J.A. Kennea (PSU) and N.P.M. Kuin (UCL-MSSL) for the Swift team
Kennea and Williams (GCN Circ. 32635) reported the initial Swift results. We provide an update on the BAT trigger 1126853, AKA Swift J1913.1+1946 (GCN Circ. 32632). At the time of the trigger, the initial BAT position was 95° from the Sun (6.2 hours East) and 84° from the 100%-illuminated Moon. Table 1 contains the best reported positions from Swift, and the latest XRT position can be viewed at http://www.swift.ac.uk/xrt_positions.
Lipunov et al. (GCN Circ. 32634) reported the position from MASTER for the optical afterglow of this GRB. Kuin and Dichiara (GCN Circ. 32656) reported the detection with UVOT of an optical afterglow. de Ugarte Postigo et al. (GCN Circ. 32648) determined a redshift of 0.151 from VLT, Castro-Tirado et al. (GCN Circ. 32686) determined a redshift of 0.1505 from GTC, and Izzo et al. (GCN Circ. 32765) determined a redshift of 0.151 from VLT. Table 2 is a summary of GCN Circulars about this GRB from observatories other than Swift.
Standard analysis products for this burst are available at https://gcn.gsfc.nasa.gov/swift_gnd_ana.html.
As reported by Krimm et al. (GCN Circ. 32688),
the BAT ground-calculated position is RA, Dec = 288.254, 19.809 deg which is RA(J2000) = 1
The mask-weighted light curve (Figure 1) shows a flat and long-lasting emission that may have started before the burst came into the BAT FOV at T-26 s.
The burst emission seems to end at ~T+1320 s, however, we cannot rule out the possibility that the emission extends beyond the available event data that end at T+1371 s.
The lower limit of
The time-averaged spectrum from T+103.3 s to T+1338.7 s s is best fit by a simple power-law model.
The power law index of the time-averaged spectrum is 2.08 ± 0.03.
The fluence in the 15-150 keV band is 7.4 ± 0.1 x 1
The results of the batgrbproduct analysis are available at https://gcn.gsfc.nasa.gov/notices_s/1126853/BA/.
Analysis of the initial XRT data was reported by Kennea et al. (GCN Circ. 32651). We have analysed 277 ks of XRT data for GRB 221009A (E Bissaldi et al. GCN Circ. 32637), from 174 s to 5176.4 ks after the BAT trigger. The data comprise 16 ks in Windowed Timing (WT) mode with the remainder in Photon Counting (PC) mode.
The late-time light curve (Figure 2) (from T0+18.4 ks) can be modelled with a series of power-law decays. The initial decay index is α=1.519 ± 0.004. At T+42.0 ks the decay flattens to an α of 0.9 (+0.5, -0.8). The light curve breaks again at T+45.4 ks to a decay with α=1.730 ± 0.015, again at T+441 ks s to α=-0.2 (+1.1, -1.3), and again at T+512 ks s to α=1.90 (+0.10, -0.07), before a final break at T+1745 ks s after which the decay index is 1.10 ± 0.16.
A spectrum formed from the WT mode data can be fitted with an absorbed power-law with a photon spectral index of 1.806 ± 0.011. The best-fitting absorption column is 6.70 (+0.16, -0.15) x 1
A summary of the PC-mode spectrum is thus:
Galactic foreground: 5.4 x 1
Intrinsic column: 7.6 (+2.9, -2.6) x 1
Photon index: 1.79 (+0.20, -0.19)
The results of the XRT team automatic analysis are available at http://www.swift.ac.uk/xrt_products/01126853.
Analysis of the UVOT data was reported by Kuin and Dichiara (GCN Circ. 32656).
Table 3 gives preliminary
magnitudes using the UVOT photometric system
(Breeveld et al. 2011, AIP Conf. Proc., 1358, 373).
No correction has been made for the expected extinction in the Milky Way
corresponding to a reddening of
Figure 1. The BAT
mask-weighted light curve in the four individual and total
energy bands. The units are counts
Figure 2. The XRT light curve.
Any data from a crosshatched region are not included in the fit.
