TITLE: GCN CIRCULAR
NUMBER: 39434
SUBJECT: EP250223a: Global MASTER-Net observations report
DATE: 25/02/23 18:36:57 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru>
V.Lipunov, E.Gorbovskoy, N.Tiurina, P.Balanutsa, , D.Vlasenko, I.Panchenko,
A.Kuznetsov, G.Antipov, A.Sankovich, A.Sosnovskij, Yu.Tselik, M.Gulyaev, Ya.Kechin,
V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU),
O.Gress, N.Budnev (ISU),
C.Francile, F. Podesta, R.…
[View More]Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA),
A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory),
A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity)
D.Buckley (SAAO),
R.Rebolo (The Instituto de Astrofisica de Canarias),
L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez,
A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory)
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) was pointed to the EP250223a ( EP Team et al., GCN 39429) errorbox 6703 sec after notice time and 11479 sec after trigger time at 2025-02-23 18:15:54 UT, with upper limit up to 18.4 mag. Observations started at twilight. The observations began at zenith distance = 13 deg. The sun altitude is -12.2 deg.
The galactic latitude b = -13 deg., longitude l = 232 deg.
Real time updated cover map and OT discovered available here:
https://master.sai.msu.ru/site/master2/observ.php?id=2788235
We obtain a following upper limits.
Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment
_________|_____________________|_____________________|____________________________________|_____|_______|_______|________
11509 | 2025-02-23 18:15:54 | MASTER-SAAO | (06h 31m 54.68s , -22d 37m 59.1s) | C | 60 | 18.4 |
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/39434.
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TITLE: GCN CIRCULAR
NUMBER: 39433
SUBJECT: GRB 250221A: VLA radio detection
DATE: 25/02/23 18:32:23 GMT
FROM: Roberto Ricci at INAF-IRA <ricci(a)ira.inaf.it>
R. Ricci (U Rome), E. Troja (U Rome) report on behalf of a larger collaboration:
We observed the GRB 250221A discovered by Swift/BAT (Caputo et al. GCN 39396) with
the Very Large Array at the centre frequency of 10 GHz (X-band) with a bandwidth of 4 GHz
at a mid time of 1.95 days after the trigger.
A weak source is …
[View More]detected at the target position with a flux density of 63 +/- 9 microJy.
Further observations are planned to assess its variability.
We thank the VLA staff for promptly executing the observations.
View this GCN Circular online at https://gcn.nasa.gov/circulars/39433.
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TITLE: GCN CIRCULAR
NUMBER: 39432
SUBJECT: Fermi GRB 250223A: Global MASTER-Net observations report
DATE: 25/02/23 18:31:10 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru>
V.Lipunov, E.Gorbovskoy, N.Tiurina, P.Balanutsa, , D.Vlasenko, I.Panchenko,
A.Kuznetsov, G.Antipov, A.Sankovich, A.Sosnovskij, Yu.Tselik, M.Gulyaev, Ya.Kechin,
V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU),
O.Gress, N.Budnev (ISU),
C.Francile, F. Podesta,…
[View More] R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA),
A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory),
A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity)
D.Buckley (SAAO),
R.Rebolo (The Instituto de Astrofisica de Canarias),
L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez,
A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory)
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 GRB 250223A ( Fermi GBM team, GCN 39430) errorbox 6037 sec after notice time and 6071 sec after trigger time at 2025-02-23 18:17:23 UT, with upper limit up to 17.8 mag. Observations started at twilight. The observations began at zenith distance = 81 deg. The sun altitude is -12.4 deg.
The galactic latitude b = -61 deg., longitude l = 358 deg.
Real time updated cover map and OT discovered available here:
https://master.sai.msu.ru/site/master2/observ.php?id=2788279
We obtain a following upper limits.
Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment
_________|_____________________|_____________________|____________________________________|_____|_______|_______|________
6101 | 2025-02-23 18:17:23 | MASTER-SAAO | (21h 30m 33.95s , -55d 53m 54.3s) | C | 60 | 16.5 |
6180 | 2025-02-23 18:18:42 | MASTER-SAAO | (21h 44m 51.61s , -55d 55m 08.8s) | C | 60 | 16.9 |
6260 | 2025-02-23 18:20:01 | MASTER-SAAO | (21h 48m 30.70s , -54d 02m 03.5s) | C | 60 | 16.9 |
6339 | 2025-02-23 18:21:20 | MASTER-SAAO | (22h 02m 01.64s , -54d 00m 54.6s) | C | 60 | 17.2 |
6419 | 2025-02-23 18:22:40 | MASTER-SAAO | (21h 57m 39.63s , -55d 54m 33.4s) | C | 60 | 17.4 |
6498 | 2025-02-23 18:23:59 | MASTER-SAAO | (22h 11m 47.32s , -55d 55m 37.0s) | C | 60 | 17.8 |
6577 | 2025-02-23 18:25:18 | MASTER-SAAO | (22h 06m 14.56s , -52d 07m 28.6s) | C | 60 | 17.5 |
6656 | 2025-02-23 18:26:38 | MASTER-SAAO | (22h 19m 06.47s , -52d 08m 45.6s) | C | 60 | 17.8 |
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/39432.
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TITLE: GCN CIRCULAR
NUMBER: 39431
SUBJECT: Fermi trigger No 762020305: Global MASTER-Net observations report
DATE: 25/02/23 16:46:54 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru>
V.Lipunov, E.Gorbovskoy, N.Tiurina, P.Balanutsa, , D.Vlasenko, I.Panchenko,
A.Kuznetsov, G.Antipov, A.Sankovich, A.Sosnovskij, Yu.Tselik, M.Gulyaev, Ya.Kechin,
V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU),
O.Gress, N.Budnev (ISU),
C.Francile, …
[View More]F. Podesta, R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA),
A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory),
A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity)
D.Buckley (SAAO),
R.Rebolo (The Instituto de Astrofisica de Canarias),
L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez,
A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory)
MASTER-Tunka robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in Russia (Applied Physics Institute, Irkutsk State University) started inspect of the Fermi GRB250223.68 (trigger No 762020305,17h 30m 28.80s , +41d 02m 24.0s, R=5.1) errorbox 569 sec after notice time and 603 sec after trigger time at 2025-02-23 16:28:23 UT, with upper limit up to 16.6 mag. The observations began at zenith distance = 74 deg. The sun altitude is -47.4 deg.
The galactic latitude b = 32 deg., longitude l = 66 deg.
Real time updated cover map and OT discovered available here:
https://master.sai.msu.ru/site/master2/observ.php?id=2788242
We obtain a following upper limits.
Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment
_________|_____________________|_____________________|____________________________________|_____|_______|_______|________
632 | 2025-02-23 16:28:23 | MASTER-Tunka | (17h 31m 26.47s , +40d 50m 52.7s) | C | 55 | 15.9 |
687 | 2025-02-23 16:28:23 | MASTER-Tunka | (17h 31m 26.50s , +40d 50m 52.7s) | C | 165 | 16.5 | Coadd
691 | 2025-02-23 16:29:22 | MASTER-Tunka | (17h 31m 26.58s , +40d 50m 54.0s) | C | 55 | 16.1 |
749 | 2025-02-23 16:30:21 | MASTER-Tunka | (17h 31m 26.76s , +40d 50m 55.4s) | C | 55 | 16.6 |
810 | 2025-02-23 16:31:19 | MASTER-Tunka | (17h 31m 27.02s , +40d 50m 55.5s) | C | 60 | 14.9 |
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/39431.
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TITLE: GCN CIRCULAR
NUMBER: 39429
SUBJECT: EP250223a: Einstein Probe detection of an X-ray transient
DATE: 25/02/23 16:22:43 GMT
FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn>
T. Y. Lian, W. J. Zhang (NAOC, CAS), Y. Wang (PMO, CAS), X. Tian (GXU), R. Z. Li(YNAO, CAS), H. W. Pan (NAOC, CAS) report on behalf of the Einstein Probe team:
We report on the detection of an X-ray transient by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission, designated …
[View More]EP250223a. The transient triggered EP-WXT (ID: 01709131863) at 2025-02-23T15:04:35.749 (UTC). The WXT position of the source is R.A. = 98.258 deg, DEC = -22.432 deg (J2000) with an uncertainty of 3 arcmin in radius (90% C.L. statistical and systematic).
