TITLE: GCN CIRCULAR
NUMBER: 34923
SUBJECT: GRB 231030B: GRBAlpha detection
DATE: 23/10/31 19:40:44 GMT
FROM: Marianna Dafčíková at Masaryk University <500025(a)mail.muni.cz>
M. Dafcikova, J. Ripa (Masaryk U.), A. Pal (Konkoly Observatory), N. Werner (Masaryk U.), M. Ohno, H. Takahashi (Hiroshima U.), L. Meszaros, B. Csak (Konkoly Observatory), N. Husarikova, F. Munz , M. Topinka, M. Kolar, J.-P. Breuer, F. Hroch (Masaryk U.), T. Urbanec, M. Kasal, A. Povalac (Brno U. of …
[View More]Technology), J. Hudec, J. Kapus, M. Frajt (Spacemanic s.r.o), R. Laszlo, M. Koleda (Needronix s.r.o), M. Smelko, P. Hanak, P. Lipovsky (Technical U. of Kosice), G. Galgoczi (Wigner Research Center/Eotvos U.), Y. Uchida, H. Poon, H. Matake (Hiroshima U.), N. Uchida (ISAS/JAXA), T. Bozoki (Eotvos U.), G. Dalya (Eotvos U.), yyT. Enoto (Kyoto U.), Zs. Frei (Eotvos U.), G. Friss (Eotvos U.), Y. Fukazawa, K. Hirose (Hiroshima U.), S. Hisadomi (Nagoya U.), Y. Ichinohe (Rikkyo U.), K. Kapas (Eotvos U.), L. L. Kiss (Konkoly Observatory), T. Mizuno (Hiroshima U.), K. Nakazawa (Nagoya U.), H. Odaka (Univ of Tokyo), J. Takatsy (Eotvos U.), K. Torigoe (Hiroshima U.), N. Kogiso, M. Yoneyama (Osaka Metropolitan U.), M. Moritaki (U. Tokyo), T. Kano (U. Michigan) -- the GRBAlpha collaboration.
The long-duration GRB 231030B (Fermi/GBM detection: GCN 34915; AstroSat/CZT detection: GCN 34919; INTEGRAL/SPI-ACS peak detection at 2023-10-30 ~19:58:20 UT) was observed by the GRBAlpha 1U CubeSat (Pal et al. 2023, A&A, 677, 40; arXiv:2302.10048).
The detection was confirmed at the peak time 2023-10-30 19:58:21 UTC. The T90 duration measured by GRBAlpha is 21 s and the overall significance during T90 reaches 15 sigma.
The light curve obtained by GRBAlpha is available here:
https://grbalpha.konkoly.hu/static/share/GRB231030B_GCN.pdf
All GRBAlpha detections are listed at: https://monoceros.physics.muni.cz/hea/GRBAlpha/
GRBAlpha, launched on 2021 March 22, is a demonstration mission for a future CubeSat constellation (Werner et al. Proc. SPIE 2018). The detector of GRBAlpha consists of a 75 x 75 x 5 mm3 CsI scintillator read out by a SiPM array, covering the energy range from ~50 keV to ~1000 keV. To increase the duty cycle and the downlink rate, the upgrade of the on-board data acquisition software stack is in progress. The ground segment is also supported by the radio amateur community and it takes advantage of the SatNOGS network for increased data downlink volume.
View this GCN Circular online at https://gcn.nasa.gov/circulars/34923.
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TITLE: GCN CIRCULAR
NUMBER: 34922
SUBJECT: GRB 231028B: VZLUSAT-2 detection
DATE: 23/10/31 19:20:48 GMT
FROM: Marianna Dafčíková at Masaryk University <500025(a)mail.muni.cz>
M. Dafcikova, J. Ripa (Masaryk U.), A. Pal (Konkoly Observatory), N. Werner (Masaryk U.), M. Ohno (Hiroshima U.), L. Meszaros, B. Csak (Konkoly Observatory), H. Takahashi (Hiroshima U.), F. Munz , M. Topinka, F. Hroch, N. Husarikova, J.-P. Breuer (Masaryk U.), J. Hudec, J. Kapus, M. Frajt, M. Rezenov (…
[View More]Spacemanic s.r.o), R. Laszlo (Needronix), G. Galgoczi (Wigner Research Center/Eotvos U.), N. Uchida (ISAS/JAXA), T. Enoto (Kyoto U.), Zs. Frei (Eotvos U.), Y. Fukazawa, K. Hirose, H. Matake (Hiroshima U.), S. Hisadomi (Nagoya U.), Y. Ichinohe (Rikkyo U.), L. L. Kiss (Konkoly Observatory), T. Mizuno (Hiroshima U.), K. Nakazawa (Nagoya U.), H. Odaka (Univ of Tokyo), K. Torigoe (Hiroshima U.), P. Svoboda, V. Daniel, J. Dudas, M. Junas, J. Gromes (VZLU), I. Vertat (FEL ZCU) -- the VZLUSAT-2/GRB payload collaboration.
