Konus-Wind waiting-mode events
The page presents the transients found in the Konus-WIND waiting mode data. The transient events are searched using an automated procedure based on Bayesian block decomposition of the KW waiting mode data (Svinkin et al., in prep.) To date, the database contains ~26 000 events occurred in 1994–2017.
Of them, ~13 000 are soft-spectrum solar X-ray flare candidates and ~13 000 are hard-spectrum transients (including ~4000 triggered events). Using the CGRO-BATSE, BeppoSAX, Swift-BAT, Fermi-GBM, and GOES data, we have found ~6900 previously non-identified events (gamma-ray bursts, soft gamma-repeater bursts, and hard X-ray transient flares).
Below are the links to the tables for each year of the KW observations: Each table contains the following columns:
- UT
- event start determined by Bayesian block decomposition (truncated to integer seconds)
- Dur.
- event duration (truncated to integer seconds)
- Name
- GRB name according to the GCN (https://gcn.gsfc.nasa.gov/), if available
- Type
- event classification (for triggered events)
- Det.
- KW detector(s) where the event is statistically significant: S1 points toward the south ecliptic pole, S2 points toward the north ecliptic pole
- Channels
- energy bands where event is statistically significant: ~20–80 keV (G1), ~80–350 keV (G2), ~350–1200 keV (G3)
- KW
- indicates if the event was detected in the KW triggered mode
- Others
- Other instrument detections: CGRO-BATSE(BAT), BeppoSAX(SAX), Swift-BAT(SWI), Fermi-GBM(FER)
- Comment
- any additional information
The data plot for each event shows count rates in the G1, G2, and G3 energy bands of each detector (red – S1, blue – S2); the Bayesian block decomposition (light red – S1, light blue – S2); the background level estimated for the event (dashed lines).
The current Konus-WIND events observed in the burst and waiting modes: KW event list.
For any questions, comments and suggestions concerning events detected by Konus-Wind in waiting mode please contact Dmitry Svinkin (svinkin@mail·ioffe·ru).
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