RA (J2000) | Dec (J2000) | Error | Note | Reference |
---|---|---|---|---|
1 |
+19°46'24.6" | 0.61" | UVOT | GCN Circ. 32632 |
1 |
+19°46'16.3" | 5.6" | XRT | ? |
1 |
+19°48'34.1" | 2.4' | BAT-refined | Krimm et al. GCN Circ. 32688 |
Band | Authors | GCN Circ. | Subject | Observatory | Notes |
---|---|---|---|---|---|
Optical | Lipunov et al. | 32634 | Swift GRB221009.59: Global MASTER-Net OT detection |
MASTER | detection |
Optical | Hu et al. | 32644 | BOOTES-2/TELMA and OSN optical detections |
BOOTES-2 | detection |
Optical | Belkin et al. | 32645 | (Swift J1913.1+1946): Mondy optical observations |
Mondy | detection |
Optical | de Wet and Groot | 32646 | (Swift J1913.1+1946): MeerLICHT observations |
MeerLICHT | |
Optical | Xu et al. | 32647 | Nanshan/NEXT photometry and Xinglong-2.16m spectroscopy |
Xinjiang Astro. Obs. | spectroscopy |
Optical | de Ugarte Postigo et al. | 32648 | Redshift from X-shooter/VLT | VLT | redshift |
Optical | Brivio et al. | 32652 | REM optical and NIR detection of the afterglow |
REM | detection |
Optical | Durbak et al. | 32654 | or Swift J1913.1+1946: PRIME near-infrared detection |
detection | |
Optical | Paek et al. | 32659 | GRB 221009A: Multi-color detection of the optical |
LOAO | detection |
Optical | Kumar et al. | 32662 | Swift J1913.1+1946: GIT detection of the optical afterglow |
GROWTH-India Tel. | detection |
Optical | F. Romanov | 32664 | (Swift J1913.1+1946): Burke-Gaffney Observatory optical observations |
Burke-Gaffney Obs. | |
Optical | Chen et al. | 32667 | Lulin SLT-40cm optical observations | Lulin | |
Optical | Vidal et al. | 32669 | Swift J1913.1+1946: Lick/Nickel telescope optical observations |
KAIT | detection |
Optical | Kim et al. | 32670 | Swift J1913.1+1946: Assy optical afterglow observation |
Assy-Turgen Obs. | detection |
Optical | Groot et al. | 32678 | BlackGEM optical observations | detection | |
Optical | F. Romanov | 32679 | (Swift J1913.1+1946): iTelescope optical observation |
iTelescope | |
Optical | Belkin et al. | 32684 | Sintez-Newton/CrAO optical observations | CrAO | detection |
Optical | Castro-Tirado et al. | 32686 | 10.4m GTC spectroscopic redshift confirmation |
GTC | redshift |
Optical | Watson et al. | 32692 | COATLI Detection of the Afterglow | COATLI | detection |
Optical | Strausbaugh and Cucchiara | 32693 | LCOGT Optical Afterglow Detection | Las Cumbres Obs. Global Tele.Network | detection |
Optical | Butler et al. | 32705 | COATLI Continued Monitoring of the Afterglow |
COATLI | |
Optical | Vinko et al. | 32709 | optical afterglow measurements from Konkoly Observatory |
Konkoly | detection |
Optical | Mao et al. | 32727 | GMG observation | Gao-Mei-Gu | |
Optical | Zaznobin et al. | 32729 | Sayan observatory 1.6-m telescope observations |
Sayan Obs. | |
Optical | Sasada et al. | 32730 | MITSuME Okayama optical observation | MITSuME Okayama | |
Optical | Strausbaugh and Cucchiara | 32738 | LCOGT Continued Observations - Optical Upper Limits |
Las Cumbres Obs. Global Tele.Network | upper limits |
Optical | O'Connor et al. | 32739 | Lowell Discovery Telescope Afterglow Detection |
Lowell Discovery Telescope | detection |
Optical | Bikmaev et al. | 32743 | RTT-150 optical observations | ||
Optical | Rastinejad and Fong | 32749 | Gemini-South Optical Afterglow Detection | Gemini | detection |
Optical | O'Connor et al. | 32750 | Gemini-South Infrared Afterglow Detection |
Gemini | detection |
Optical | Bikmaev et al. | 32752 | RTT-150 optical observations | light curve | |
Optical | Schneider et al. | 32753 | OHP optical observations | ||
Optical | D’Avanzo et al. | 32755 | continued REM optical/NIR observations and evidence for an achromatic steepening in the afterglow light curve |