The long duration GRB 231028B (Fermi/GBM detection: trigger no. 720224759; Konus/WIND detection at 2023-10-28 22:25:55.024 UT) was detected by the GRB detectors on board of the VZLUSAT-2 3U CubeSat (https://www.vzlusat2.cz/en/).
The data acquisition was performed by the GRB detector units no. 0 and no. 1. The detection was confirmed at the peak time 2023-10-28 22:25:58 (22:26:31) UTC. The T90 duration is 43 s (37 s) and the significance during T90 reaches 13 sigma (8 sigma) for detector unit no. 0 (no. 1).
The light curve obtained by VZLUSAT-2 is available here:
https://vzlusat2.konkoly.hu/static/share/GRB231028B_GCN_VZLUSAT2.pdf
All VZLUSAT-2 detections are listed at: https://monoceros.physics.muni.cz/hea/VZLUSAT-2/
The GRB detectors on VZLUSAT-2 are a demonstration payload for a future CubeSat constellation (Werner et al. Proc. SPIE 2018). Two GRB modules of VZLUSAT-2 are placed in a perpendicular manner and each consists of a 75 x 75 x 5 mm3 CsI scintillator read out by a SiPM array, covering the energy range from ~30 keV to ~1000 keV. VZLUSAT-2 was launched on 2022 January 13 from Cape Canaveral.
View this GCN Circular online at https://gcn.nasa.gov/circulars/34922.
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TITLE: GCN CIRCULAR
NUMBER: 34921
SUBJECT: Fermi trigger No 720415645: Global MASTER-Net observations report
DATE: 23/10/31 18:15:51 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru>
V. Lipunov, V.Kornilov, E. Gorbovskoy, K. Zhirkov, N.Tyurina, P.Balanutsa, A.Kuznetsov, V.Senik, D. Vlasenko,
G.Antipov, D.Zimnukhov, E.Minkina, A.Chasovnikov, V.Topolev, D.Kuvshinov, D. Cheryasov, Ya.Kechin, Yu.Tselik, A. Sosnovskij
(Lomonosov Moscow State …
[View More]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. Gress, N.M. Budnev, O.Ershova
(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),
V. Yurkov, A. Gabovich
(Blagoveschensk Educational State University)
MASTER-SAAO robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in South Africa (South African Astronomical Observatory) started inspect of the Fermi GRB231031.14 (trigger No 720415645,10h 20m 52.80s , -77d 30m 36.0s, R=8.59) errorbox 51708 sec after notice time and 51745 sec after trigger time at 2023-10-31 17:49:46 UT, with upper limit up to 15.1 mag. Observations started at twilight. The observations began at zenith distance = 69 deg. The sun altitude is -10.2 deg.
The galactic latitude b = -17 deg., longitude l = 295 deg.
Real time updated cover map and OT discovered available here:
https://master.sai.msu.ru/site/master2/observ.php?id=2293539
We obtain a following upper limits.
Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment
_________|_____________________|_____________________|____________________________________|_____|_______|_______|________
51776 | 2023-10-31 17:49:46 | MASTER-SAAO | (09h 52m 09.44s , -78d 30m 02.3s) | C | 60 | 14.6 |
51866 | 2023-10-31 17:51:16 | MASTER-SAAO | (10h 31m 40.28s , -78d 29m 40.8s) | C | 60 | 13.9 |
52037 | 2023-10-31 17:54:07 | MASTER-SAAO | (10h 08m 57.73s , -76d 36m 12.9s) | C | 60 | 14.6 |
52128 | 2023-10-31 17:55:38 | MASTER-SAAO | (10h 39m 45.58s , -76d 34m 21.4s) | C | 60 | 13.6 |
52208 | 2023-10-31 17:56:58 | MASTER-SAAO | (11h 09m 45.42s , -76d 32m 15.4s) | C | 60 | 14.7 |
52378 | 2023-10-31 17:59:48 | MASTER-SAAO | (10h 45m 55.31s , -74d 40m 47.5s) | C | 60 | 14.4 |
52475 | 2023-10-31 18:01:25 | MASTER-SAAO | (09h 47m 01.87s , -78d 29m 16.3s) | C | 60 | 15.1 |
Filter C is a clear (unfiltred) band.
The observation and reduction will continue.
The message may be cited.
View this GCN Circular online at https://gcn.nasa.gov/circulars/34921.
