOEvent alert type Indicates that this event is a hardware injection if 1, no if 0 Indicates that this event is an open alert if 1, no if 0 Web page for evolving status of this GW candidate List of instruments used in analysis to identify this event False alarm rate for GW candidates with this strength or greater Data analysis working group Low-latency data analysis pipeline Specific low-latency search Sky Map FITS Central frequency of GW burst signal Measured duration of GW burst signal Estimated fluence of GW burst signal Source classification: binary neutron star (BNS), neutron star-black hole (NSBH), binary black hole (BBH), MassGap, or terrestrial (noise) Qualitative properties of the source, conditioned on the assumption that the signal is an astrophysical compact binary merger Report of a candidate gravitational wave event Candidate gravitational wave event identified by low-latency analysis V1: Virgo 3 km gravitational wave detector H1: LIGO Hanford 4 km gravitational wave detector L1: LIGO Livingston 4 km gravitational wave detector ivo://gwnet/LVC#S200114f-2-Preliminary ivo://gwnet/LVC#S200114f-1-Preliminary Initial localization is now available