TITLE: GCN CIRCULAR
NUMBER: 38900
SUBJECT: GRB 250109A / EP250109A: Swift/BAT-GUANO localization skymap of a burst
DATE: 25/01/10 21:06:43 GMT
FROM: Jimmy DeLaunay at Penn State <delauj2(a)gmail.com>
James DeLaunay (PSU), Samuele Ronchini (PSU), Aaron Tohuvavohu (Caltech), Gayathri Raman (PSU), Jamie A. Kennea (PSU), Tyler Parsotan (NASA GSFC) report:
Swift/BAT did not localize GRB 250109A onboard (T0: 2025-01-09T06:17:08.60 UTC, Fermi trig 758096233)
The Fermi notice, …
[View More]distributed in near real-time, triggered the Swift Mission Operations Center operated Gamma-ray Urgent Archiver for Novel Opportunities (GUANO; Tohuvavohu et al. 2020, ApJ, 900, 1).
Upon trigger by this notice, GUANO sent a command to the Swift Burst Alert Telescope (BAT) to save 200 seconds of BAT event-mode data from [-50,+150] seconds around the time of the burst. All the requested event mode data was delivered to the ground.
The BAT likelihood search, NITRATES (DeLaunay + Tohuvavohu 2022, ApJ, 941, 169), performed on the temporal window [T0-20 s, T0+20 s], detects the burst with a sqrt(TS) of 12.1 in a 16.384 s analysis time bin, starting at T0 - 8.192 s.
Using the NITRATES analysis, parameter estimation was performed to obtain the localization of this burst in the form of a HEALPIX Multi-Order Coverage (MOC) skymap. This localization accounts for both statistical and systematic errors. More details in the creation and calibration of these maps will soon be published (DeLaunay et al. 2025. in prep)
The 90% credible area is 0.06 deg2 and the 50% credible area is ~0.01 deg2.
The integrated probability inside the coded field of view is 98%.
55% of the NITRATES localization probability is contained within a 0.1 deg radius circle around the maximum probability position. The majority of the remaining probability is contained within similarly sized peaks of probability across the BAT coded field of view.
The maximum probability position of the NITRATES skymap is,
RA, Dec = 88.806, -12.458 deg which is
RA(J2000) = 05h 55m 13.4s
Dec(J2000) = -12d 27′ 28.8″
The NITRATES skymap is consistent with the Fermi localization reported in the final position notice (GCN 38873). It is also consistent with the position of the X-ray transient EP250109a (GCN 38864, GCN 38889), with the position lying on the 0.28 credible region contour. The spatial and temporal coincidence of GRB 250109A and EP250109a make it very likely that they originate from the same cosmic event.
A plot of the probability skymap can be viewed here:
[skymap_plot](https://guano.swift.psu.edu/trigger_report?id=758096263/#:~:te…
The probability skymap file can be downloaded from the link here
[skymap_fits_file](https://guano.swift.psu.edu/files/758096263/0_n_PROBMAP)
Instructions on how to read and manipulate this map can be found here:
https://guano.swift.psu.edu/documentation
More details about this burst can be found on the trigger report page here:
https://guano.swift.psu.edu/trigger_report?id=758096263
GUANO is a fully autonomous, extremely low latency, spacecraft commanding pipeline designed for targeted recovery of BAT event mode data around the times of compelling astrophysical events to enable more sensitive GRB searches.
A live reporting of Swift/BAT event data recovered by GUANO can be found at:
https://www.swift.psu.edu/guano/
View this GCN Circular online at https://gcn.nasa.gov/circulars/38900.
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TITLE: GCN CIRCULAR
NUMBER: 38899
SUBJECT: GRB 250109A / EP250109a: Swift detection of the X-ray afterglow
DATE: 25/01/10 20:57:21 GMT
FROM: Jamie Kennea at Penn State <jak51(a)psu.edu>
J. A. Kennea (PSU), P. A. Evans and K. L. Page (Leicester) report on behalf of the Swift/XRT team:
Swift/XRT performed a further 3.1ks of exposure on GRB 250109A (GCN #38887) AKA EP250109a (GCN #38864), following on from a rapid 1ks observation which did not detect the counterpart (GCN #38867). …
[View More]Combining the two datasets, we detect one point source inside the EP WXT error circle, at the following position: RA/Dec(J2000) = 88.80698, -12.4958, which is equivalent to:
RA(J2000) = 05h 55m 13.67s,
Dec(J2000) = -12° 29′ 44.8″,
with an estimated uncertainty of 5.8 arc-seconds radius (90% containment). This position lies 6 arc-seconds from the EP FXT position, and 1.1 arc-seconds from the SVOM-VT reported optical position (GCN #38872). Given the localization coincidence, this source is likely to be the afterglow of GRB 250109A.