REM | light curve |
Optical | Huber et al. | 32758 | Pan-STARRS optical photometry | Pan-STARRS | |
Optical | Shrestha et al. | 32759 | Large Binocular Telescope Observatory optical afterglow detection |
Gemini | detection |
Optical | Izzo et al. | 32765 | VLT spectroscopic detection of the host galaxy |
VLT | |
Optical | Belkin et al. | 32769 | continued Assy optical afterglow observations, possible SN evidence |
Assy-Turgen Obs. | light curve |
Optical | Shrestha et al. | 32771 | Faulkes Telescope North continued optical afterglow follow-up |
FTN | detection |
Optical | Rajabov et al. | 32795 | GRANDMA observations | GRANDMA | |
Optical | O'Connor et al. | 32799 | Continued LDT Afterglow Monitoring | Lowell Discovery Telescope | detection |
Optical | Im et al. | 32803 | BOAO NIR detections | BOAO | detection |
Optical | Ferro et al. | 32804 | TNG NIR detection | TNG | detection |
Optical | Rossi et al. | 32809 | LBT optical imaging | LBT | detection |
Optical | Gupta et al. | 32811 | 1.3m DFOT Optical Observations | DFOT | detection |
Optical | Belkin et al. | 32818 | optical observations, SN photometric evidence |
Assy-Turgen Obs. | detection |
Optical | Levan et al. | 32821 | James Webb Space Telescope Observations | James Webb | detection |
Optical | Maiorano et al. | 32850 | spectroscopic confirmation of SN in LBT spectra |
LBT | |
Optical | Pellegrin and Rumstay | 32852 | SARA-RM 1m Optical Afterglow Detection | SARA | detection |
Optical | O'Connor et al. | 32860 | Further Gemini-South Infrared Observations |
Gemini | detection |
Optical | Pellegrin and Rumstay | 32912 | Correction to GCN Circ. 32852 (GRB 221009A: SARA-RM 1m Optical Afterglow Detection) |
SARA | detection |
Optical | Levan et al. | 32921 | Hubble Space Telescope observations | Hubble Space Telescope | detection |
Optical | Aguerre et al. | 32934 | GRANDMA/Kilonova-Catcher observations | GRANDMA | |
Optical | de Wet | 32944 | Correction to GCN Circ. 32646 (GRB 221009A (Swift J1913.1+1946): MeerLICHT observations) |
MeerLICHT | |
Optical | Lindfors et al. | 32995 | Optical polarization observation | NOT | |
Radio | Bright et al. | 32653 | Swift J1913.1+1946: AMI-LA observations | AMI | |
Radio | de Ugarte Postigo et al. | 32676 | NOEMA mm detection | NOEMA | detection |
Radio | Rhodes et al. | 32707 | Swift J1913.1+1946: SMA observations | SMA | |
Radio | Laskar et al. | 32740 | MeerKAT detection | MeerKAT | detection |
Radio | Laskar et al. | 32757 | VLA detection | VLA | detection |
Radio | Urata et al. | 32761 | ALMA and ACA detections | ALMA | detection |
Radio | Bhandari et al. | 32763 | ATCA detection | ATCA | detection |
Radio | Leung et al. | 32766 | ATCA radio spectrum | ATCA | detection |
Radio | Marongiu et al. | 32791 | Medicina Radio Telescope observations | Medicina Radio | |
Radio | Atri et al. | 32907 | High-precision position of the compact radio counterpart to GRB221009A |
VLBA | detection |
Radio | Niinuma et al. | 32949 | Japanese VLBI Network observation | VLBI | |
X-ray | Negro | 32690 | planned observation with the Imaging X-ray Polarimetry Explorer (IXPE) |
plans | |
X-ray | Brethauer et al. | 32695 | NuSTAR Detection | NuSTAR | detection |
X-ray | Manfreda | 32754 | IXPE preliminary upper limits of X-ray polarization |
upper limits | |
X-ray | Kobayashi et al. | 32756 | MAXI/GSC refined analysis of the bright X-ray afterglow of GRB 221009A/Swift J1913.1+1946 |
MAXI | |
X-ray | Liu et al. | 32767 | LEIA X-ray Afterglow Detection | detection | |
X-ray | Brethauer et al. | 32788 | Second epoch of NuSTAR data | NuSTAR | |
X-ray | Aimuratov et al. | 32802 | X-ray light-curve and the indication of TeV light-curve |
||
Gamma-ray | Veres et al. | 32636 | Fermi GBM detection of an extraordinarily bright GRB |