A follow-up observation with the Follow-up X-ray Telescope (FXT) was performed automatically. Within the WXT error cirlce, an uncatalogued X-ray source was detected at R.A. = 98.2722 deg, DEC = -22.4442 deg (J2000) with an uncertainty of 20 arcsec in radius (90% C.L. statistical and systematic).
Further information will be updated when the telemetry data is received.
Launched on January 9, 2024, EP is a space X-ray observatory to monitor the soft X-ray sky with X-ray follow-up capability (Yuan et al. 2022, Handbook of X-ray and Gamma-ray Astrophysics).
View this GCN Circular online at https://gcn.nasa.gov/circulars/39429.
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TITLE: GCN CIRCULAR
NUMBER: 39428
SUBJECT: LIGO/Virgo/KAGRA S250206dm: Upper limits from IceCube neutrino searches
DATE: 25/02/23 15:10:32 GMT
FROM: Jessie Thwaites at IceCube/U Wisc-Madison <thwaites(a)wisc.edu>
IceCube Collaboration (http://icecube.wisc.edu/) reports:
IceCube has performed an additional search [1] for track-like muon neutrino events consistent with the sky localization of gravitational-wave candidate S250206dm in a time range of -0.1 day, +14 days from the …
[View More]alert event time (2025-02-06 19:01:30.439 UTC to 2025-02-20 21:25:30.439 UTC).
During this time period IceCube was collecting good quality data. In this case, we report a p-value of 0.85, consistent with no significant excess of track events. IceCube's sensitivity assuming an E^-2 spectrum (E^2 dN/dE) to neutrino point sources within the locations spanned by the 90% spatial containment of the 7-Update map ranges from 0.028 to 1.010 GeV cm^-2 in this time window.
Searches for track-like muon neutrino events detected by IceCube consistent with the 7-Update skymap in a time range of 1000 seconds centered on the alert event time (2025-02-06 21:17:10.436 UTC to 2025-02-06 21:33:50.436 UTC) were also performed using two hypothesis tests. [1,2]. The first search is a maximum likelihood analysis which searches for a generic point-like neutrino source coincident with the given GW skymap. The second uses a Bayesian approach to quantify the joint GW + neutrino event significance, which assumes a binary merger scenario and accounts for known astrophysical priors, such as GW source distance, in the significance estimate [3].
For these searches we report an overall p-value of 0.021 for the generic transient search and 0.044 for the Bayesian search using the 7-Update map. These p-values measure the consistency of the observed track-like events with the known atmospheric backgrounds for this single map (not trials corrected for multiple GW events). These results are updated since GCN 39176 with the updated skymap. Further details are available at https://gcn.nasa.gov/missions/icecube. Additional details and updates will be posted at https://roc.icecube.wisc.edu/public/LvkNuTrackSearch/.
The IceCube Neutrino Observatory is a cubic-kilometer neutrino detector operating at the geographic South Pole, Antarctica. The IceCube realtime alert point of contact can be reached at roc(a)icecube.wisc.edu.
[1] Abbasi et al. Astrophys.J. 944 (2023) 1, 80
[2] M. G. Aartsen et al 2020 ApJL 898 L10
[3] I. Bartos et al. 2019 Phys. Rev. D 100, 083017
View this GCN Circular online at https://gcn.nasa.gov/circulars/39428.
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TITLE: GCN CIRCULAR
NUMBER: 39427
SUBJECT: GRB 250221A: continued Assy optical observations, brightening afterglow confirmation
DATE: 25/02/23 11:51:11 GMT
FROM: Alexei Pozanenko at IKI, Moscow <grb.alex(a)gmail.com>
N. Pankov (HSE, IKI), V. Kim (FAI), M. Krugov (FAI), Y. Aimuratov (FAI),
A. Volnova(IKI), A. Pozanenko (IKI) report on behalf of IKI GRB FuN:
We observed the optical afterglow (Francile et al., GCN 39395; Watson et
al., GCN 39397; Melandri et al., GCN 39406; …
[View More]Shilling et al., GCN 39409; Guo
et al., GCN 39412; Muenter et al., GCN 39417; Palmerio et al., GCN 39418;
Pankov et al., GCNs 39422,39424; Ghosh et al., GCN 39425) of the Swift GRB
250221A (Caputo et al., GCN 39396) with AZT-20 telescope of Assy-Turgen
observatory starting on 2025-02-22 (UT) 15:01:45 in r' filter.