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TITLE: GCN CIRCULAR
NUMBER: 34920
SUBJECT: GRB 231030B: Fermi GBM Detection
DATE: 23/10/31 14:33:19 GMT
FROM: sumanbala2210(a)gmail.com
S. Bala (USRA) and C. Meegan (UAH) report on behalf of
the Fermi Gamma-ray Burst Monitor Team:
"At 19:58:19.94 UT on 30 October 2023, the Fermi Gamma-ray Burst Monitor (GBM)
triggered and located GRB 231030B (trigger 720388704/231030832).
The Fermi GBM Final Real-time Localization is reported in GCN 34915.
The GBM light curve consists of a single …
[View More]bright peak with a duration (T90)
of about 10.8 s (50-300 keV). The time-averaged spectrum
from T0+0.003 to T0+20.544 s is best fit by
a Band function with Epeak = 240 +/- 20 keV,
alpha = -0.78 +/- 0.04, and beta = -2.02 +/- 0.08.
The event fluence (10-1000 keV) in this time interval is
(2.17 +/- 0.05)E-05 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+1.3 s in the 10-1000 keV band is 24.7 +/- 0.4 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog:
https://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html
For Fermi GBM data and info, please visit the official Fermi GBM Support Page:
https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/"
View this GCN Circular online at https://gcn.nasa.gov/circulars/34920.
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TITLE: GCN CIRCULAR
NUMBER: 34919
SUBJECT: GRB 231030B: AstroSat CZTI detection
DATE: 23/10/31 14:01:12 GMT
FROM: Gaurav Waratkar at IIT Bombay <gauravwaratkar(a)iitb.ac.in>
P. K. Navaneeth (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,…
[View More] 42, 73) showed the detection of a likely long GRB 231030B which was also detected by Fermi-GBM (Fermi GBM Team, GCN Circ. 34915).
The source was clearly detected in the CZT detectors in the 20-200 keV energy range. The light curve peaks at 2023-10-30 19:58:21.25 UTC. The measured peak count rate associated with the burst is 356 (+57, -41) counts/s above the background in the combined data of three quadrants (out of four), with a total of 1131 (+128, -178) counts. The local mean background count rate was 242 (+2, -4) counts/s. Using cumulative rates, we measure a T90 of 6.4 (+2.1, -2.3) s.
The source was also clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range. The light curve peaks at 2023-10-30 19:58:20.73 UTC. The measured peak count rate associated with the burst is 705 (+74, -78) counts/s above the background in the combined data of all quadrants, with a total of 2538 (+365, -401) counts. The local mean background count rate was 1484 (+6, -7) counts/s. We measure a T90 of 7.4 (+3.6, -3.1) s from the cumulative Veto light curve.
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.
CZTI GRB detections are reported regularly on the payload site at:
http://astrosat.iucaa.in/czti/?q=grb
View this GCN Circular online at https://gcn.nasa.gov/circulars/34919.
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TITLE: GCN CIRCULAR
NUMBER: 34917
SUBJECT: IPN triangulation of GRB 231020A
DATE: 23/10/30 20:36:49 GMT
FROM: Dmitry Svinkin at Ioffe Institute <svinkin(a)mail.ioffe.ru>
A.S. Kozyrev, D.V. Golovin, M.L. Litvak, I.G. Mitrofanov, and A.B. Sanin
on behalf of the MGNS/BepiColombo and HEND/Mars Odyssey teams,
J. Benkhoff on behalf of the BepiColombo team,
D. Svinkin, D. Frederiks, A. Ridnaia, A. Lysenko,
and T. Cline on behalf of the Konus-Wind team,
A. Goldstein, M. S. Briggs, C. …
[View More]Wilson-Hodge,
and E. Burns on behalf of the Fermi GBM team,
E. Bozzo and C. Ferrigno, on behalf of the INTEGRAL SPI-ACS GRB team,
S. Barthelmy, J. Cummings, H. Krimm, D. Palmer, and A. Tohuvavohu
on behalf of the Swift-BAT team,
and
W. Boynton, C. Fellows, K. Harshman, H. Enos, R. Starr,
and A.S. Gardner on on behalf of the GRS-Odyssey GRB team,
report:
The long-duration GRB 231020A
(Fermi-GBM detection: The Fermi GBM team, GCN Circ. 34856;
Bala et al., GCN Circ. 34869;
BALROG localization: Preis et al., GCN Circ. 34861;
AstroSat-CZTI detection: Navaneeth et al., GCN Circ. 34880;
GRID detection: Wang and Yang, GCN Circ. 34903)
was detected by Fermi (GBM trigger 719521023), INTEGRAL (SPI-ACS),
Konus-Wind, Swift (BAT), Mars-Odyssey (HEND), BepiColombo (MGNS),
AstroSat (CZTI), and GRID, at about 68218 s UT (18:56:58).