The combined XRT flux from this afterglow is 9(+5,-4) x 10^-14 erg/s/cm^2 (0.3-10 keV).
View this GCN Circular online at https://gcn.nasa.gov/circulars/38899.
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TITLE: GCN CIRCULAR
NUMBER: 38898
SUBJECT: GRB 250108A: Swift/XRT afterglow fading
DATE: 25/01/10 17:28:08 GMT
FROM: Tullia Sbarrato at INAF-OAB <tullia.sbarrato(a)inaf.it>
Tullia Sbarrato (INAF-OAB) & Noel Klinger (GSFC/UMBC/CRESSTII)
report on behalf of the Swift-XRT team:
Swift-XRT has performed further follow-up observations of the
SVOM/ECLAIRs GRB 250108A (Zheng et al., GCN 38845),
collecting 6.6 ks of Photon Counting (PC) mode data between
T0+16.1 ks and T0+192.1 ks.…
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The X-ray source detected in the first 2.7 ks of data reported as
“Source 1” and presented as possible GRB afterglow candidate
(Ambrosi et al., GCN 38853) has faded more than 2 sigma
in the latest observation, and it is thus confirmed as the
X-ray afterglow of the burst.
The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00021755.
This circular is an official product of the Swift-XRT team.
View this GCN Circular online at https://gcn.nasa.gov/circulars/38898.
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TITLE: GCN CIRCULAR
NUMBER: 38897
SUBJECT: GRB 250107D: CALET Gamma-Ray Burst Monitor detection
DATE: 25/01/10 17:22:49 GMT
FROM: Yuta Kawakubo at Aoyama Gakuin University <kawakubo(a)phys.aoyama.ac.jp>
T. Sakamoto, A. Yoshida, S. Sugita, Y. Kawakubo (AGU),
K. Yamaoka (Nagoya U), S. Nakahira (JAXA), Y. Asaoka (ICRR), S. Torii,
Y. Akaike, K. Kobayashi (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U),
N. Cannady (GSFC/UMBC), M. L. Cherry (LSU), S. Ricciarini (U of Florence),
P. S. …
[View More]Marrocchesi (U of Siena),
and the CALET collaboration:
The short GRB 250107D (IPN triangulation: Kozyrev et al., GCN Circ. 38880;
Konus-Wind detection: Frederiks et al., GCN Circ. 38881) triggered the CALET
Gamma-ray Burst Monitor (CGBM) at 05:23:36.72 UTC on 7 January 2025
(https://cgbm.calet.jp/cgbm_trigger/flight/1420262534/index.html).
The burst signal was seen by only the SGM detector. Because of a problem with the ground
alert processing script, the GCN notice was not distributed automatically for this event.
The burst light curve shows a single pulse that starts
at T+0.17 sec, peaks at T+0.25 sec, and ends at T+0.32 sec.
The T90 and T50 durations measured by the SGM data are 0.13 +/- 0.03 sec
and 0.08 +/- 0.02 sec (40-1000 keV), respectively.
The ground-processed light curve is available at
https://cgbm.calet.jp/cgbm_trigger/ground/1420262534/
The CALET data used in this analysis are provided by
the Waseda CALET Operation Center located at Waseda University.
View this GCN Circular online at https://gcn.nasa.gov/circulars/38897.
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TITLE: GCN CIRCULAR
NUMBER: 38896
SUBJECT: GRB 250107C: CALET Gamma-Ray Burst Monitor detection
DATE: 25/01/10 16:51:07 GMT
FROM: Yuta Kawakubo at Aoyama Gakuin University <kawakubo(a)phys.aoyama.ac.jp>
A. Yoshida, T. Sakamoto, S. Sugita, Y. Kawakubo (AGU),
K. Yamaoka (Nagoya U), S. Nakahira (JAXA), Y. Asaoka (ICRR), S. Torii,
Y. Akaike, K. Kobayashi (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U),
N. Cannady (GSFC/UMBC), M. L. Cherry (LSU), S. Ricciarini (U of Florence),
P. S. …
[View More]Marrocchesi (U of Siena),
and the CALET collaboration:
The long GRB 250107C (SVOM/GRM observation: SVOM/GRM team, GCN Circ.
