Swift Observations of GRB 221009A

J.A. Kennea (PSU) and N.P.M. Kuin (UCL-MSSL) for the Swift team

1. Introduction

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.

2. BAT Observations and Analysis

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) = 19h13m00.9s Dec(J2000) = +19°48'34.1" with an uncertainty of 2.4 arcmin, (radius, sys+stat, 90% containment). The partial coding was 9%.

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 T90 (15-350 keV) is 1068.40 ± 13.34 s (estimated error including systematics).

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 10-5 erg cm-2. This fluence is larger than that of 99.5% of the long GRBs in the Second BAT GRB Catalog (Sakamoto et al. 2011). The 1-s peak photon flux measured from T+776.47 s in the 15-150 keV band is 1.9 ± 0.3 ph cm-2 s-1. All the quoted errors are at the 90% confidence level.

The results of the batgrbproduct analysis are available at https://gcn.gsfc.nasa.gov/notices_s/1126853/BA/.

3. XRT Observations and Analysis

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 1021 cm-2, at a redshift of 0.151, in addition to the Galactic value of 5.4 x 1021 cm-2 (Willingale et al. 2013). The PC mode spectrum has a photon index of 1.79 (+0.20, -0.19) and a best-fitting absorption column of 7.6 (+2.9, -2.6) x 1021 cm-2. The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 6.2 x 10-11 (1.1 x 10-10) erg cm-2 count-1.

A summary of the PC-mode spectrum is thus:
Galactic foreground: 5.4 x 1021 cm-2
Intrinsic column: 7.6 (+2.9, -2.6) x 1021 cm-2 at z=0.151
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.

4. UVOT Observations and Analysis

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 EB-V of 1.563 mag. in the direction of the GRB (Schlegel et al. 1998).

BAT light curve

Figure 1. The BAT mask-weighted light curve in the four individual and total energy bands. The units are counts s-1 illuminated-detector-1. The vertical green dash-dotted lines show the T50 interval, the vertical black dashed lines show the T90 interval, and vertical blue (orange) solid lines show the start (stop) of slews.

XRT light curve

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
19h13m03.48s +19°46'24.6" 0.61" UVOT GCN Circ. 32632
19h13m03.43s +19°46'16.3" 5.6" XRT ?
19h13m00.9s +19°48'34.1" 2.4' BAT-refined Krimm et al. GCN Circ. 32688

Table 1. Positions from the Swift instruments.

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 Emax=7.8 GeV
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 Epeak=375±87 keV
T90=327 seconds
Fluence=2.12±0.05x10-5erg cm-2
(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 Epeak=975 (-332,+712) keV
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 Epeak=375±87 keV
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

Table 2. Summary of GCN Circulars from other observatories sorted by band and then circular number.

Filter Tstart(s) Tstop(s) 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