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').
Advanced Search
To narrow the search results, use advanced search syntax. This allows for specifying which circular field to search (submitter, subject, and/or body). For additional information, refer to the advanced search documentation.
Advanced Search Examples (click to copy):
subject:"Swift"body:"GRB"submitter:"Judith Racusin"- Fermi418277210: iPTF optical observations
- GRB 140408A: RATIR Optical Upper Limits
- GRB 140408A: Swift-BAT refined analysis
- GRB 140408A: GROND Detection of an Afterglow Candidate
- GRB 140408A: Swift/UVOT Upper Limits
- GRB 140408A: Swift-XRT refined Analysis
- GRB 140408A: MITSuME Okayama upper limits
- GRB 140408A: Enhanced Swift-XRT position
- GRB 140408A: Fermi GBM detection
- Swift Trigger 595162: a possible GRB
- GRB 140408A: Swift detection of a burst
- GRB 140406A: Fermi GBM observation
- GRB 140402A: Deep limit on the optical afterglow from Magellan observations
- GRB 111225A: Archeological redshift of the Christmas Burst 2011 from GTC
- GRB 140402A: Swift/UVOT Upper Limits
- GRB 140331A: Continued RATIR Optical and NIR Observations
- GRB 140402A: Swift-XRT observations
- GRB 140402A: MASTER optical observations
- GRB 140402A BAT refined analysis
- GRB 140402A : Xinglong TNT upper limit
- GRB 140402A: Marginal BAT detection
- GRB 140402A: Fermi GBM detection
- GRB 140402A: Fermi-LAT detection of a burst
- Swift trigger 594286: Is likely a noise trigger
- GRB 140219A: Correction to GCN 15885 (Suzaku-WAM fluence)
- GRB 140330A: Fermi GBM observation
- GRB 140331A: Swift-XRT refined Analysis
- GRB 140301A: Zadko observatory - Gingin optical observations
- GRB 140331A: Swift-BAT refined analysis
- Retraction of the Fermi/LAT high-energy counterpart for GRB 140330A
- GRB 140331A: Swift/UVOT Upper Limits
- GRB 140302A: TAROT La Silla observatory optical observations
- GRB 140323A: Zadko observatory - Gingin optical observations
- GRB 140330A: intense and persistent gamma-ray emission detected by AGILE
- GRB 140331A: Zadko observatory - Gingin optical observations
- Konus-Wind observation of GRB 140330A
- GRB 140129B: AAO optical upper limit
- GRB 140129A: Mondy optical observations
- GRB 140331A: MITSuME Okayama upper limits
- GRB 140331A: Enhanced Swift-XRT position
- IPN triangulation of GRB 130330A
- GRB 140331A: RATIR Optical and NIR Observations
- GRB 140331A: Swift detection of a burst
- GRB 140330A: Fermi-LAT Detection
- GRB 140329A: Fermi-LAT detection
- Konus-Wind observation of GRB 140329A
- IPN Triangulation of GRB 140329A
- MAXI ID=745548350 is UV Ceti
- GRB 140320D: MASTER optical observations
- GRB 140329A: Fermi GBM observation of a bright burst
- Swift trigger 593744: detection of a flare from UV Cet
- GRB 140320D: Suzaku WAM observation of the prompt emission
- GRB 140323A : Suzaku WAM observation of the prompt emission
- Fermi Gamma-ray Burst Monitor trigger 417486540 / 140326020 is not a GRB
- GRB 140226A/iPTF14yb: Mondy optical observations
- GRB 140320C: Mondy optical observations and afterglow confirmation
- Konus-Wind observation of GRB 140323A
- GRB 140323A: Fermi-LAT detection
- GRB 140323A: Swift-XRT refined Analysis
- GRB 140323A: Fermi GBM observation
- GRB 140323A: BOOTES-3 optical upper limit.
- GRB 140323A: Swift/UVOT Upper Limits
- GRB 140323A: Swift-BAT refined analysis
- GRB 140323A: Enhanced Swift-XRT position
- GRB 140323A: Swift detection of a burst
- GRB 140320A: RATIR Optical and NIR Observations
- Konus-Wind observation of GRB 140320D
- GRB 140320B: P60 detection of a very red afterglow
- IPN Triangulation of very intense GRB 140320D
- GRB 140320C: Mini-GWAC prompt observation
- GRB 140320C: Swift/UVOT Upper Limits
- GRB 140320A: Swift-BAT refined analysis
- GRB 140320B: Swift/UVOT Upper Limits
- GRB 140320A: Swift/UVOT Upper Limits
- GRB 140320C: Swift-XRT observations
- GRB 140320A: Confirmation of a fading X-ray afterglow
- GRB 140320C: Swift-XRT detection of the X-ray afterglow
- GRB 140320A: Fermi GBM detection
- GRB 140320B: Swift-XRT detection of the afterglow
- GRB 140320C: Mondy optical observations
- GRB 140320A: Enhanced Swift-XRT position
- GRB 140320A: Swift-XRT detection of an afterglow candidate
- GRB 140320C: MASTER optical observations
- GRB 140320C: FTN optical observations
- GRB 140320C: A long GRB detected by INTEGRAL
- GRB 140320B: Xinglong TNT upper limit
- GRB 140320B: ISON-NM optical observations
- GRB 140320B: A long GRB detected by INTEGRAL
- GRB 140320B: FTN optical afterglow candidate
- Swift Trigger 592558 is not an astrophysical source
- GRB 140320A: Fermi GBM observations suggest a short GRB
- GRB 140320A: Swift detection of a burst
- GRB 140318A: Continued RATIR Optical and NIR Observations
- GRB 140318A: Mondy optical limit
- GRB 140318A: Swift/UVOT Upper Limits
- GRB 140318A: Swift-BAT refined analysis
- GRB 140311B: Mondy optical limit
- GRB 140311A: Mondy optical limits
- GRB 140318A: Swift-XRT refined Analysis
- GRB 140318A: Liverpool Telescope optical observations