GRB 220512A
GCN Circular 32025
Subject
GRB 220512A: Fermi GBM Final Real-time Localization
Date
2022-05-12T05:14:12Z (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 05:03:55 UT on 12 May 2022, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 220512A (trigger 674024640.16888 / 220512211).
The on-ground calculated location, using the Fermi GBM trigger data, is RA = 128.6, Dec = 84.0 (J2000 degrees, equivalent to J2000 08h 34m, 84d 00'), with a statistical uncertainty of 1.7 degrees.
The angle from the Fermi LAT boresight is 118.0 degrees.
The skymap can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2022/bn220512211/quicklook/glg_skymap_all_bn220512211.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/bn220512211/quicklook/glg_healpix_all_bn220512211.fit
The GBM light curve can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2022/bn220512211/quicklook/glg_lc_medres34_bn220512211.gif
GCN Circular 32026
Subject
Fermi GRB 220512A: Global MASTER-Net observations report
Date
2022-05-12T05:30:34Z (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 220512A ( Fermi GBM team, GCN 32025) errorbox 470 sec after notice time and 509 sec after trigger time at 2022-05-12 05:12:24 UT, with upper limit up to 19.2 mag. The observations began at zenith distance = 55 deg. The sun altitude is -32.8 deg.
The galactic latitude b = 30 deg., longitude l = 129 deg.
Real time updated cover map and OT discovered available here:
https://master.sai.msu.ru/site/master2/observ.php?id=1970452
We obtain a following upper limits.
Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment
_________|_____________________|_____________________|____________________________________|_____|_______|_______|________
540 | 2022-05-12 05:12:24 | MASTER-OAGH | (10h 24m 51.71s , +84d 48m 08.6s) | C | 60 | 18.2 |
540 | 2022-05-12 05:12:24 | MASTER-OAGH | (10h 19m 25.52s , +85d 11m 06.3s) | C | 60 | 18.5 |
651 | 2022-05-12 05:13:46 | MASTER-OAGH | (08h 33m 00.84s , +84d 00m 48.6s) | C | 120 | 19.1 |
651 | 2022-05-12 05:13:46 | MASTER-OAGH | (08h 27m 58.70s , +84d 25m 22.4s) | C | 120 | 19.0 |
803 | 2022-05-12 05:16:07 | MASTER-OAGH | (08h 28m 04.69s , +84d 25m 48.8s) | C | 140 | 18.8 |
803 | 2022-05-12 05:16:07 | MASTER-OAGH | (08h 33m 07.25s , +84d 01m 13.8s) | C | 140 | 18.8 |
984 | 2022-05-12 05:18:48 | MASTER-OAGH | (08h 33m 02.46s , +84d 02m 18.4s) | C | 180 | 18.9 |
984 | 2022-05-12 05:18:48 | MASTER-OAGH | (08h 27m 58.84s , +84d 26m 56.3s) | C | 180 | 19.0 |
1185 | 2022-05-12 05:22:10 | MASTER-OAGH | (08h 33m 02.68s , +84d 01m 00.5s) | C | 180 | 19.2 |
1185 | 2022-05-12 05:22:10 | MASTER-OAGH | (08h 27m 59.98s , +84d 25m 41.9s) | C | 180 | 19.2 |
Filter C is a clear (unfiltred) band.
The observation and reduction will continue.
The message may be cited.