The burst was outside the coded field of view of the BAT.
We have triangulated it to a preliminary, 3 sigma error box
whose coordinates are:
---------------------------------------------
RA(2000), deg Dec(2000), deg
---------------------------------------------
Center:
314.493 (20h 57m 58s) -29.254 (-29d 15' 15")
Corners:
314.061 (20h 56m 15s) -28.067 (-28d 04' 02")
314.696 (20h 58m 47s) -29.893 (-29d 53' 33")
314.881 (20h 59m 31s) -30.286 (-30d 17' 09")
314.275 (20h 57m 06s) -28.562 (-28d 33' 43")
---------------------------------------------
The error box area is 247 sq. arcmin, and its maximum
dimension is 2.3 deg (the minimum one is 2.2 arcmin).
The Sun distance was 101 deg.
This localization may be improved.
The IPN localization is consistent with, but reduces the area of,
the Fermi-GBM final localization.
A triangulation map and HEALPix FITS file are posted at
http://www.ioffe.ru/LEA/GRBs/GRB231020_T68224/IPN
The Konus-Wind time history and spectrum will be given
in a forthcoming GCN Circular.
View this GCN Circular online at https://gcn.nasa.gov/circulars/34917.
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TITLE: GCN CIRCULAR
NUMBER: 34916
SUBJECT: GRB 231030B: BALROG localization (Fermi Trigger 720388704 / GRB 231030832)
DATE: 23/10/30 20:28:59 GMT
FROM: Jochen Greiner at MPE <jcgrog(a)mpe.mpg.de>
T. Preis, B. Biltzinger, J. Burgess & J. Greiner (all MPE Garching) report:
The public trigdat data of the Fermi Gamma-ray Burst Monitor (GBM) trigger
720388704 at 19:58:19 on 30 Oct. 2023 were automatically fitted for spectrum
and sky location with BALROG (Burgess et al. 2018, …
[View More]MNRAS 476, 1427;
Berlato et al. 2019, ApJ 873, 60).
The best-fit position (1 sigma statistical errors) is:
RA(2000.0) = 249.1+/-2.4 deg
Decl.(2000.0) = 63.3+/-0.9 deg
We estimate an additional systematic error of 2 deg.
Further details are available at:
https://grb.mpe.mpg.de/grb/GRB231030832/
The Healpix map can be downloaded from:
https://grb.mpe.mpg.de/grb/GRB231030832/healpix
The location parameters are available as JSON at:
https://grb.mpe.mpg.de/grb/GRB231030832/json
View this GCN Circular online at https://gcn.nasa.gov/circulars/34916.
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TITLE: GCN CIRCULAR
NUMBER: 34914
SUBJECT: GRB 231028A: Swift-BAT refined analysis
DATE: 23/10/30 17:03:43 GMT
FROM: Tyler Parsotan at NASA GSFC <tyler.parsotan(a)nasa.gov>
H. A. Krimm (NSF), S. D. Barthelmy (GSFC),
S. Laha (GSFC/UMBC), A. Y. Lien (U Tampa),
C. B. Markwardt (GSFC), D. M. Palmer (LANL),
T. Parsotan (GSFC/UMBC), T. Sakamoto (AGU),
M. Stamatikos (OSU) (i.e. the Swift-BAT team):
Using the data set from T-240 to T+962 sec from the recent telemetry downlink,
we …
[View More]report further analysis of BAT GRB 231028A (trigger #1193078)
(Williams et al., GCN Circ. 34894). The BAT ground-calculated position is
RA, Dec = 214.016, 20.897 deg which is
RA(J2000) = 14h 16m 03.8s
Dec(J2000) = +20d 53' 47.8"
with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 68%.
The mask-weighted lightcurve shows a broad initial pulse with subsequent
extended emission.
T90 (15-350 keV) is 37.23 +- 0.98 sec (estimated error including systematics).
The time-averaged spectrum from T-6.86 to T+41.95 sec is best fit by a simple
power-law model. The power law index of the time-averaged spectrum is
1.40 +- 0.04. The fluence in the 15-150 keV band is 7.2 +- 0.2 x 10^-06 erg/cm2.
The 1-sec peak photon flux measured from T+1.06 sec in the 15-150 keV band
is 8.6 +- 0.4 ph/cm2/sec. All the quoted errors are at the 90% confidence
level.
The results of the batgrbproduct analysis are available at
http://gcn.gsfc.nasa.gov/notices_s/1193078/BA/
View this GCN Circular online at https://gcn.nasa.gov/circulars/34914.
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