Open Access

Table 1

Transient γ-ray signals obtained from the performed VSSTW analysis.

Identifier RA (deg) Dec (deg) #Slice/# interval Length (6 h) Local. signif. (σ) Global signif. (σ) Assoc. source Class
FST 080915 119.9 −57.9 1/169 1 17.0 >5 GRB 080916C GRB
FST 090322 190.8 17.4 2/322 1 6.9 3.4 GRB 090323 GRB
FST 090328 90.9 −42.1 2/343 2 10.7 >5 GRB 090328 GRB
FST 090509 333.6 −26.7 2/514 1 18.6 >5 GRB 090510A GRB
FST 090902 264.1 27.4 2/976 1 9.0 >5 GRB 090902B GRB
FST 090926 353.5 −66.4 2/1071 1 17.3 >5 GRB 090926A GRB
FST 091003 251.3 36.7 2/1099 1 6.9 3.4 GRB 091003 GRB
FST 100310 315.5 46.0 3/233 4 7.9 >5 V407 Cygni nova
FST 100413 192.2 8.4 3/370 1 7.8 4.9 GRB 100414A GRB
FST 110307 347.9 −5.4 4/180 3 10.7 >5 FLSF 2011-03-07 solar flare
FST 110416 83.5 21.9 4/338 4 21.8 >5 Crab flare pwn
FST 110906 165.4 6.3 4/914 1 10.9 >5 FLSF 2011-09-06 solar flare
FST 120306 347.7 −5.1 5/142 3 54.6 >5 FLSF 2012-03-07 solar flare
FST 120624 170.9 8.8 5/582 1 7.6 4.6 GRB 120624B GRB
FST 120707 105.9 22.7 5/629.5 4 7.0 3.7 FLSF 2012-07-06 solar flare
FST 120710 94.3 −70.8 5/646 1 7.1 3.8 GRB 120711A GRB
FST 130327 218.1 −69.9 6/183 1 10.3 >5 GRB 130327B GRB
FST 130427 173.0 27.5 6/307 1 30.9 >5 GRB 130427A GRB
FST 130821 314.3 −11.7 6/773 1 6.8 3.2 GRB 130821A GRB
FST 131011 196.4 −7.2 6/975 1 15.3 >5 FLSF 2013-10-11 solar flare
FST 131231 10.8 −1.8 6/1299 1 10.8 >5 GRB 131231A GRB
FST 140206 315.4 −8.6 6/1447 1 10.4 >5 GRB 140206B GRB
FST 140224 338.4 −9.1 7/22 1 42.1 >5 FLSF 2014-02-25 solar flare
FST 140810 119.1 27.8 7/689 2 7.6 4.6 GRB 140810A GRB
FST 140901 160.6 8.0 7/776 1 23.7 >5 FLSF 2014-09-01 solar flare
FST 140928 44.3 −55.7 7/884 1 6.8 3.2 GRB 140928A GRB
FST 141207 160.0 3.7 7/1165 1 8.3 >5 GRB 141207A GRB
FST 150523 115.2 −45.6 8/331 1 7.3 4.1 GRB 150523A GRB
FST 150527 117.3 −51.4 8/471 1 10.7 >5 GRB 150627A GRB
FST 160509 310.9 76.3 9/239 3 7.2 4.0 GRB 160509A GRB
FST 160623 315.4 42.4 9/419 1 9.1 >5 GRB 160623A GRB
FST 160625 308.8 6.8 9/430 1 14.5 >5 GRB 160625B GRB
FST 160821 171.2 42.3 9/657 1 7.9 >5 GRB 160821A GRB
FST 161107 275.0 −28.3 9/970 4 8.0 >5 V5856 Sgr nova
FST 170214 256.0 −2.1 9/1364 1 10.2 >5 GRB 170214A GRB
FST 170915 203.9 −46.8 10/678 1 8.8 >5 GRB 170906A GRB
FST 170910 168.9 5.0 10/697 1 52.3 >5 FLSF 2017-09-10 solar flare
FST 171010 66.6 −10.3 10/817 1 8.0 >5 GRB 171010A GRB
FST 171117 194.7 −63.8 10/962 1 8.2 >5 PSR B1259-63 γ-ray binary
FST 180112 43.8 76.5 10/1193 1 7.1 3.8 new GRB candidate
FST 180210 1.9 18.2 10/1308 1 7.7 4.8 GRB 180210A GRB
FST 180414 158.8 −59.7 11/59 4 14.3 >5 V906 Carinae nova
FST 180720 0.1 −2.7 11/448 1 7.7 4.8 GRB 180720B GRB
FST 181225 347.9 −9.9 11/1079.5 1 7.0 3.7 GRB 181225A GRB
FST 200713 59.5 −54.4 13/346 4 7.9 >5 YZ Reticuli nova
FST 210809 267.4 −6.7 14/412 4 19.1 >5 RS Ophiuchi nova
FST 211023 73.2 85.1 14/712 1 7.3 4.1 GRB 211023A GRB
FST 220408 92.7 −50.9 14/1379 1 8.2 >5 GRB 220408B GRB
FST 221017 156.8 15.9 15/161 1 8.9 >5 GRB 220617A GRB
FST 220627 201.0 −32.7 15/201 1 7.5 4.5 GRB 220627A GRB
FST 221009 288.5 19.8 15/616 3 14.6 >5 GRB 221009A GRB
FST 221023 230.3 15.0 15/673 1 24.9 >5 GRB 221023A GRB
FST 230812 248.9 47.7 16/344 1 9.0 >5 GRB 230812B GRB
FST 231231 280.9 −23.2 16/908 2 7.7 4.8 new solar flare

Notes. The second and third columns show the right ascension and the declination of a transient γ-ray source. The fourth and fifth columns show the start date and the length of a high-γ-ray-flux state. The six and seventh columns show the local and global significances at which the high flux state is detected. The eighth and ninth columns show the name and class of a γ-ray source associated with a transient signal.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.