38870; IPN triangulation: Svinkin et al., GCN Circ. 38879; Konus-Wind detection:
Frederiks et al., GCN Circ. 38895) triggered the CALET Gamma-ray Burst Monitor (CGBM)
at 18:52:15.99 UTC on 7 January 2025
(https://cgbm.calet.jp/cgbm_trigger/flight/1420311052/index.html).
The burst signal was seen by only the SGM detector. Because of a problem with the ground
alert processing script, the GCN notice was not distributed automatically for this event.
The burst light curve shows a double-peaked structure that starts
at T-0.2 sec, peaks at T+0.7 sec, and ends at T+3.0 sec.
The T90 and T50 durations measured by the SGM data are 2.6 +/- 0.2 sec
and 1.6 +/- 0.1 sec (40-1000 keV), respectively.
The ground-processed light curve is available at
https://cgbm.calet.jp/cgbm_trigger/ground/1420311052/
The CALET data used in this analysis are provided by
the Waseda CALET Operation Center located at Waseda University.
View this GCN Circular online at https://gcn.nasa.gov/circulars/38896.
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TITLE: GCN CIRCULAR
NUMBER: 38895
SUBJECT: Konus-Wind detection of GRB 250107C
DATE: 25/01/10 15:59:26 GMT
FROM: Dmitry Frederiks at Ioffe Institute <fred(a)mail.ioffe.ru>
D. Frederiks, A.Lysenko, A. Ridnaia, D. Svinkin,
A. Tsvetkova, M. Ulanov, and T. Cline,
on behalf of the Konus-Wind team, report:
The long GRB 250107C (SVOM/GRM observation: Xue et al., GCN 38870;
IPN triangulation: Svinkin et al., GCN 38879)
triggered Konus-Wind (KW) at T0=67934.719 s UT (18:52:14.719).
…
[View More]The burst consists of two overlapping peaks and had the total duration of ~4 s.
The emission is seen up to ~10 MeV.
The Konus-Wind light curve of this GRB is available at
http://www.ioffe.ru/LEA/GRBs/GRB250107_T67934/
As observed by Konus-Wind, the burst had
a fluence of (3.02 ± 0.13)x10^-5 erg/cm^2 and
a 64-ms peak energy flux, measured from T0 + 0.960 s,
of (2.23 ± 0.15)x10^-5 erg/cm^2/s (both in the 20 keV - 10 MeV energy range).
The time-integrated spectrum (measured from T0 to T0+10.752 s)
is best fit in the 20 keV - 15 MeV range
by a GRB (Band) function with the following model parameters:
the low-energy photon index alpha = -0.41 (-0.06,+0.06),
the high energy photon index beta = -3.03 (-0.28,+0.18),
the peak energy Ep = 254 (-10,+11) keV,
chi2 = 78/79 dof.
The spectrum near the peak count rate (measured from T0+0.768 s to T0+1.024 s)
is best fit in the 20 keV - 15 MeV range
by a GRB (Band) function with the following model parameters:
the low-energy photon index alpha = -0.01 (-0.13,+0.15),
the high energy photon index beta = -3.09 (-0.49,+0.29),
the peak energy Ep = 286 (-22,+21) keV,
chi2 = 30/38 dof.
All the quoted errors are estimated at the 68% confidence level.
All the presented results are preliminary.
View this GCN Circular online at https://gcn.nasa.gov/circulars/38895.
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TITLE: GCN CIRCULAR
NUMBER: 38894
SUBJECT: LIGO/Virgo/KAGRA S250109bi: Updated Sky localization
DATE: 25/01/10 14:58:34 GMT
FROM: alexandresebastien.goettel(a)LIGO.org
The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration report:
We have conducted further analysis of the LIGO Hanford Observatory (H1) and Virgo Observatory (V1) data around the time of the compact binary merger (CBC) candidate S250109bi (GCN Circular 38863). Parameter estimation has …
[View More]been performed using Bilby [1] and a new sky map, Bilby.multiorder.fits,0, distributed via GCN Notice, is available for retrieval from the GraceDB event page:
https://gracedb.ligo.org/superevents/S250109bi
For the Bilby.multiorder.fits,0 sky map, the 90% credible region is 2819 deg2. Marginalized over the whole sky, the a posteriori luminosity distance estimate is 2255 +/- 734 Mpc (a posteriori mean +/- standard deviation).
