GRB 220608A
GCN Circular 32178
Subject
GRB 220608A: Fermi GBM Final Real-time Localization
Date
2022-06-08T05:14:06Z (3 years ago)
From
Fermi GBM Team at MSFC/Fermi-GBM <do_not_reply@GIOC.nsstc.nasa.gov>
The Fermi GBM team reports the detection of a likely LONG GRB
At 05:03:44 UT on 8 Jun 2022, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 220608A (trigger 676357429.750658 / 220608211).
The on-ground calculated location, using the Fermi GBM trigger data, is RA = 229.3, Dec = -0.2 (J2000 degrees, equivalent to J2000 15h 17m, 0d 12'), with a statistical uncertainty of 1.2 degrees.
The angle from the Fermi LAT boresight is 86.0 degrees.
The skymap can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2022/bn220608211/quicklook/glg_skymap_all_bn220608211.png
The HEALPix FITS file, including the estimated localization systematic, can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2022/bn220608211/quicklook/glg_healpix_all_bn220608211.fit
The GBM light curve can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2022/bn220608211/quicklook/glg_lc_medres34_bn220608211.gif
GCN Circular 32179
Subject
Fermi GRB 220608A: Global MASTER-Net observations report
Date
2022-06-08T05:30:24Z (3 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov@xray.sai.msu.ru>
V. Lipunov, V.Kornilov, E.Gorbovskoy, K.Zhirkov, N.Tyurina, P.Balanutsa, A.Kuznetsov, D. Vlasenko,
G.Antipov, D.Zimnukhov, V.Senik, E.Minkina, A.Chasovnikov, V.Topolev, D.Kuvshinov, D.Cheryasov, Ya.Kechin
(Lomonosov Moscow State University, SAI, Physics Department),
R. Podesta, C.Lopez, F. Podesta, C.Francile
(Observatorio Astronomico Felix Aguilar OAFA),
R. Rebolo, M. Serra
(The Instituto de Astrofisica de Canarias),
D. Buckley
(South African Astronomical Observatory),
O.A. Gres, N.M. Budnev
(Irkutsk State University, API),
L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez, A.R.Corella, L.H.Rodriguez
(INAOE, Guillermo Haro Astrophysics Observatory),
A. Tlatov, D. Dormidontov
(Kislovodsk Solar Station of the Pulkovo Observatory),
A. Gabovich, V.Yurkov
(Blagoveschensk Educational State University)
MASTER-OAGH robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in Mexico (OAGH National Institute for Astrophysics, Optics and Electronics) started inspect of the Fermi GRB 220608A ( Fermi GBM team, GCN 32178) errorbox 40 sec after notice time and 78 sec after trigger time at 2022-06-08 05:05:03 UT, with upper limit up to 18.1 mag. The observations began at zenith distance = 31 deg. The sun altitude is -27.5 deg.
The galactic latitude b = 45 deg., longitude l = 1 deg.
Real time updated cover map and OT discovered available here:
https://master.sai.msu.ru/site/master2/observ.php?id=1999930
We obtain a following upper limits.
Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment
_________|_____________________|_____________________|____________________________________|_____|_______|_______|________
89 | 2022-06-08 05:05:03 | MASTER-OAGH | (15h 18m 06.15s , +00d 12m 39.1s) | C | 20 | 18.1 |
89 | 2022-06-08 05:05:03 | MASTER-OAGH | (15h 17m 57.32s , +00d 36m 54.2s) | C | 20 | 17.3 |
130 | 2022-06-08 05:05:44 | MASTER-OAGH | (15h 17m 52.23s , +00d 36m 07.2s) | C | 20 | 16.4 |
130 | 2022-06-08 05:05:44 | MASTER-OAGH | (15h 18m 01.03s , +00d 11m 39.2s) | C | 20 | 17.6 |
176 | 2022-06-08 05:06:25 | MASTER-OAGH | (15h 17m 58.38s , +00d 35m 46.9s) | C | 30 | 15.6 |
176 | 2022-06-08 05:06:25 | MASTER-OAGH | (15h 18m 07.14s , +00d 11m 45.8s) | C | 30 | 17.2 |
232 | 2022-06-08 05:07:16 | MASTER-OAGH | (15h 17m 55.44s , +00d 38m 26.1s) | C | 40 | 14.8 |
232 | 2022-06-08 05:07:16 | MASTER-OAGH | (15h 18m 04.16s , +00d 13m 41.8s) | C | 40 | 16.8 |
298 | 2022-06-08 05:08:17 | MASTER-OAGH | (15h 17m 55.37s , +00d 36m 37.7s) | C | 50 | 15.3 |
298 | 2022-06-08 05:08:17 | MASTER-OAGH | (15h 18m 04.07s , +00d 11m 56.5s) | C | 50 | 17.3 |
379 | 2022-06-08 05:09:28 | MASTER-OAGH | (15h 17m 58.24s , +00d 38m 23.5s) | C | 70 | 14.9 |
379 | 2022-06-08 05:09:28 | MASTER-OAGH | (15h 18m 06.90s , +00d 13m 38.7s) | C | 70 | 17.3 |
465 | 2022-06-08 05:11:00 | MASTER-OAGH | (15h 08m 20.46s , +01d 14m 14.4s) | C | 60 | 15.3 |
465 | 2022-06-08 05:11:00 | MASTER-OAGH | (15h 08m 28.99s , +00d 49m 33.2s) | C | 60 | 17.0 |
804 | 2022-06-08 05:15:53 | MASTER-OAGH | (15h 17m 10.99s , -00d 11m 35.4s) | C | 150 | 16.2 |
804 | 2022-06-08 05:15:53 | MASTER-OAGH | (15h 17m 19.75s , -00d 35m 47.3s) | C | 150 | 17.6 |
990 | 2022-06-08 05:18:44 | MASTER-OAGH | (15h 17m 17.07s , -00d 10m 35.4s) | C | 180 | 15.7 |
990 | 2022-06-08 05:18:44 | MASTER-OAGH | (15h 17m 25.80s , -00d 35m 21.6s) | C | 180 | 17.4 |
1191 | 2022-06-08 05:22:06 | MASTER-OAGH | (15h 17m 14.38s , -00d 10m 51.0s) | C | 180 | 16.1 |
1191 | 2022-06-08 05:22:06 | MASTER-OAGH | (15h 17m 22.89s , -00d 34m 13.3s) | C | 180 | 17.6 |
Filter C is a clear (unfiltred) band.
The observation and reduction will continue.
The message may be cited.
GCN Circular 32183
Subject
GRB 220608A: AstroSat CZTI detection
Date
2022-06-09T03:23:52Z (3 years ago)
From
Gaurav Waratkar at IIT,Bombay <gauravwaratkar@iitb.ac.in>
R. Gopalakrishnan (IUCAA), V. Prasad (IUCAA), G. Waratkar (IITB), A.
Vibhute (IUCAA), V. Bhalerao (IITB), D. Bhattacharya (Ashoka
University/IUCAA), A. R. Rao (IUCAA/TIFR), and S. Vadawale (PRL) report
on behalf of the AstroSat CZTI collaboration:
Analysis of AstroSat CZTI data with the CIFT framework (Sharma et al.,
2021, JApA, 42, 73) showed detection of a long GRB 220608A which was
also reported by Fermi GBM (GCN 32178).
The source was clearly detected in the 20-200 keV energy range. The
light curve showed multiple peaks of emission with the strongest peak at
2022-06-08 05:03:45.50 UTC. The measured peak count rate associated with
the burst is 294 (+43, -35) counts/s above the background in the
combined data of three quadrants, with a total of 2720 (+389, -365)
counts. The local mean background count rate was 393 (+1, -2) counts/s.
Using cumulative rates, we measure a T90 of 36 (+11, -3) s.
It was also clearly detected in the CsI anticoincidence (Veto) detector
in the 100-500 keV energy range. The light curve showed multiple peaks
of emission with the strongest peak at 2022-06-08 05:03:44.45 UTC. The
measured peak count rate is 483 (+71, -70) counts/s above the background
in the combined Veto data of four quadrants, with a total of 4040 (+617,
-645) counts. The local mean background count rate was 1621 (+4, -4)
counts/s. We measure a T90 of 36 (+5, -10) s from the cumulative Veto
light curve.
CZTI GRB detections are reported regularly on the payload site at
http://astrosat.iucaa.in/czti/?q=grb. CZTI is built by a TIFR-led
consortium of institutes across India, including VSSC, URSC, IUCAA, SAC,
and PRL. The Indian Space Research Organisation funded, managed, and
facilitated the project.