The afterglow is clearly detected. Preliminary photometry of the afterglow
in the stacked image is the following
Date UT start t-T0 Exp. Filter OT Err. UL(3sigma)
2025-02-22 15:01:45 1.49280 45x60 r' 20.50 0.05 22.7
The photometry is based on nearby PS1 stars.
Compared to our previous observations (Pankov et al., GCNs 39422, 39424,
39426) we can confirm the afterglow brightening. We can estimate the time
of the maximum earlier than 2025-02-22 (UT) 12:29:44
View this GCN Circular online at https://gcn.nasa.gov/circulars/39427.
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TITLE: GCN CIRCULAR
NUMBER: 39426
SUBJECT: GRB 250221A: continued Mondy optical observations, brightening afterglow
DATE: 25/02/23 11:47:30 GMT
FROM: Alexei Pozanenko at IKI, Moscow <grb.alex(a)gmail.com>
N. Pankov (HSE, IKI), A. Pozanenko (IKI), E. Klunlo (ISZF), A. Volnova
(IKI) report on behalf of IKI GRB FuN:
We observed the optical afterglow (Francile et al., GCN 39395; Watson et
al., GCN 39397; Melandri et al., GCN 39406; Shilling et al., GCN 39409; Guo
et al., GCN 39412;…
[View More] Muenter et al., GCN 39417; Palmerio et al., GCN 39418;
Pankov et al., GCNs 39422,39424; Ghosh et al., GCN 39425) of the Swift GRB
250221A (Caputo et al., GCN 39396) with AZT-33IK telescope of Mondy
observatory starting on 2025-02-22 (UT) 12:29:44 in R filter.
The afterglow is clearly detected. Preliminary photometry of the afterglow
in the stacked image is the following
Date UT start t-T0 Exp. Filter OT Err. UL(3sigma)
2025-02-22 12:29:44 1.38790 18x120 R 19.95 0.05 21.6
The photometry is based on nearby USNO-B1.0 (R2) stars.
Compared to our previous observations (Pankov et al., GCNs 39422,39424) the
afterglow has apparently become brighter.
View this GCN Circular online at https://gcn.nasa.gov/circulars/39426.
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TITLE: GCN CIRCULAR
NUMBER: 39425
SUBJECT: GRB 250221A: Optical counterpart detection by LCO.
DATE: 25/02/22 15:06:17 GMT
FROM: ankur ghosh at CAPP, University of Johannesburg <ghosh.ankur1994(a)gmail.com>
Ankur Ghosh, Soebur Razzaque (CAPP, University of Johannesburg), Alexander Moskvitin, Yulia Sotnikova (SAO RAS), Naveen Dukiya (ARIES), Rahul Gupta (NASA GSFC) on behalf of a larger collaboration.
We observed the field of the GRB 250221A triggered by Swift (Caputo et al., …
[View More]GCN 39396) in B, r filters of the 1-meter Sinistro telescope at the Las Cumbres Observatory Global Telescope (LCOGT) node located at Cerro Tololo Interamerican Observatory, Chille. The 1-m Sinistro telescope is equipped with a 4K x 4K CCD (FOV: 26 x 26 arcmin, scale: 0.39 arcsec/pixel).
Observations began on February 21, 2025, starting 22.46 hours after the GRB trigger.
We clearly detect the optical transient (OT) reported by GCNs ( Francile et al., GCN 39395; Watson et al., GCN 39397; Melandri et al., GCN 39406; Shilling et al., GCN 39409; Guo et al., GCN 39412; Muenter et al., GCN 39417; Palmerio et al., GCN 39418; Pankov et al., GCN 39422; Pankov et al., GCN 39424) in our B, r band image.
|Date| |UTstart| |t-T0 (hours)| |Exp (sec)| |Filter| |Magnitude|
----------------------------------------------------------------------------------------------------
2025-02-22 02:02:15.36 22.46 1 x 1200 B B = 21.91 +/- 0.06
2025-02-22 02:10:02.78 22.59 1 x 900 r r = 20.85 +/- 0.06
----------------------------------------------------------------------------------------------------
The field was calibrated against nearby APASS stars, with magnitudes converted using Lupton (2005) equations, and has not been corrected for Galactic extinction.
View this GCN Circular online at https://gcn.nasa.gov/circulars/39425.
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