Fermi GBM | |
Gamma-ray | Bissaldi et al. | 32637 | or Swift J1913.1+1946: Fermi-LAT detection |
Fermi LAT | |
Gamma-ray | Svinkin et al. | 32641 | IPN triangulation of extremely bright GRB 221009A |
IPN | |
Gamma-ray | Lesage et al. | 32642 | Fermi GBM observation | Fermi GBM | Fluence=2.12±0.05x1 (brighter than 88% of long GRBs) |
Gamma-ray | Ursi et al. | 32650 | (Swift J1913.1+1946): AGILE/MCAL detection |
AGILE | |
Gamma-ray | Piano et al. | 32657 | (Swift J1913.1+1946): AGILE/GRID detection |
AGILE | |
Gamma-ray | Pillera et al. | 32658 | Fermi-LAT refined analysis | Fermi LAT | |
Gamma-ray | Gotz et al. | 32660 | Swift J1913.1+1946: INTEGRAL SPI/ACS observations |
INTEGRAL | |
Gamma-ray | Lapshov et al. | 32663 | Swift J1913.1+1946: SRG/ART-XC observation |
SRG/ART | |
Gamma-ray | Frederiks et al. | 32668 | Konus-Wind detection | Konus-Wind | |
Gamma-ray | Huang et al. | 32677 | LHAASO observed GRB 221009A with more than 5000 VHE photons up to around 18 TeV |
LHAASO | |
Gamma-ray | Ayala et al. | 32683 | Upper limits from HAWC 8 hours after trigger |
HAWC | |
Gamma-ray | Ripa et al. | 32685 | Detection by GRBAlpha | GRBAlpha | |
Gamma-ray | Savchenko et al. | 32691 | INTEGRAL detection of Hard X-ray emission up to 38 hours after trigger |
INTEGRAL | |
Gamma-ray | Mitchell et al. | 32746 | Gamma-ray Detection by SIRI-2 | SIRI-2 | |
Gamma-ray | Xia et al. | 32748 | a 397.7 GeV photon observed by Fermi-LAT at 0.4 day after the GBM trigger |
Fermi GBM | |
Gamma-ray | Liu et al. | 32751 | HEBS detection | HEBS | |
Gamma-ray | Omodei et al. | 32760 | Fermi LAT data rate effects due to extremely high flux |
Fermi LAT | |
Gamma-ray | Kozyrev et al. | 32805 | Improved IPN localization for GRB 221009A (BepiColombo-MGNS light curve) |
IPN | |
Gamma-ray | Minaev et al. | 32819 | Analysis of the initial episode using data of GBM/Fermi and SPI-ACS/INTEGRAL |
Fermi GBM | |
Gamma-ray | Omodei et al. | 32916 | Extended Bad Time Intervals for Fermi LAT data |
Fermi LAT | |
Gamma-ray | Laboratory | 32973 | :DAMPE observed a 34.7 GeV p | DAMPE | |
Neutrino | Collaboration | 32665 | Upper limits from a neutrino search with IceCube |
IceCube | upper limits |
Neutrino | Collaboration | 32741 | search for neutrinos with KM3NeT | ||
Other | Schnoor et al. | 32744 | Detection as sudden ionospheric disturbances (SID) |
detection | |
Other | Guha and Nicholson | 32745 | Ionospheric disturbance observed in India |
||
Other | Kann and Fernandez | 32762 | Armchair Energetics | light curve | |
Other | Aimuratov et al. | 32780 | A type I BdHN of exceptional energetics | ||
Other | J. Atteia | 32793 | The probability of observing GRB 221009A at z = 0.151 |
redshift | |
Other | de Ugarte Postigo et al. | 32800 | Spectroscopic detection of emerging SN features |
||
Other | Aimuratov et al. | 32808 | Peak luminosity of the supernova vs. synchrotron afterglow |
||
Other | Aimuratov et al. | 32828 | Determination of the black holes mass and spin |
||
Other | of the LIGO and Virgo | 32877 | LIGO-Virgo-KAGRA and GEO600 statement on GRB 221009A |
||
Other | Kimura et al. | 33038 | MuSCAT3 observations | light curve |
Filter | Exp(s) | Mag | ||
---|---|---|---|---|
white | 179 | 329 | 147 | 16.68 ± 0.03 |
v | 668 | 688 | 20 | 15.55 ± 0.10 |
b | 593 | 613 | 20 | 17.05 ± 0.11 |
u | 337 | 587 | 246 | 17.68 ± 0.06 |
w1 | 718 | 1293 | 58 | >18.2 |
w2 | 817 | 1219 | 39 | >19.1 |
Table 3. UVOT observations reported by Kuin and Dichiara (GCN Circ. 32656). The start and stop times of the exposures are given in seconds since the BAT trigger. The preliminary detections and 3-σ upper limits are given. No correction has been made for extinction in the Milky Way.
December 10, 2022