GCN Circulars
GCN Circulars are rapid astronomical bulletins submitted by and distributed to community members worldwide. They are used to share discoveries, observations, quantitative near-term predictions, requests for follow-up observations, or future observing plans related to high-energy, multi-messenger, and variable or transient astrophysical events. See the documentation for help with subscribing to or submitting Circulars.
To navigate to a specific circular, enter the associated Circular ID (e.g. 'gcn123', 'Circular 123', or '123').
33 results found.
- GRB 221009A: Determination of the black holes mass and spin
- GRB 221009A: Peak luminosity of the supernova vs. synchrotron afterglow
- GRB 221009A X-ray light-curve and the indication of TeV light-curve
- GMRT radio detection of GRB 180720B
- GRB 180720B: CALET Gamma-Ray Burst Monitor detection
- NuSTAR observations of GRB 180720B
- GRB 180720B: OAJ optical observations
- GRB 180720B: AMI-LA 15.5 GHz observation
- GRB 180720B long follow up requested
- GRB 180720B: KAIT Optical Observations
- GRB 180720B: D50 optical observations
- GRB 180720B: MASTER Global Net OT observations
- GRB 180720B: REM photometry
- GRB 180720B: ISON-Castelgrande optical observations
- GRB 180720B: Testing the universality of the newly born neutron star in BdHNe
- GRB 180720B: COATLI Optical Detection
- Konus-Wind observation of GRB 180720B
- GRB 180720B: MITSuME Ishigaki optical observations
- GRB 180720B: Swift-BAT refined analysis
- GRB 180720B: VLT/X-shooter redshift
- GRB 180720B: MAXI/GSC detection
- GRB 180720B: LCO optical afterglow observations
- GCN 22984 was for GRB 180720B
- GRB 180720B: OSN detection, fading slower?
- GRB 180720B: Swift-XRT refined Analysis
- GRB 180720B: MITSuME Akeno optical observations
- GRB 180720B: Fermi GBM observation
- GRB 180720B : Fermi-LAT detection
- GRB 180720B : TSHAO optical observations
- GRB 180720B: Kanata 1.5m optical/NIR observation
- GRB 180720B: LCO Haleakala possible bright optical candidate
- Correction: Swift trigger #848890 is GRB 180720B (not GRB 180720A)
- GRB 180720B: Swift detection of a burst