Back to Main Page
Observation Date (UT) Observation Lat

Canonical Name:GRB 221009A
TeVCat Name:TeV J1913+198
Other Names:Swift J1913.1+1946
Source Type:GRB
R.A.:19 13 03 (hh mm ss)
Dec.:+19 48 09 (dd mm ss)
Gal Long: 52.98 (deg)
Gal Lat: 4.34 (deg)
Distance: z=0.151
Flux: (Crab Units)
Energy Threshold: GeV
Spectral Index:
Extended:No
Discovery Date:2022-10
Discovered By: LHAASO
TeVCat SubCat:Default Catalog

Source Notes:

Detection Details:

The detection of VHE emission from this GRB was announced in GCN Circular
by Huang et al. on behalf of the LHAASO Collaboration (2022):
- "GRB 221009A is detected by LHAASO-WCDA at energy above 500 GeV,
centered at RA = 288.3, Dec = 19.7 within 2000 seconds after T0, with
the significance above 100 s.d., and is observed as well by
LHAASO-KM2A with the significance about 10 s.d., where the energy of
the highest photon reaches 18 TeV."

This represents the first detection of photons above 10 TeV from GRBs.

More details on this GRB can be found here.

Important information about the Fermi LAT data can be found here.

Source Position:
The position given in TeVCat was reported by Dichiara et al. (2022):
- R.A. (J2000): 19h 13m 03s
- Dec. (J2000): +19d 48' 09"

Distance:

The redshift given in TeVCat was reported by de Ugarte Postigo et al. (2022):
- "We detect a very red continuum with absorption features that
correspond to CaII, CaI and NaID at a redshift of z = 0.151. We also
detect multiple features due to the Milky Way’s interstellar medium,
due to the large Galactic column density of material along this line
of sight. At this redshift the event has an isotropic equivalent
energy of Eiso=2x10^54 erg (using the GBM fluence reported in GCN 32642),
barring saturation effects in the Fermi/GBM fluence. This is within
the upper end of GRB energetics. Further follow-up is strongly
encouraged."

Classification:
From Veres et al. on behalf of the Fermi GBM Team (2022):
- "The GBM light curve consists of an initial ~10 s long pulse,
followed by an extraordinarily bright episode at ~180 s after the
trigger time, lasting at least 100 seconds."

Spectral Properties:

From Pillera et al. on behalf of the Fermi-LAT Team (2022):
- "The 100 MeV - 1 GeV photon flux in the time interval 200-800 s
after the GBM trigger is (6.2 +/- 0.4)E-03 ph/cm2/s. The estimated
photon index above 100 MeV is -1.87 +/- 0.04."

Temporal Properties:
From Pillera et al. on behalf of the Fermi-LAT Team (2022):
- "The LAT lightcurve shows a bright structured emission episode which
is temporally coincident with the GBM main emission episode starting
at T0+200s."

Energetics:

From Huang et al. on behalf of the LHAASO Collaboration (2022):
- "GRB 221009A is detected by LHAASO-WCDA at energy above 500 GeV,
centered at RA = 288.3, Dec = 19.7 within 2000 seconds after T0, with
the significance above 100 s.d., and is observed as well by
LHAASO-KM2A with the significance about 10 s.d., where the energy of
the highest photon reaches 18 TeV."

From Pillera et al. on behalf of the Fermi-LAT Team (2022):
- "The highest-energy photon is 99.3 GeV (with a probability of 99.2%)
which is observed 240 seconds after the GBM trigger. This represents
the highest GRB photon energy ever detected by Fermi-LAT (the previous
record holder being a 95 GeV event from GRB 130427A)."


Seen by: LHAASO
Want a reference added? Send a bibtex entry to the TeVCat Team