✨Early-Warning Alerts¶
During O3, automated public alerts for CBC events have been sent within as little as 2 minutes after merger. However, some BNS mergers are detectable for up to tens of seconds before merger during the event’s inspiral phase during which the signal sweeps in frequency from tens of hertz to kilohertz across LIGO’s sensitive band.
Since it is generally assumed that detectable electromagnetic (or neutrino) emission starts shortly after merger, a pre-merger gravitational-wave detection would provide early warning of an impending electromagnetic transient and might make it possible for automated follow-up facilities to capture any prompt emission from the merger environment, the jet, and other unknown activity.
We have commissioned an experimental capability to produce and distribute early warning gravitational-wave alerts up to tens of seconds before merger. We have also reduced the latency of ordinary post-merger alerts to within tens of seconds after merger.
We are conducting a trial early warning public alert infrastructure. Since production analysis had to be suspended due to COVID-19 pandemic, we are replaying an 8-day period of saved LIGO data from O3 with a random (and undisclosed) time shift. Starting on 2020-06-09 and lasting for one week, early-warning alerts arising from the replayed data will be publicly distributed as test alerts at a rate of approximately once per day.
Subscribe to Early-Warning Alerts¶
Early warning alerts are publicly distributed as GCN Notices just like ordinary gravitational-wave alerts (see the Alert Contents section). They have exactly the same format and content as a Preliminary GCN Notice. In particular, early warning GCN Notices have significance estimates, sky localizations, and source classifications. Also, like Preliminary GCN Notices, Early Warning GCN Notices are sent prior to vetting by humans, and are not accompanied by a GCN Circular.
Early warning alerts are differentiated from ordinary alerts by the new
LVC_EARLY_WARNING
GCN Notice type. If you are receiving GCN Notices via an
anonymous VOEvent connection and you are using the Python sample code from the
Receiving GCNs section, then all you have to do is add the notice
type to your GCN handler:
import gcn
@gcn.handlers.include_notice_types(
gcn.notice_types.LVC_EARLY_WARNING, # <-- new notice type here
gcn.notice_types.LVC_PRELIMINARY,
gcn.notice_types.LVC_INITIAL,
gcn.notice_types.LVC_UPDATE,
gcn.notice_types.LVC_RETRACTION)
def process_gcn(payload, root):
... # <-- put your code here
gcn.listen(handler=process_gcn)
(If you are using a non-anonymous GCN connection or one of the many other notice formats provided by GCN, then you will also need to submit a change to your GCN Notice subscription settings.)
Important
Since these early-warning events will arise from time-shifted and replayed
data and not live observations, the GCN notices will be flagged as test
events by setting the VOEvent role="test"
attribute.
Detection Method¶
Three CBC search pipelines are participating in early-warning alerts: GstLAL, SPIIR, and MBTA. See the Online Pipelines section for details on these analyses. Localizations will be produced with BAYESTAR; see the Sky Localization and Parameter Estimation section for details.
Note
The following material describes the detection method and simulated observing capabilities with GstLAL, but is also broadly applicable to SPIIR and MBTA.
BNS signals sweep up smoothly in frequency for a few minutes across the Advanced LIGO band. In that time, they may accumulate enough SNR to be detected before merger. A GW170817-like system with a total network SNR of 32 will already accumulate an SNR of 11 by the time the signal sweeps up to 30 Hz, about a minute before merger.
The early warning search is a matched-filter search that uses templates that have been truncated at a selection of end frequencies—or equivalently, cut off at a selection of times before merger. The early warning template bank spans (source frame) component masses between 1 and 2 \(M_\odot\) and chirp masses between 0.9 and 1.7 \(M_\odot\). The end frequencies are 29 Hz, 32 Hz, 38 Hz, 49 Hz, and 56 Hz, corresponding to about 60 s, 45 s, 30 s, 15 s, and 10 s before merger.
Early warning events passing a FAR threshold of one per week are sent as alerts.
Source Classification¶
The automated source classification and properties have not been trained or tested extensively for early warning alerts. However, the early warning analysis is only sensitive to BNS-mass mergers. As a result, the favored source class in early warning GCN Notices will always be either BNS or Terrestrial, with a 0% chance of NSBH or BBH. The HasNS and HasRemnant fields will always show 100%.
Localization¶
Sky localizations for early warning alerts are typically very coarse because the early warning analysis inherently does not make use of the full duration and bandwidth of the gravitational-wave signal. The localization improves slowly up until the last second before merger, and then converges rapidly in the last second.
The animations below show the evolution of early-warning sky maps for three representative events with different SNR values.
Final SNR |
11 |
18 |
25 |
---|---|---|---|
Distance |
250 Mpc |
210 Mpc |
160 Mpc |
Sky map (animated GIF) |
|||
Frequency |
Localization accuracy (90% credible area) |
||
29 Hz |
Not detected |
Not detected |
12000 deg2 |
32 Hz |
10000 deg2 |
||
38 Hz |
9200 deg2 |
8200 deg2 |
|
49 Hz |
2300 deg2 |
1000 deg2 |
730 deg2 |
56 Hz |
1000 deg2 |
700 deg2 |
250 deg2 |
1024 Hz |
10 deg2 |
31 deg2 |
5.4 deg2 |
Detection Rate and Localization Accuracy¶
In the figure below, we show predicted detection rates, distances, and localization uncertainties for simulated BNS events. Of all BNS events detected by LIGO and Virgo, only 5-30% will be amenable for sending early warning alerts. About 5% of all BNS events will be localized to an area of ~400 deg2 by ~30 seconds before merger. At the time of merger, the sky localization will be reduced to about ~1 deg2 for these events. At 60 s before merger, one event per year is expected to be localized to within 400 deg2. At 30 seconds before merger, at least one event per year is expected to be localized to within 40 deg2 and ~4 events per year are expected to be localized to within 400 deg2. By 10 seconds before merger, ~10 events per year are expected to be localized to within 400 deg2.
The figure below shows the cumulative fraction of recovered injections as a function of distance. This figure shows the distance distribution of the events recovered at various early warning frequencies.