2026-09-05 15:47:04 UTC
JD 2461289.16
STATION 04 · MULTI-MESSENGER WIRE DOSSIER Gamma-Ray Burst CONFIRMED

GRB 221009A

“"The BOAT": Brightest Of All Time 18-TeV Cosmological Monster”
Fermi GBM, Swift BAT & LHAASO Trigger: 2022-10-09 13:16:59 UTC
ASTROPHYSICAL LOCALIZATION & TELEMETRY
FRAME: ICRS / J2000
Sky Coordinates 19h 13m 03.5s +19° 48' 35" (288.26458°, 19.80972°)
Cosmological Redshift z = 0.1510 Luminosity Dist: 2.4 Billion ly (z = 0.151)
Constellation / Field Sagitta Host Field Environment
Detection Significance Historical BOAT (> 50σ trigger) Multi-detector confidence
t90 duration
327 seconds (Ultra-long collapsar)
fluence 10 1000kev
0.021 erg cm⁻² (Highest ever measured)
isotropic energy
~1.2 × 10^55 erg
max photon energy
18 TeV (LHAASO detection)
afterglow mag
Peak V ~ 14.5 (Visible in amateur telescopes)
progenitor
Collapsar (Supernova SN 2022xiw)

01 Scientific Overview & Source Physics

GRB 221009A was an unprecedented, once-in-10,000-years cosmological blast. Emitting an isotropic-equivalent energy E_iso exceeding 10^55 ergs, the burst completely saturated space-based detectors, perturbed Earth's ionosphere at 500 km altitude, and generated the highest-energy photon ever observed from a GRB: a staggering 18 TeV photon detected by LHAASO in China.

02 Multi-Messenger Follow-Up Campaign Matrix

Observatory / Instrument Spectral Regime Observational Detection & Counterpart Findings
JWST (NIRSpec / MIRI)
Infrared (1–25 µm)
Spectroscopically confirmed associated Type Ic core-collapse supernova SN 2022xiw at day 168.
LHAASO Water Cherenkov
Very High Energy (0.2–18 TeV)
Recorded ~5000 high-energy photons; observed early afterglow rise and jet break.
ALMA
Millimeter (100 GHz)
High-precision reverse-shock millimeter synchrotron detection.