For further information about analysis methodology and the contents of this alert, refer to the LIGO/Virgo/KAGRA Public Alerts User Guide https://emfollow.docs.ligo.org/.
[1] Ashton et al. ApJS 241, 27 (2019) doi:10.3847/1538-4365/ab06fc and Morisaki et al. (2023) arXiv:2307.13380
View this GCN Circular online at https://gcn.nasa.gov/circulars/38894.
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TITLE: GCN CIRCULAR
NUMBER: 38893
SUBJECT: LIGO/Virgo/KAGRA S250109f: Updated Sky localization
DATE: 25/01/10 14:55:16 GMT
FROM: alexandresebastien.goettel(a)LIGO.org
The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration report:
We have conducted further analysis of the LIGO Hanford Observatory (H1), LIGO Livingston Observatory (L1), and Virgo Observatory (V1) data around the time of the compact binary merger (CBC) candidate S250109f (GCN Circular …
[View More]38860). Parameter estimation has been performed using Bilby [1] and a new sky map, Bilby.multiorder.fits,0, distributed via GCN Notice, is available for retrieval from the GraceDB event page:
https://gracedb.ligo.org/superevents/S250109f
For the Bilby.multiorder.fits,0 sky map, the 90% credible region is 243 deg2. Marginalized over the whole sky, the a posteriori luminosity distance estimate is 3200 +/- 948 Mpc (a posteriori mean +/- standard deviation).
For further information about analysis methodology and the contents of this alert, refer to the LIGO/Virgo/KAGRA Public Alerts User Guide https://emfollow.docs.ligo.org/.
[1] Ashton et al. ApJS 241, 27 (2019) doi:10.3847/1538-4365/ab06fc and Morisaki et al. (2023) arXiv:2307.13380
View this GCN Circular online at https://gcn.nasa.gov/circulars/38893.
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TITLE: GCN CIRCULAR
NUMBER: 38892
SUBJECT: LIGO/Virgo/KAGRA S250108eo: Updated Sky localization
DATE: 25/01/10 14:50:11 GMT
FROM: alexandresebastien.goettel(a)LIGO.org
The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration report:
We have conducted further analysis of the LIGO Hanford Observatory (H1), LIGO Livingston Observatory (L1), and Virgo Observatory (V1) data around the time of the compact binary merger (CBC) candidate S250108eo (GCN Circular …
[View More]38851). Parameter estimation has been performed using Bilby [1] and a new sky map, Bilby.multiorder.fits,0, distributed via GCN Notice, is available for retrieval from the GraceDB event page:
https://gracedb.ligo.org/superevents/S250108eo
For the Bilby.multiorder.fits,0 sky map, the 90% credible region is 795 deg2. Marginalized over the whole sky, the a posteriori luminosity distance estimate is 4306 +/- 1349 Mpc (a posteriori mean +/- standard deviation).
For further information about analysis methodology and the contents of this alert, refer to the LIGO/Virgo/KAGRA Public Alerts User Guide https://emfollow.docs.ligo.org/.
[1] Ashton et al. ApJS 241, 27 (2019) doi:10.3847/1538-4365/ab06fc and Morisaki et al. (2023) arXiv:2307.13380
View this GCN Circular online at https://gcn.nasa.gov/circulars/38892.
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TITLE: GCN CIRCULAR
NUMBER: 38891
SUBJECT: EP-WXT trigger EP250108a:Xinglong optical follow-up observations
DATE: 25/01/10 14:14:46 GMT
FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn>
Report on behalf of the Xinglong collaboration: Junjie-Jin(NAOC), Haiyang-Mu(NAOC), Jinlei-Zhang(NAOC), Shengsheng-Zhang(NAOC), Pengliang-Du(NAOC), JianFeng-Tian(NAOC), Zhou-Fan(NAOC), Hong-Wu(NAOC), Jie-Zheng (NAOC)
We observed the field of the X-ray transient, EP 250108a by the the Tsinghua-NAOC 0.…
[View More]8-m telescope (TNT) located at Xinglong, Hebei, China. A total of 300 s g-band exposures were taken , with a median observation time of 2025-01-09 T11:51:01, approximately 23.5 hours after the EP trigger. No optical counterpart was detected, with a 5-sigma limiting magnitude of 21.85, calibrated with Pan-STARRS sources in the field.
View this GCN Circular online at https://gcn.nasa.gov/circulars/38891.
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